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Sangeang Api

Photo of this volcano
  • Country
  • Volcanic Region
  • Landform | Volc Type
  • Last Known Eruption
  • 8.2°S
  • 119.07°E

  • 1,912 m
    6,273 ft

  • 264050
  • Latitude
  • Longitude

  • Summit
    Elevation

  • Volcano
    Number

Most Recent Weekly Report: 16 February-22 February 2022 Citation IconCite this Report

The Darwin VAAC reported that on 17 February ash plumes from Sangeang Api rose to altitudes of 4-4.9 km (13,000-16,000 ft) a.s.l. and drifted SW and WSW. The Alert Level remained at 2 (on a scale of 1-4).

Sources: Darwin Volcanic Ash Advisory Centre (VAAC), Pusat Vulkanologi dan Mitigasi Bencana Geologi (PVMBG, also known as CVGHM)


Most Recent Bulletin Report: March 2022 (BGVN 47:03) Citation IconCite this Report

Small ash plume on 17 February 2022

Sangeang Api is a complex volcano on the small island of Sangeang in the Lesser Sunda Islands, Indonesia, consisting of two volcanic cones. After a major explosion in May 2014, activity continued until November 2015, with thermal anomalies indicating possible lava dome growth or lava flows (BGVN 39:02 and 41:10). Another eruptive period during July 2017 into June 2020 included occasional weak ash explosions with ash plumes and emissions, hot material discharged from the summit crater, periods of numerous thermal anomalies, summit incandescence, and infrequent Strombolian activity (BGVN 42:09, 43:11, 44:05, 45:02, and 45:08). The volcano is monitored by Pusat Vulkanologi dan Mitigasi Bencana Geologi (PVMBG, or CVGHM), the Darwin Volcanic Ash Advisory Center (VAAC), and by various satellites.

The only documented activity during August 2020-February 2022 was an ash plume on 17 February 2022 reported by the Darwin VAAC that rose to an altitude of 4-4.9 km (~3 km above the summit) and drifted SW and WSW. During August 2020-February 2022, Sentinel-2 satellite images during this time were usually obscured by weather clouds, but no thermal signals or volcanic activity were observed when there were clear views. During May 2021 through February 2022, the MIROVA (Middle InfraRed Observation of Volcanic Activity) volcano hotspot detection system recorded ten scattered hotspots within 5 km of the summit; the cause of the weak anomalies is unknown.

Information Contacts: Pusat Vulkanologi dan Mitigasi Bencana Geologi (PVMBG, also known as Indonesian Center for Volcanology and Geological Hazard Mitigation, CVGHM), Jalan Diponegoro 57, Bandung 40122, Indonesia (URL: http://www.vsi.esdm.go.id/); Darwin Volcanic Ash Advisory Centre (VAAC), Bureau of Meteorology, Northern Territory Regional Office, PO Box 40050, Casuarina, NT 0811, Australia (URL: http://www.bom.gov.au/info/vaac/); MIROVA (Middle InfraRed Observation of Volcanic Activity), a collaborative project between the Universities of Turin and Florence (Italy) supported by the Centre for Volcanic Risk of the Italian Civil Protection Department (URL: http://www.mirovaweb.it/); Sentinel Hub Playground (URL: https://www.sentinel-hub.com/explore/sentinel-playground).

Weekly Reports - Index


2022: February
2020: January | May | June
2019: June | July | August | September | October | November | December
2018: May | October
2017: July | August
2015: July | November
2014: May | June
2013: May | June
2012: October | December
2009: June


16 February-22 February 2022 Citation IconCite this Report

The Darwin VAAC reported that on 17 February ash plumes from Sangeang Api rose to altitudes of 4-4.9 km (13,000-16,000 ft) a.s.l. and drifted SW and WSW. The Alert Level remained at 2 (on a scale of 1-4).

Sources: Darwin Volcanic Ash Advisory Centre (VAAC); Pusat Vulkanologi dan Mitigasi Bencana Geologi (PVMBG, also known as CVGHM)


10 June-16 June 2020 Citation IconCite this Report

The Darwin VAAC reported that on 10 June an ash plume from Sangeang Api rose to an altitude of 3 km (10,000 ft) a.s.l. and drifted NE. The Alert Level remained at 2 (on a scale of 1-4).

Sources: Pusat Vulkanologi dan Mitigasi Bencana Geologi (PVMBG, also known as CVGHM); Darwin Volcanic Ash Advisory Centre (VAAC)


6 May-12 May 2020 Citation IconCite this Report

The Darwin VAAC reported that on 10 May a discrete ash emission from Sangeang Api rose to an altitude of 2.1 km (7,000 ft) a.s.l. and drifted E. The Alert Level remained at 2 (on a scale of 1-4).

Sources: Darwin Volcanic Ash Advisory Centre (VAAC); Pusat Vulkanologi dan Mitigasi Bencana Geologi (PVMBG, also known as CVGHM)


22 January-28 January 2020 Citation IconCite this Report

The Darwin VAAC reported that on 23 January an ash emission from Sangeang Api rose to an altitude of 3 km (10,000 ft) a.s.l. and drifted NNE. The Alert Level remained at 2 (on a scale of 1-4).

Sources: Darwin Volcanic Ash Advisory Centre (VAAC); Pusat Vulkanologi dan Mitigasi Bencana Geologi (PVMBG, also known as CVGHM)


25 December-31 December 2019 Citation IconCite this Report

The Darwin VAAC reported that during 25-28 December discrete minor ash emissions from Sangeang Api rose to altitudes of 2.4-3 km (8,000-10,000 ft) a.s.l. and drifted W, SW, and E. The Alert Level remained at 2 (on a scale of 1-4).

Source: Darwin Volcanic Ash Advisory Centre (VAAC)


18 December-24 December 2019 Citation IconCite this Report

The Darwin VAAC reported that during 18-19 December discrete minor ash emissions from Sangeang Api rose to an altitude of 2.4 km (8,000 ft) a.s.l. and drifted W. The Alert Level remained at 2 (on a scale of 1-4).

Source: Darwin Volcanic Ash Advisory Centre (VAAC)


11 December-17 December 2019 Citation IconCite this Report

The Darwin VAAC reported that during 11-13 and 17 December discrete ash emissions from Sangeang Api rose to an altitude of 2.4 km (8,000 ft) a.s.l. and drifted NW and W. A thermal anomaly was visible on 27 November. The Alert Level remained at 2 (on a scale of 1-4).

Source: Darwin Volcanic Ash Advisory Centre (VAAC)


4 December-10 December 2019 Citation IconCite this Report

The Darwin VAAC reported that during 4-5 and 7-9 December discrete ash emissions from Sangeang Api rose to an altitude of 2.4 km (8,000 ft) a.s.l. and drifted NW, W, and SW. A thermal anomaly was visible on 27 November. The Alert Level remained at 2 (on a scale of 1-4).

Source: Darwin Volcanic Ash Advisory Centre (VAAC)


27 November-3 December 2019 Citation IconCite this Report

The Darwin VAAC reported that during 27 November-3 December discrete and short-lived ash emissions from Sangeang Api rose to altitudes of 2.4-3.3 km (8,000-11,000 ft) a.s.l. and drifted NW, W, and SW. A thermal anomaly was visible on 27 November. The Alert Level remained at 2 (on a scale of 1-4).

Source: Darwin Volcanic Ash Advisory Centre (VAAC)


20 November-26 November 2019 Citation IconCite this Report

The Darwin VAAC reported that during 20-26 November discrete and short-lived ash emissions from Sangeang Api rose to 2.4 km (8,000 ft) a.s.l. and drifted SW and W. The Alert Level remained at 2 (on a scale of 1-4).

Source: Darwin Volcanic Ash Advisory Centre (VAAC)


13 November-19 November 2019 Citation IconCite this Report

The Darwin VAAC reported that during 14-19 November discrete and short-lived ash emissions from Sangeang Api rose to 2.4 km (8,000 ft) a.s.l. and drifted NW and W. Thermal anomalies were recorded at least during 18-19 November. The Alert Level remained at 2 (on a scale of 1-4).

Source: Darwin Volcanic Ash Advisory Centre (VAAC)


6 November-12 November 2019 Citation IconCite this Report

The Darwin VAAC reported that during 6-12 November discrete and short-lived ash emissions from Sangeang Api rose to 3 km (10,000 ft) a.s.l. and drifted NW, W, and SW. Thermal anomalies were visible during 6-8 November. The Alert Level remained at 2 (on a scale of 1-4).

Source: Darwin Volcanic Ash Advisory Centre (VAAC)


30 October-5 November 2019 Citation IconCite this Report

The Darwin VAAC reported that during 30-31 October and 3-4 November discrete and short-lived ash emissions from Sangeang Api rose 2.7-3.5 km (9,000-11,000 ft) a.s.l. and drifted NW, W, and SW. Thermal anomalies were visible on 3 and 5 November. The Alert Level remained at 2 (on a scale of 1-4).

Source: Darwin Volcanic Ash Advisory Centre (VAAC)


23 October-29 October 2019 Citation IconCite this Report

The Darwin VAAC reported that during 26-28 October multiple discrete ash emissions from Sangeang Api rose to 2.1-2.7 km (7,000-9,000 ft) a.s.l. and dissipated rapidly to the NW, WNW, and W. A thermal anomaly was visible in satellite images on 26 October. The Alert Level remained at 2 (on a scale of 1-4).

Source: Darwin Volcanic Ash Advisory Centre (VAAC)


11 September-17 September 2019 Citation IconCite this Report

The Darwin VAAC reported that on 11 September a diffuse ash plume from Sangeang Api was identified in satellite images rising to 3 km (10,000 ft) a.s.l. and drifting N. The Alert Level remained at 2 (on a scale of 1-4).

Source: Darwin Volcanic Ash Advisory Centre (VAAC)


4 September-10 September 2019 Citation IconCite this Report

The Darwin VAAC reported that during 5-7 September intermittent diffuse ash plumes from Sangeang Api were identified in satellite images rising to 3 km (10,000 ft) a.s.l. and drifting S and SW. The Alert Level remained at 2 (on a scale of 1-4).

Source: Darwin Volcanic Ash Advisory Centre (VAAC)


28 August-3 September 2019 Citation IconCite this Report

The Darwin VAAC reported that during 28 August-3 September intermittent ash plumes from Sangeang Api were identified in satellite images rising to 3 km (10,000 ft) a.s.l. and drifting N, NW, W, and SW. The Alert Level remained at 2 (on a scale of 1-4).

Source: Darwin Volcanic Ash Advisory Centre (VAAC)


21 August-27 August 2019 Citation IconCite this Report

The Darwin VAAC reported that during 21-26 August intermittent ash plumes from Sangeang Api were identified in satellite images rising to 3 km (10,000 ft) a.s.l. and drifting W and WNW. The Alert Level remained at 2 (on a scale of 1-4).

Source: Darwin Volcanic Ash Advisory Centre (VAAC)


14 August-20 August 2019 Citation IconCite this Report

The Darwin VAAC reported that during 14-20 August intermittent ash plumes from Sangeang Api were identified in satellite images rising to 2.4-3 km (8,000-10,000 ft) a.s.l. and quickly dissipating to the N, NW, W, and SW. The Alert Level remained at 2 (on a scale of 1-4).

Source: Darwin Volcanic Ash Advisory Centre (VAAC)


7 August-13 August 2019 Citation IconCite this Report

The Darwin VAAC reported that during 7-13 August ash plumes from Sangeang Api were identified in satellite images rising to 2.4-3 km (8,000-10,000 ft) a.s.l. and drifting in multiple directions. The Alert Level remained at 2 (on a scale of 1-4).

Source: Darwin Volcanic Ash Advisory Centre (VAAC)


31 July-6 August 2019 Citation IconCite this Report

The Darwin VAAC reported that during 31 July-3 August ash plumes from Sangeang Api were identified in satellite images rising to 2.4-3 km (8,000-10,000 ft) a.s.l. and drifting in multiple directions. The Alert Level remained at 2 (on a scale of 1-4).

Source: Darwin Volcanic Ash Advisory Centre (VAAC)


24 July-30 July 2019 Citation IconCite this Report

The Darwin VAAC reported that during 24-30 July multiple ash plumes from Sangeang Api were identified by pilots and in satellite images rising to 2.4-3 km (8,000-10,000 ft) a.s.l. and quickly dissipating N, NW, W, and SW. The Alert Level remained at 2 (on a scale of 1-4).

Source: Darwin Volcanic Ash Advisory Centre (VAAC)


17 July-23 July 2019 Citation IconCite this Report

The Darwin VAAC reported that during 17-18 and 20-22 July ash plumes from Sangeang Api were identified by pilots and in satellite images rising to 2.1-4.6 km (7,000-15,000 ft) a.s.l. and drifting NW, W, and SW. The Alert Level remained at 2 (on a scale of 1-4).

Source: Darwin Volcanic Ash Advisory Centre (VAAC)


10 July-16 July 2019 Citation IconCite this Report

The Darwin VAAC reported that during 10-16 July ash plumes from Sangeang Api were visible in satellite images rising to 2.1-3 km (7,000-10,000 ft) a.s.l. and drifting in multiple directions. The Alert Level remained at 2 (on a scale of 1-4).

Source: Darwin Volcanic Ash Advisory Centre (VAAC)


3 July-9 July 2019 Citation IconCite this Report

The Darwin VAAC reported that during 4-5 July ash plumes from Sangeang Api were visible in satellite images rising to 2.1-2.3 km (7,000-8,000 ft) a.s.l. and drifting SW and W. During 6-9 July multiple ash plumes rose to 3-4.6 km (10,000-15,000 ft) a.s.l. and drifted N, NW, and SW. Thermal anomalies were visible on 4 and 8 July.

Source: Darwin Volcanic Ash Advisory Centre (VAAC)


26 June-2 July 2019 Citation IconCite this Report

The Darwin VAAC reported that on 27 June ash plumes from Sangeang Api rose to 2.1 km (7,000 ft) a.s.l. and drifted NW. A thermal anomaly was also visible. On 29 June a discrete ash puff that rose to 2.4 km (8,000 ft) a.s.l. drifted NW, and steam emissions were ongoing.

Source: Darwin Volcanic Ash Advisory Centre (VAAC)


12 June-18 June 2019 Citation IconCite this Report

The Darwin VAAC reported that on 17 June multiple discrete emissions with increasing ash content over a period of about an hour rose from Sangeang Api to altitudes of 1.2-2.1 (4,000-7,000 ft) a.s.l. and drifted W and WNW, based on satellite images and weather models. A thermal anomaly was also visible. The Alert Level remained at 2 (on a scale of 1-4).

Sources: Darwin Volcanic Ash Advisory Centre (VAAC); Pusat Vulkanologi dan Mitigasi Bencana Geologi (PVMBG, also known as CVGHM)


10 October-16 October 2018 Citation IconCite this Report

Based on a VONA from PVMBG an ash emission from Sangeang Api was generated at 1338 on 15 October; it rose 250 m above the summit and drifted SW, W, and NW. The VONA noted that the ash emission possibly rose higher than what a ground observer had estimated. Seismic data was dominated by signals indicating emissions as well as local tectonic earthquakes. The Aviation Color Code was changed from Yellow to Orange.

Source: Pusat Vulkanologi dan Mitigasi Bencana Geologi (PVMBG, also known as CVGHM)


9 May-15 May 2018 Citation IconCite this Report

Based on a VONA from PVMBG, on 9 May a gas emission was observed at 1807 from Sangeang Api that rose to 4,150 m (13,000 ft) a.s.l. and drifted west. On 9 May the Aviation Color Code was changed from unassigned to Yellow.

Sources: Darwin Volcanic Ash Advisory Centre (VAAC); Pusat Vulkanologi dan Mitigasi Bencana Geologi (PVMBG, also known as CVGHM)


9 August-15 August 2017 Citation IconCite this Report

Based on analyses of satellite imagery, the Darwin VAAC reported that on 12 August an ash plume from Sangeang Api rose to 2.7 km (9,000 ft) a.s.l. and drifted NW.

Source: Darwin Volcanic Ash Advisory Centre (VAAC)


2 August-8 August 2017 Citation IconCite this Report

Based on analyses of satellite imagery, the Darwin VAAC reported that during 7-8 August minor emissions from Sangeang Api rose 2.4 km (8,000 ft) a.s.l. and drifted WSW.

Source: Darwin Volcanic Ash Advisory Centre (VAAC)


26 July-1 August 2017 Citation IconCite this Report

Based on analyses of satellite imagery, pilot observations, and wind data, the Darwin VAAC reported that during 29-30 July ash plumes from Sangeang Api rose to altitudes of 2.4-2.7 km (8,000-9,000 ft) a.s.l. and drifted NW and W.

Source: Darwin Volcanic Ash Advisory Centre (VAAC)


19 July-25 July 2017 Citation IconCite this Report

Based on analyses of satellite imagery, PVMBG observations, and wind data, the Darwin VAAC reported that during 19-20 July ash plumes from Sangeang Api rose to altitudes of 2.4-4.3 km (8,000-14,000 ft) a.s.l. and drifted NW.

Source: Darwin Volcanic Ash Advisory Centre (VAAC)


12 July-18 July 2017 Citation IconCite this Report

PVMBG reported a small eruption at Sangeang Api at 1154 on 15 July characterized by Strombolian activity, and an ash plume that rose 100-200 m above the crater rim and drifted SW. Prior to the event, thermal anomalies had increased beginning in March, and seismicity had increased starting in April.

Based on analyses of satellite imagery, PVMBG observations, and wind data, the Darwin VAAC reported that on 16 July an ash plume rose to an altitude of 2.1 km (7,000 ft) a.s.l., or 200 m above the crater rim, and drifted NW.

Sources: Pusat Vulkanologi dan Mitigasi Bencana Geologi (PVMBG, also known as CVGHM); Darwin Volcanic Ash Advisory Centre (VAAC)


4 November-10 November 2015 Citation IconCite this Report

PVMBG reported that observers at the Sangeang Api observation post in Desa Sangeang Darat, Bima, West Nusa Tenggara, reported that during 1 July-30 September diffuse white plumes rose up to 250 m above the crater rim. During 1 October-1 November white-to-gray plumes rose as high as 350 m. Beginning on 23 October occasional weak thumping noises were reported. Crater incandescence possibly indicated lava-dome growth or lava-flow advancement. The Alert Level remained at 2 (on a scale of 1-4); visitors and residents were warned not to approach the crater within a 1.5-km radius.

Source: Pusat Vulkanologi dan Mitigasi Bencana Geologi (PVMBG, also known as CVGHM)


8 July-14 July 2015 Citation IconCite this Report

Based on analyses of satellite imagery and wind data, the Darwin VAAC reported that on 8 July an ash plume from Sangeang Api rose to an altitude of 2.7 km (9,000 ft) a.s.l. and drifted over 35 km SE.

Source: Darwin Volcanic Ash Advisory Centre (VAAC)


1 July-7 July 2015 Citation IconCite this Report

Based on analyses of satellite imagery and wind data, the Darwin VAAC reported that on 7 July an ash plume from Sangeang Api rose to an altitude of 2.7 km (9,000 ft) a.s.l. and drifted over 35 km E.

Source: Darwin Volcanic Ash Advisory Centre (VAAC)


18 June-24 June 2014 Citation IconCite this Report

PVMBG reported seismic and visual monitoring of Sangeang Api during 1-17 June. During clear conditions, incandescence at the summit and white-and-gray plumes (100-1,500 m above the summit) were visible. On 1 June seismicity dramatically decreased, and as of 17 June was still declining. The Alert Level was reduced from 3 to 2 (on a scale of 1-4) on 17 June.

Source: Pusat Vulkanologi dan Mitigasi Bencana Geologi (PVMBG, also known as CVGHM)


11 June-17 June 2014 Citation IconCite this Report

Based on analyses of satellite imagery and wind data, the Darwin VAAC reported that on 14 June an ash plume from Sangeang Api rose to an altitude of 2.1 km (7,000 ft) a.s.l. and drifted 55 km NW.

Source: Darwin Volcanic Ash Advisory Centre (VAAC)


4 June-10 June 2014 Citation IconCite this Report

Based on analyses of satellite imagery and wind data, the Darwin VAAC reported that during 4-7 June ash plumes from Sangeang Api rose to an altitude of 3 km (10,000 ft) a.s.l. and drifted 45-110 km W and NW.

Source: Darwin Volcanic Ash Advisory Centre (VAAC)


28 May-3 June 2014 Citation IconCite this Report

PVMBG reported that during January-29 May diffuse white plumes rose at most 25 m above Sangeang Api's crater. On 30 May seismicity increased, with tremor starting at 0500 and becoming continuous at 1348. An eruption at 1555 generated an ash plume that rose 3 km and drifted W, causing ashfall over the sea. The Alert Level was raised to 3 (on a scale of 1-4). The island has no permanent settlements, and is only occupied during the growing and harvest seasons; civil authorities evacuated 135 people to the mainland. Based on satellite images, pilot observations, and the Indonesian Meteorological Office, the Darwin VAAC reported that on 30 May an ash plume rose to an altitude of 15.2 km (50,000 ft) a.s.l. and drifted 440 km E and 750 km SE.

BNPB reported that on 31 May two larger explosions occurred at 1330 and 2242. According to the VAAC, ash plumes from those explosions rose to altitudes of 13.7-15.2 km (45,000-50,000 ft) a.s.l. and drifted 280 km NW and other various directions. Later in the day the ash plumes became detached. Ashfall affected many areas in the Bima Regency on the mainland, including Wera, and prompted the evacuation of 7,328 people from four villages within a radius of 8 km from Sangeang Api. The Bima and Tambolaka airports were temporarily closed. According to a news article, all flights to and from the Darwin International Airport in Australia on 31 May were canceled.

The VAAC noted that ash plumes rose to an altitude of 4.3 km (14,000 ft) a.s.l. on 1 June and drifted W and SW. During 2-3 June ash plumes rose to altitudes of 3-4.3 km (10,000-14,000 ft) a.s.l. and drifted 45 km W.

Sources: Pusat Vulkanologi dan Mitigasi Bencana Geologi (PVMBG, also known as CVGHM); Badan Nacional Penanggulangan Bencana (BNPB); Darwin Volcanic Ash Advisory Centre (VAAC); The Guardian News


12 June-18 June 2013 Citation IconCite this Report

CVGHM reported that during May through 13 June diffuse white plumes rose 10 m above Sangeang Api's crater. Both the lava dome and surrounding areas showed no changes since November 2012. The Alert Level had been increased to 3 (on a scale of 1-4) on 19 May due to a trend of increasing seismicity; as many as 77 shallow earthquakes and 66 deep earthquakes had been detected daily. Residents and tourists were advised to stay away from the craters within a radius of 5 km. Since then seismicity decreased; 15 shallow earthquakes and three deep earthquakes were recorded on 13 June. The Alert Level was lowered to 2 on 14 June. The public were advised not to approach the craters within a radius of 1.5 km.

Source: Pusat Vulkanologi dan Mitigasi Bencana Geologi (PVMBG, also known as CVGHM)


15 May-21 May 2013 Citation IconCite this Report

CVGHM reported that during 1-19 May diffuse white plumes rose 10 m above Sangeang Api's crater. Both the lava dome and surrounding areas showed no changes since November 2012. Seismicity had increased on 26 April and remained high. The Alert Level was raised to 3 (on a scale of 1-4) on 19 May. Residents and tourists were advised not to approach the craters within a radius of 5 km.

Source: Pusat Vulkanologi dan Mitigasi Bencana Geologi (PVMBG, also known as CVGHM)


26 December-1 January 2013 Citation IconCite this Report

CVGHM reported that during November through mid-December observers at the Sangeang, Bima observation post (50 km SW) noted occasional diffuse white plumes rising 5-15 m above Sangeang Api's crater. The lava dome and surrounding areas had not changed compared to October observations. Avalanches had occurred on the W and SW flanks. Earthquakes had declined. The Alert Level was lowered to 2 (on a scale of 1-4) on 21 December.

Source: Pusat Vulkanologi dan Mitigasi Bencana Geologi (PVMBG, also known as CVGHM)


10 October-16 October 2012 Citation IconCite this Report

CVGHM reported that during 1-10 October Sangeang Api was often not visible due to fog; occasionally plumes were visible and rose as high as 20 m above the crater. The lava dome and surrounding areas had not changed compared to the beginning of the year. Both the number and magnitude of earthquakes increased on 5 October, declined during 6-8 October, then again increased on 9 October. The Alert Level was raised to 3 (on a scale of 1-4) on 10 October.

Source: Pusat Vulkanologi dan Mitigasi Bencana Geologi (PVMBG, also known as CVGHM)


3 June-9 June 2009 Citation IconCite this Report

CVGHM reported that on 4 June the Alert Level for Sangeang Api was raised to 2 (on a scale of 1-4) due to recent increases in the number of earthquakes. White plumes rose 5-25 m during 1 May-3 June.

Source: Pusat Vulkanologi dan Mitigasi Bencana Geologi (PVMBG, also known as CVGHM)


Bulletin Reports - Index

Reports are organized chronologically and indexed below by Month/Year (Publication Volume:Number), and include a one-line summary. Click on the index link or scroll down to read the reports.

07/1985 (SEAN 10:07) Explosions eject tephra, lava flow; island evacuated

08/1985 (SEAN 10:08) Eruption declines; 4.5 km lava flow

09/1985 (SEAN 10:09) 30 July eruption plume seen on satellite images

10/1985 (SEAN 10:10) Lava advance stops; fewer and smaller explosions

11/1985 (SEAN 10:11) Strombolian explosions; lava flow in growing channel; pyroclastic flow deposit

12/1985 (SEAN 10:12) Summit explosions in July and December

01/1986 (SEAN 11:01) Continued gas explosions and lava ejection

03/1986 (SEAN 11:03) Small explosions increase slightly

04/1986 (SEAN 11:04) Continued small explosions; glow

05/1986 (SEAN 11:05) Explosions and lava flow advance continue

06/1986 (SEAN 11:06) Explosions and crater glow continue

07/1986 (SEAN 11:07) Ash clouds; red glow above crater

09/1986 (SEAN 11:09) Fewer explosions

10/1986 (SEAN 11:10) Explosions continue

11/1986 (SEAN 11:11) Numerous explosions

12/1986 (SEAN 11:12) Small explosions but no seismicity

02/1987 (SEAN 12:02) Frequent small gas explosions

03/1987 (SEAN 12:03) Small gas explosions continue

04/1987 (SEAN 12:04) About 50 small explosions daily

06/1987 (SEAN 12:06) Frequent explosions continue

07/1987 (SEAN 12:07) Activity continues; plumes to 600 m

08/1987 (SEAN 12:08) Small explosions continue

09/1987 (SEAN 12:09) Small explosions continue

10/1987 (SEAN 12:10) Fewer explosions

12/1987 (SEAN 12:12) Eruptive activity continues at steady rate

02/1988 (SEAN 13:02) Explosions and earthquakes end

05/1999 (BGVN 24:05) March to May plumes are thin and rise to 150 m above the summit

07/2009 (BGVN 34:07) Increased seismicity, including explosion earthquakes, during May-June 2009

12/2009 (BGVN 34:12) Explosive eruptions during 1997-1999 were previously unreported

07/2013 (BGVN 38:07) Fumarolic emissions and variable seismicity during 2012-2013

02/2014 (BGVN 39:02) Ashfall from 30 May 2014 eruption causes evacuations, airline delays

10/2016 (BGVN 41:10) Large explosions in May 2014 followed by thermal anomalies until early November 2015

09/2017 (BGVN 42:09) Weak Strombolian activity and occasional weak ash plumes, 15 July-12 August 2017

11/2018 (BGVN 43:11) Ongoing crater activity and thermal anomalies during September 2017-October 2018

05/2019 (BGVN 44:05) Ongoing frequent explosions with ash plumes, Strombolian activity, and block avalanches, November 2018-April 2019

02/2020 (BGVN 45:02) Ash emissions and lava flow extrusion continue during May 2019 through January 2020

08/2020 (BGVN 45:08) Two ash plumes and small thermal anomalies during February-June 2020

03/2022 (BGVN 47:03) Small ash plume on 17 February 2022




Information is preliminary and subject to change. All times are local (unless otherwise noted)


July 1985 (SEAN 10:07) Citation IconCite this Report

Explosions eject tephra, lava flow; island evacuated

"Sangeang Api . . . began to erupt on 30 July, with a series of explosions from the summit crater (Doro Api). The first explosion occured at about 0900 and produced a plume of tephra and gas to about 3,500 m altitude. Additional explosions occurred at 1130 (6,500 m), 1320 (6,500 m), and 1800 (1,500 m). Ashfall in Bima (50 km SW of the volcano), the capital of Sumbawa, totaled about 2 mm, and ashfall along the NE coast of Sumbawa, in the vicinity of the village of Wera, totaled about 2 cm. Between 30 July and 1 August, the 1,242 inhabitants of Sangeang Api island were evacuated to Sumbawa. Numerous additional Vulcanian explosions took place during the following week, reaching a maximum altitude of 2,500 m. Poor weather prevented systematic observations 1-5 August. On 6 August at 1939, a 0.7-km-long aa flow was observed advancing W from the region of Doro Api crater, toward the village of Doro Sangeang. By 9 August, the flow was 1.7 km long.

"The most recent eruption of Sangeang Api was in 1966; earlier eruptions occurred in 1512, 1715, 1821, 1860, 1911, 1912, 1927, 1953, [1954-1958 (six eruptions)], and 1964. Typical activity begins with strong Vulcanian explosions followed within a few days by Strombolian explosions. Eruptions in 1953 and 1964 ended with a lava flow and weak Strombolian explosions. Lavas from Sangeang Api are of basaltic composition (49-51% SiO2)."

Information Contacts: VSI.


August 1985 (SEAN 10:08) Citation IconCite this Report

Eruption declines; 4.5 km lava flow

"Sangeang Api continued to erupt in early September. Activity consisted of a single lava flow that has moved approximately 4.5 km W from Doro Api. The frequency of explosions has declined steadily from ~150/day in early August to ~50/day in early September. The maximum explosion cloud height was ~1 km. From 9 to 14 August, the number of small (M < 1) shallow volcanic earthquakes ranged from 190-400/day. By 6-11 September the number of volcanic earthquakes had decreased to 12-40/day."

"A gas plume has been continuously emitted from the volcano since activity began on 30 July. In late August, the gas plume rose less than 0.5 km and was carried W by steady winds. The plume was translucent with a bluish gray to bluish white color. The larger explosions contributed dark gray clouds of fine tephra to the plume. Its SO2 content was in the range of 50-100 metric tons/hour when measured on 23 August."

"The evacuation of the approximately 1,250 inhabitants from Sangeang Island was completed in early August. Inhabitants are in the process of moving their homes to Sumbawa Island."

Information Contacts: J. Matahelumual and T. Casadevall, VSI.


September 1985 (SEAN 10:09) Citation IconCite this Report

30 July eruption plume seen on satellite images

GMS images showed plumes from the initial 30 July activity (figure 1). Digital data analyses of temperatures at the tops of the plumes compared with radiosonde altitude profiles suggested that they reached a maximum altitude of 14.1 km (table 1), below the tropopause. However, Yosihiro Sawada notes that for both this and other eruptions, altitudes calculated with this technique seem to be consistently higher than estimates from ground observers.

Figure (see Caption) Figure 1. Surface temperatures (in °C) of eruption clouds from Sangeang Api (left), 30 July 1985, 1400 (top) and 1700 (bottom) Zones of plume surface from Sangeang Api (right) with temperatures less than 10°C on 30 July at 1400, 1700, 1830, and 2000. Courtesy of Yosihiro Sawada.

Table 1. Sangeang Api eruption cloud data from GMS satellite images on 30 July 1985. Maximum altitude of the eruption cloud is estimated by comparing the GMS digital temperature data with temperature/altitude data profiles from nearby radiosondes. No plume was evident on the image returned at 1100. A plume could be detected from 30 July at 1400 until 31 July at 0200, but none was visible 3 hours later. Maximum plume extent was reached at 1900.

Date Time Length (km) Width (km) Min Temp Max Alt (km) Remarks
30 Jul 1985 1400 135 105 -71°C 14.1 emerging from volcano
30 Jul 1985 1700 315 100 -50°C 11.8 detached from volcano
30 Jul 1985 1800 385 150 -37°C 10.2 detached from volcano
30 Jul 1985 1830 405 160 -30°C 9.4 detached from volcano
30 Jul 1985 1900 425 130 -24°C 8.5 detached from volcano

Information Contacts: Y. Sawada, MRI, Tsukuba.


October 1985 (SEAN 10:10) Citation IconCite this Report

Lava advance stops; fewer and smaller explosions

"Sangeang Api entered into eruption on 30 July. The main features of the activity included an initial phase of mild Vulcanian explosions, followed by Strombolian explosions, a lava flow, and a persistent plume of water vapor and gas. The initial explosions on 30 July were accompanied by a small nuée ardente that followed the drainage of the Sori Kawangge 4 km down the SSW flank to ~200 m altitude, and produced a dark-colored, hornblende-bearing pumice. The eruption has continued through the first week of November but at a greatly reduced level from August. The frequency of explosions has declined steadily from ~150/day in early August to ~50/day in early September and fewer than 6/day in early November. The maximum height of the explosion cloud was ~1 km above the vent in August and

". . . The daily earthquake count shows a steadily decreasing trend, and in early November the number of earthquakes was less than 30/day. The lava flow, first observed on 6 August flowing W from the region of Doro Api crater (toward the village of Doro Sangeang), had advanced to about 4.7 km from the summit by 1 October. The flow showed no additional growth during October."

Photographs taken by astronauts from Space Shuttle mission 61A (30 October-5 November) showed a fairly dense plume extending roughly 50-100 km from Sangeang Api (figure 2).

Figure (see Caption) Figure 2. Space Shuttle photograph (no. 61A-40-062), taken 5 November 1985, showing a plume emerging from Sangeang Api, plus a portion of Sumbawa Island. Note that north is to the left. Courtesy of Charles A. Wood.

Information Contacts: J. Matahelumual, Suparto S., and T. Casadevall, VSI; C. Wood, NASA.


November 1985 (SEAN 10:11) Citation IconCite this Report

Strombolian explosions; lava flow in growing channel; pyroclastic flow deposit

"Sangeang Api continued to erupt with 10-30 Strombolian explosions/day in November and the first week in December. The 1985 lava channel had not lengthened from the 4.7 km observed in late September. However, the volume of the main channel has grown because of a considerable increase in height during the past 2 months. A slow-moving lava flow in the central channel is located atop the main feeder tube. Periodic overflows of this channel add both fluid lava and rubble to the outer flanks of this tube. On 5 December, four separate overflows of fluid lava and rock rubble were observed rolling down the sides of the central channel.

"A brief visit was made to the central crater on 4 December during a period of quiet. The active vent was a large cinder cone in Doro Api Crater. This central cone, which previously rose about 40 m from the floor of Doro Api, was estimated to be approximately 180-200 m above the floor during the 4 December visit. Thundering detonations were heard almost continuously during the 15 minutes spent in the crater and 1 mild Strombolian explosion hurled incandescent blocks. At night, a continuous reddish glow at the bottom of the gas plume over the crater suggested that a small lava lake may exist within Doro Api or the central cone. Fountaining of fluid lava, sheets, or ribbons was observed to accompany some of the larger Strombolian explosions at night.

"We also confirmed the existence of a small-volume pyroclastic flow that was probably produced during the initial activity of 30 July. Local residents reported that the activity caused a number of small fires in the vicinity of Doro Montoy crater (just N of Doro Api) and the Sori Mbere drainage on the S flank of the volcano. A small block and ash flow, still hot to the touch, was found in the Sori Mbere drainage in December. Lahars generated by heavy rainfall and unconsolidated material on the upper slopes of the volcano have been common during and immediately after previous episodes. Outcrops along the shoreline indicate that a number of lahars and possibly also pyroclastic flows have entered the sea. Small mudflows were produced by heavy rains on 2 December. One traveled down the Sori Mbere drainage while a second mudflow entered the sea at Oi Nono Jara on the S side of Sangeang Island.

"This pattern of activity conforms to that of previous 20th century eruptions of Sangeang Api. The 1911 activity included numerous explosions and a lava flow from the summit crater that moved more than 6 km down the W flank. The activity that began in March 1953 produced a lava flow and intermittent explosions through 1954. The 1964 eruption began on 29 January with strong explosions from the 1954 crater, and a lava flow first observed on 3-4 February moved N and E to about 750 m elevation. Explosions and outflow of lava continued for at least several months and possibly until the end of 1965."

Information Contacts: T. Casadevall and L. Pardyanto, VSI.


December 1985 (SEAN 10:12) Citation IconCite this Report

Summit explosions in July and December

"Sangeang Api continued to erupt in December. Compositions of 30 July pumice and mid-August dense lava bombs are given in table 2."

Table 2. Whole rock analyses of samples collected from Sangeang Api. X-ray fluorescence analyses by the USGS Laboratory, Denver, Colorado. Sample 1: pumice from eruption on 30 July 1985. Sample 2: ejected block, dense lava explosion mid-August 1985. Total iron expressed as Fe2O3; loss on ignition at 900°C.

Element Sample 1 (pumice) Sample 2 (block)
SiO2 53.8 49.3
Al2O3 18.9 17.9
Fe2O3 7.23 11.1
MgO 2.51 4.60
CaO 7.30 10.2
Na20 4.33 3.07
K20 3.60 2.40
TiO2 [0.66] 1.03
P2O5 0.38 0.32
MnO 0.22 0.23
LOI 1.09 0.05
Total [100.02] 100.2

Information Contacts: Suparto S. and T. Casadevall, VSI.


January 1986 (SEAN 11:01) Citation IconCite this Report

Continued gas explosions and lava ejection

"Activity started on 30 July [1985] from the main summit crater (Doro Api . . .). At about 0900 a thick plume rose to 3,500 m height. The eruption continued with explosions at 1130 (6,500 m), 1320 (6,500 m) and 1800 (1,500 m). About 2 mm of ash fell in Bima, 50 km SW of the volcano. Between then and 5 August explosions occurred every 30-60 minutes. Black plumes reached 2,000-2,500 m height. On 6 August at 1939 lava was observed flowing W from Doro Api crater. At the end of September the lava flow had advanced ~4,750 m. Numerous explosions took place from September to November, producing columns ~400-500 m high. On 17 November an explosion ejected incandescent lava fragments to ~250 m height and a plume rose to 1,200 m above the crater [see also 10:7-12]. During December and January, gas explosions, sometimes accompanied by ejection of incandescent lava fragments, averaged ~80 events/day. The 1,242 inhabitants of the island were evacuated to the main island of Sumbawa. There were no casualties."

Information Contacts: A. Sudradjat, VSI.


March 1986 (SEAN 11:03) Citation IconCite this Report

Small explosions increase slightly

". . . By comparison with activity in December and January, the frequency of small explosions increased slightly during February and March to ~80/day [but see 11:1]. The height of the eruption clouds averaged ~900 m. Since December 1985, no visits have been made to examine the 1985 lava flow, but continued lava production is suspected."

Information Contacts: Olas, A. Sudradjat, and T. Casadevall, VSI.


April 1986 (SEAN 11:04) Citation IconCite this Report

Continued small explosions; glow

". . . Activity consisted of small explosions with eruption clouds reaching <1 km above the crater. Persistent glow has been observed above the summit crater during the night, suggesting the presence of lava within the crater and in the 1985 lava channel which drains W from the crater."

Information Contacts: Olas, Suratman, Suparto, Kaswanda, and A. Sudradjat, VSI.


May 1986 (SEAN 11:05) Citation IconCite this Report

Explosions and lava flow advance continue

Observers at Sangeang Api reported no changes in the eruption . . . . Several explosions/hour at Doro Api crater and slow growth of the lava flow continued. Only rockfall earthquakes were recorded.

Information Contacts: A. Sudradjat, L. Pardyanto, and T. Casadevall, VSI.


June 1986 (SEAN 11:06) Citation IconCite this Report

Explosions and crater glow continue

The eruption continued through June with several explosions/day that produced clouds reaching ~1 km above the summit. A persistent reddish glow continued to be visible at night above Doro Api crater.

Information Contacts: L. Pardyanto, Olas, Kaswanda, A. Sudradjat, and T. Casadevall, VSI.


July 1986 (SEAN 11:07) Citation IconCite this Report

Ash clouds; red glow above crater

Sangeang Api has been in continuous eruption for a year. Activity in July included several explosions/day, producing eruption clouds . . . ~1 km above the summit. A persistent reddish glow was visible at night above the Doro Api crater.

Information Contacts: L. Pardyanto, Olas, Kaswanda, Suratman, A. Sudradjat, and T. Casadevall, VSI.


September 1986 (SEAN 11:09) Citation IconCite this Report

Fewer explosions

"Explosions from the summit crater decreased in frequency during September."

Information Contacts: L. Pardyanto, Olas, Kaswanda, Suratman, A. Sudradjat, and T. Casadevall, VSI.


October 1986 (SEAN 11:10) Citation IconCite this Report

Explosions continue

Summit explosions . . . were continuing in October.

Information Contacts: Suratman and T. Casadevall, VSI.


November 1986 (SEAN 11:11) Citation IconCite this Report

Numerous explosions

During November >130 explosions were recorded from Dori Api crater. The maximum height of eruption columns was 700 m. Continued extrusion of lava was suspected but not confirmed. No volcanic earthquakes were recorded.

Information Contacts: VSI; ANS.


December 1986 (SEAN 11:12) Citation IconCite this Report

Small explosions but no seismicity

Explosions continued from Doro Api Crater, ranging from 40 to 70/day from December through the first week in January. Maximum plume height was 800 m. No volcanic earthquakes were recorded.

Information Contacts: VSI.


February 1987 (SEAN 12:02) Citation IconCite this Report

Frequent small gas explosions

About 60 small gas explosions/day continued to occur through February. Plumes reached maximum heights of 600 m. No volcanic seismicity was recorded.

Information Contacts: VSI.


March 1987 (SEAN 12:03) Citation IconCite this Report

Small gas explosions continue

March eruptive activity consisted of ~250 small gas explosions with plumes reaching a maximum height of 600 m above the crater rim. Of the 22 earthquakes recorded during March, 17 were of tectonic origin (deep) and five were volcanic (shallow).

Information Contacts: VSI; T. Casadevall, USGS & VSI.


April 1987 (SEAN 12:04) Citation IconCite this Report

About 50 small explosions daily

Sangeang Api continued in eruption with an average of ~50 small explosions/day during April. The maximum plume height was 600 m. No earthquakes were detected during April.

Information Contacts: T. Casadevall, USGS & VSI.


June 1987 (SEAN 12:06) Citation IconCite this Report

Frequent explosions continue

Eruptive activity continued during May and June with ~50 explosions/day . . . . Plumes reached ~600 m above the crater rim. No earthquakes accompanied the explosions.

Information Contacts: VSI.


July 1987 (SEAN 12:07) Citation IconCite this Report

Activity continues; plumes to 600 m

Eruptive activity continued during July with ~45 explosions/day producing plumes to 600 m above the crater rim. No earthquakes accompanied the explosions. No VSI geologist has been able to visit the island to inspect the activity since early 1986.

Information Contacts: VSI.


August 1987 (SEAN 12:08) Citation IconCite this Report

Small explosions continue

The eruption . . . continued in August, with ~25 explosions/day ejecting plumes to ~600 m above the crater rim. A seismometer 5 km from the summit recorded no earthquakes accompanying the explosions.

Information Contacts: VSI.


September 1987 (SEAN 12:09) Citation IconCite this Report

Small explosions continue

September activity was similar to . . . August, with ~25 explosions/day. Plumes reached ~600 m above the crater rim.

Information Contacts: VSI.


October 1987 (SEAN 12:10) Citation IconCite this Report

Fewer explosions

Eruptive activity continued in October at a rate of ~18 explosions/day, with plumes reaching ~600 m above the crater rim. The number of daily explosions has declined steadily from 50-70/day in early 1987, and the October rate is the lowest since the eruption started in July 1985.

Information Contacts: VSI.


December 1987 (SEAN 12:12) Citation IconCite this Report

Eruptive activity continues at steady rate

Eruptive activity continued during November and December at ~18 explosions/day, about the same rate as in October.

Information Contacts: VSI.


February 1988 (SEAN 13:02) Citation IconCite this Report

Explosions and earthquakes end

The number of explosions . . . declined steadily from 50-70/day in early 1987 to ~15/day at the end of the year. By February, explosions had stopped, although fuming continued from the summit crater, producing a whitish plume. No earthquakes were reported during February.

Information Contacts: VSI.


May 1999 (BGVN 24:05) Citation IconCite this Report

March to May plumes are thin and rise to 150 m above the summit

As of 21 February the seismograph was under repair so the volcano was monitored visually. During 9 March-24 May a "white ash plume" rose 10-150 m above the summit. During 27 April - 3 May the plume remained thin, but after 4 May it vacillated between thick and thin.

Sangeang Api volcano, one of the most active in the Lesser Sunda Islands, forms a small 13-km-wide island off the NE coast of Sumbawa Island. Two large volcanic cones, 1,949-m-high Doro Api and 1,795-m-high Doro Mantoi, were constructed in the center and on the eastern rim, respectively, of an older, largely obscured caldera. Flank vents occur on the south side of Doro Mantoi and near the northern coast. Intermittent historical eruptions have been recorded since 1512, most of them during in the 20th century.

Information Contacts: Volcanological Survey of Indonesia (VSI), Jalan Diponegoro No. 57, Bandung 40122, Indonesia (URL: http://www.vsi.esdm.go.id/).


July 2009 (BGVN 34:07) Citation IconCite this Report

Increased seismicity, including explosion earthquakes, during May-June 2009

According to the Center of Volcanology and Geological Hazard Mitigation (CVGHM), restlessness began at Sangeang Api in May and June 2009. In early May 2009 white emissions reached heights of ~ 5-25 m. In addition, occasional explosion earthquakes and generally minor seismicity continued (table 3). In addition, an earthquake struck on 1-2 June 2009 that was felt at a Modified Mercali intensity of MM I.

Table 3. Summary of reported volcanic activity at Sangeang Api. Courtesy of the Center of Volcanology and Geological Hazard Mitigation (CVGHM).

Date Explosions Tremor and amplitude Deep volcanic earthquakes Shallow volcanic earthquakes
01-17 May 2009 Avg. ~3/day continuous, 3 mm Avg. ~2/day ~1/day
18-31 May 2009 ~13/day continuous, 7 mm ~4/day ~2/day
01-02 Jun 2009 ~21/day continuous, 5 mm ~2/day 1/day
03 Jun 2009 11 continuous, 6 mm 7 --

On 4 June the Alert Level was raised to 2 (on a scale of 1-4) due to the increases in the number of explosion earthquakes, tremor, and other local earthquakes. Residents and visitors were prohibited from climbing the volcano. No thermal anomalies have been seen in MODIS imagery between 1999 and August 2009.

Information Contacts: Center of Volcanology and Geological Hazard Mitigation (CVGHM), Jalan Diponegoro 57, Bandung 40122, Indonesia (URL: http://vsi.esdm.go.id/).


December 2009 (BGVN 34:12) Citation IconCite this Report

Explosive eruptions during 1997-1999 were previously unreported

A recent translation of an older report from the Center of Volcanology and Geological Hazard Mitigation (CVGHM) discussed previously undocumented interval of eruptions at Sangeang Api (figure 3) during 1997-1999. These eruptions were described, along with other known eruptions, in broad terms in their report. They were generally explosive, with lava domes and lava discharges, similar to the eruptions of 1911, 1953, 1954, 1985-1988.

Figure (see Caption) Figure 3. A photograph of the 13-km-wide Sangeang Api taken on 15 October 2002 by Space Shuttle astronauts (photo STS-112-E-5628). A wide channel running W from provides a path for inferred lava and pyroclastic flows. Courtesy of NASA Earth Observatory.

Dali Ahmad confirmed the occurrence of explosive activity during the 1997-1999 period. These took place without causing casualties because, since 1989, all of the island residents had departed to the nearby Sumbawa Island. No additional eruptions were indicated through at least 2009. In recent times the island's summit crater has produced intermittent steam clouds.

Turner and others (2003) used Uranium-series isotopes to provide insights into Sangeang Api magma evolution. The volcano erupts potassic lavas (SiO2 ~47?55%) with a spectrum of xenoliths that record the liquid line of descent. The scientists estimated that the Sangeang Api magma chamber was about 6-10 km3 in volume and underwent cooling rates of ~0.05°C/year.

Reference. Turner, S., Foden, J., George, R., Evans, P., Varne, R., Elburg, M., and Jenner, G., 2003, Rates and processes of potassic magma evolution beneath Sangeang Api volcano, East Sunda Arc, Indonesia: Journal of Petrology, v. 44, no. 3, pp. 491-515.

Information Contacts: Dali Ahmad, Center of Volcanology and Geological Hazard Mitigation (CVGHM), Jalan Diponegoro 57, Bandung 40122, Indonesia (URL: http://www.vsi.esdm.go.id/); NASA Earth Observatory (URL: http://earthobservatory.nasa.gov/).


July 2013 (BGVN 38:07) Citation IconCite this Report

Fumarolic emissions and variable seismicity during 2012-2013

This Bulletin reports Sangeang Api activity since our last report of December 2009, (BGVN 34:12) until 1 November 2013. Sangeang Api volcano resides in the Flores Sea of Indonesia (figures 4 and 5). Several seismic events and corresponding white plumes were observed in 2012 and 2013. The Alert Level corresponding to the events were temporarily raised then lowered. The Alert Level scale extends from a low of 1 to a high of 5.

Figure (see Caption) Figure 4. Sangeang Api volcano is on a 13-km-wide island of the same name located in the Lesser Sunda Islands of the Indonesian Archipelago.
Figure (see Caption) Figure 5. Sangeang Api seen in a N-looking view showing the summit area with active crater rim cut by the red triangle. A conspicuous older dormant crater lies NNE. Courtesy of Google Earth.

The Indonesian government's Center for Volcanology and Geologic Hazard Mitigation (CVGHM) performs in situ visual, seismicity and satellite monitoring of Sangeang Api volcano and reports significant events. The same agency is also called Pusat Volkanologi dan Mitigasi Bencana Geolog - or PVMBG, a name that also appears on reports.

2009 - 2011 activity. Sangeang Api seismicity increased during May and June 2009 at the same time white plumes were observed with heights from 5 to 25 m. On 4 June 2009, CVGHM increased the alert level from 1 to 2 on the scale of 1 to 4. During 2010 and 2011 Sangeang Api reporting was unarchived on the web.

2012 activity. CVGHM reported that during 1-10 October 2012 Sangeang Api was often not visible due to fog; however when visible occasionally plumes were visible and rose as high as 20 m above the crater. The lava dome and surrounding areas had not changed compared to the beginning of the year. Both the number and magnitude of earthquakes increased on 5 October, declined during 6-8 October, then again increased on 9 October 2012. The Alert Level was raised to 3 on 10 October.

CVGHM issued an eruption warning on 12 October 2012 based on increased seismic activity. They commented that surface activity had not been detected so far, but a new eruption from the summit lava dome would not be a surprise. However, the hazard warning status definitions are not a robust basis for describing predictions.

CVGHM reported that during November through mid-December 2012 observers at the Sangeang, Bima District observation post (50 km SW) noted occasional diffuse white plumes rising 5-15 m above Sangeang Api's crater. The lava dome and surrounding areas had not changed compared to October observations. Avalanches had occurred on the W and SW flanks however their size was omitted. Earthquakes had declined. The Alert Level was lowered to 2 on 21 December.

2013 activity. CVGHM reported that 1-19 May 2013 diffuse white plumes rose 10 m above Sangeang Api's crater. Both the lava dome and surrounding areas showed no changes since November 2012. Seismicity had increased on 26 April 2013 which included 14 tremor events and remained high through June. From May through 13 June 2013 diffuse white plumes rose 10 m above Sangeang Api's crater. As many as 77 shallow earthquakes and 66 deep earthquakes had been detected daily (figure 6). The risk analysis by Surono (2013) noted that lava dome growth and avalanches had occurred on the W and SW flanks (figure 7). Note figure 3 seismicity records cease after 30 May 2013.

In June 2013, 15 shallow earthquakes and three deep earthquakes were detected. The Alert Level was lowered to 2 on 14 June. The public were advised not to approach the craters within a radius of 1.5 km.

Figure (see Caption) Figure 6. Sangeang Api seismicity registered during the period 1 January - 28 May 2013. Later reporting by CVGHM states shortly after this period the seismicity decreased and the alert level decreased. Courtesy of CVGHM.
Figure (see Caption) Figure 7. Sangeang Api volcano, which is truncated by a sharp rim and central crater. This image accompanied the CVGHM risk and situation summary power point update on 30 May 2013 for alert level 3 volcanoes. Date, location, look direction, and photographer unknown. Taken from Surono (2013). Courtesy of CVGHM.

Reference. Surono (no first name), 5/30/2013 Risk and Situation Update Of Each Volcano Under Alert Level III, Ministry Of Energy and Mineral Resources, Indonesia https://docs.unocha.org/sites/dms/ROAP/Indonesia/Documents/PVMBG - VOLCANO_IN_LEVEL_III-30May2013.pdf

Information Contacts: Dali Ahmad, Center of Volcanology and Geological Hazard Mitigation (CVGHM), Jalan Diponegoro 57, Bandung 40122, Indonesia (URL: http://www.vsi.esdm.go.id/); and NASA Earth Observatory (URL: http://earthobservatory.nasa.gov/).


February 2014 (BGVN 39:02) Citation IconCite this Report

Ashfall from 30 May 2014 eruption causes evacuations, airline delays

Due to elevated seismic activity, the Indonesian Center for Volcanology and Geologic Hazard Mitigation (CVGHM) issued an alert for Sangeang Api volcano on 21 May 2014. On 30 May 2014 at 1555, CVGHM reported an eruption of the island volcano that generated an explosive eruption column of ash and sulfur dioxide into the atmosphere, extending >3 km above the summit (figure 8). While the 13-km-wide island of Sangeang has no permanent settlements or residents, dozens of farmers cultivate land on the island during the growing and harvest seasons. Photographs of the eruption showed several pyroclastic flows coming down the volcano summit to the S and E that may be hazardous to anyone of the island. On 30 May, the Alert Level was raised from 2 to 3 (on a scale of 1-4). Civil authorities evacuated 135 people from within 1.5 km of the volcano to the mainland (nearby Sumbawa Island), with the result that no one was reported to have been killed or injured during the eruption.

Figure (see Caption) Figure 8. Eruption plume rising from Sangeang Api volcano on 30 May 2014, photographed to the N from Sambawa Island. Note the distinctive lenticular white cloud condensed from uplifted moist air carried by the rising plume. Pyroclastic flows can also be seen moving down along the S and E sides of the volcano. Courtesy of Anonymous (2014).

Based on satellite images, pilot observations, and the Indonesian Meteorological Office, the Darwin VAAC reported that on 30 May an ash plume rose to an maximum altitude of 15.2 km and drifted 440 km E and 750 km SE (figure 9).

Figure (see Caption) Figure 9. After erupting, the Sangeang Api volcano sent an ash plume to the E, along with a distinctive lenticular white cloud condensed from uplifted moist air. Pilots in the area reported seeing the cloud rising to 19.8 km, spreading over a 40 km area. Photograph taken on 30 May 2014 by Sofyan Efendi looking N during a commercial flight from Bali to the fishing town of Labuan Bajo; from Hall (2014).

The Indonesian Regional Disaster Management Agency (BNPB) reported that on 31 May two larger explosions occurred at 1330 and 2242 hrs. According to the VAAC, ash plumes from these two explosions rose to altitudes of 13.7-15.2 km and drifted 280 km NW (and other various directions, including S). Later in the day the ash plumes, including one from the previous day, eventually became detached. Ashfall affected many areas in the Bima Regency on the mainland, including Wera, and prompted the evacuation of 7,328 people from four villages within a radius of 8 km from Sangeang Api. The Bima and Tambolaka airports were temporarily closed. According to a news article, all flights to and from the Darwin International Airport in Australia on 31 May were canceled (figure 10). The VAAC noted that ash plumes rose to an altitude of 4.3 km on 1 June and drifted W and SW (figure 11). During 2-3 June ash plumes rose to altitudes of 3-4.3 km and drifted 45 km W. Based on analyses of satellite imagery and wind data, the Darwin VAAC reported that on 14 June an ash plume from Sangeang Api rose to an altitude of 2.1 km and drifted 55 km NW.

Figure (see Caption) Figure 10. The Moderate Resolution Imaging Spectroradiometer (MODIS) aboard the Terra satellite captured imagery of the eruption plume from Sangeang Api (dark brown line on the image extending from the volcanic island to the SE) at 0235 UTC (1035 local time) on 31 May 2014. Ash drifted SE, shutting down airports in Bima, Indonesia, and Darwin, Australia. Service to Darwin resumed by 1 June, but Bima remained shut down as of 2 June, according to the Jakarta Globe. Other satellites have observed the ash plume as well. A near real-time tool developed by University of Wisconsin and NOAA scientists estimated that the plume reached an altitude of at least 12 to 14 km based on observations from multiple weather satellites. The Ozone Mapping & Profiler Suite on Suomi NPP also observed ash drifting toward Australia on 31 May. NASA image courtesy Jeff Schmaltz LANCE/EOSDIS MODIS Rapid Response Team, GSFC; Caption by Adam Voiland. From NASA Earth Observatory (2014, 3 June).
Figure (see Caption) Figure 11. Landsat 8 satellite collected this true-color image of an ash plume rising from the Sangeang Api, an island volcano just of the coast of Sumbawa Island, Indonesia, on 1 June 2014. Note that on this day the plume is being blown W and then SW as compared with the previous day shown in figure 8. NASA Earth Observatory images by Robert Simmon, using Landsat 8 data from the USGS Earth Explorer. From NASA Earth Observatory (2014, 1 June).

During the period from 2-17 June, thin to thick white smoke was ejected as high as 200-500 m. Seismic activity during the major part of the eruption is shown on Table 4; as of 17 June, seismicity continued to decline. The Alert Level was reduced from 3 to 2 (on a scale of 1-4) on 17 June.

Table 4. Numbers of daily earthquakes measured for 3 days during and after the eruption of Sangeang Api, as reported by CVGHM. 'VB' represents shallow volcanic earthquakes; 'VA' represents deep volcanic earthquakes; 'TL' represents local earthquake tectonics; 'X' indicates activity present; 'nr' is not reported .

Date, 2014 30 May 31 May 1 June
VB 88 143 35
VA 270 157 62
TL nr nr 5
Volcanic swarm X nr nr
Continuous tremor X X X
Tremor eruption X X X
Blowing earthquake nr nr 36

MODVOLC and other satellite imaging. Satellite infrared measurements of thermal alerts over this Sangeang Api volcano eruption first appeared as 2 pixels (an area of thermal anomaly of ≥2 km2) at 1405 UTC on 30 May 2014. These were the first thermal alerts measured over Sangeang Api since 20 October 2013. From 30 May 2014 through 7 July, satellite crossings measured alerts of between 1 and 9 pixels (areas of ≥1 to ≥9 km2, respectively) daily until 1500 UTC on 30 June; the 9-pixel thermal alert was measured 20 June 2014 at 1425 UTC (figure 12). (Note: As an explanation for this technique, the MODVOLC web site states that "Using infrared satellite data provided by the Moderate Resolution Imaging Spectroradiometer (MODIS), scientists at the Hawai'i Institute of Geophysics and Planetology, University of Hawai'i, have developed an automated system [MODVOLC] which maps the global distribution of thermal hot-spots in near-real-time, and displays the results on this web-site." A paper by Wright and others (2004) states that "Although MODIS pixels are nominally 1 km, pixel size increases with distance from nadir and at the edges of the MODIS swath (where the scan angle reaches ±55°) MODIS pixels measure ~2.08 km in the along-track, and ~4.83 km in the across-track direction.")

Figure (see Caption) Figure 12. MODVOLC image for the period 30 May to 7 July 2014 of thermal alerts measured on Sangeang Api volcano. The volcano lies on the island of Sangeang just off the Indonesian island of Sumbawa. The central array of pixels trending E-W are for those alerts measured for the period 30 May - 30 June 2014. Courtesy of MODVOLC.

Figures 13 and 14 show satellite images of ash plume temperature and SO2 plume from Sangeang Api volcano on 30 and 31 May 2014, respectively. The plume is obviously drifting to the E and S toward Australia.

Figure (see Caption) Figure 13. Composite of the Day-Night Band (DNB, red-to-yellow) at 750m resolution and the IR11.45 (I5, color scale at the top) channel at 375m resolution, image made 30 May 2014 at 1745 UTC. The DNB shows two craters at Sangeang Api volcano, Doro Api and Doro Mantoi. The brighter one was emanating the big plume with temperature values down to -196.5 K (76.6 °C) at the top. The secondary crater was emanating some material, but at much lower level so could hardly be seen. Courtesy of EUMETSAT (2014).
Figure (see Caption) Figure 14. SO2 measured from the Sangeang Api volcano plume on 31 May 2014 at 0535 UTC. The volcano is located at the W end of the measured area. Courtesy of NOAA.

References. Anonymous, 2014 (30 May), Massive volcano eruption: Sangeang Api volcano - Sunda Islands, Indonesia, Before Its News web site (http://beforeitsnews.com/environment/2014/05/massive-volcano-eruption-sangeang-api-volcano-sunda-islands-indonesia-2502094.html).

EUMETSAT, 2014, Eruption of Sangeang Api volcano: There were a series of spectacular eruptions from the Indonesian volcano Sangeang Api at the end of the May. URL: http://www.eumetsat.int/website/home/Images/ImageLibrary/DAT_2235292.html

NASA Earth Observatory, 2014 (3 June), Sangeang Api Erupts (URL: http://earthobservatory.nasa.gov/IOTD/view.php?id=83799).

NASA Earth Observatory, 2014 (1 June), Sangeang Api Eruption (URL: http://earthobservatory.nasa.gov/NaturalHazards/view.php?id=83887&eocn=image&eoci=nh_viewall)

Wright, R., Flynn, L.P, Garbeil, H., Harris, A.J.L., and Pilger, E., 2004, MODVOLC: near-real-time thermal monitoring of global volcanism, Journal of Volcanology and Geothermal Research, v. 135, pp. 29-49.

Hall, J., 2014 (30 May), Pictured from a passenger plane: Menacing 12-mile-high ash cloud looms over Indonesia's 'Mountain of Spirits' after volcano erupts, Daily Mail (URL: http://www.dailymail.co.uk/news/article-2644253/Incredible-moment-huge-volcano-erupts-Indonesia-sending-ash-spewing-thousands-feet-sky.html).

Information Contacts: Indonesian Centre for Volcanology and Geological Hazard Mitigation – CVGHM (also known as Pusat Vulkanologi dan Mitigasi Bencana Geologi - PVMBG)), Jalan Diponegoro 57, Bandung 40122, Indonesia (URL: http://www.vsi.esdm.go.id/); MODVOLC, Hawai'i Institute of Geophysics and Planetology (HIGP) Thermal Alerts System, School of Ocean and Earth Science and Technology (SOEST), Univ. of Hawai'i, 2525 Correa Road, Honolulu, HI 96822, USA (URL: http://modis.higp.hawaii.edu/); DARWIN VAAC (Darwin Volcanic Ash Advisory Centre), Bureau of Meteorology, Northern Territory Regional Office, PO Box 40050, Casuarina, NT 0811, Australia (URL: http://www.bom.gov.au/info/vaac/); Badan Penanggulangan Bencana Daerah (BPBD), Indonesian Regional Disaster Management Agency (URL: http://bpbd.malangkab.go.id/); and Badan Nasional Penanggulangan Bencana (BNPB), Indonesian National Disaster Management Agency (URL: http://www.bnpb.go.id/).


October 2016 (BGVN 41:10) Citation IconCite this Report

Large explosions in May 2014 followed by thermal anomalies until early November 2015

On 21 May 2014 the PVMBG (Pusat Vulkanologi dan Mitigasi Bencana Geologi) issued an alert for Sangeang Api based on elevated seismic activity. An explosive eruption followed on 30 May (BGVN 39:02), sending a dense column of ash and sulfur dioxide billowing more than 3 km above the volcano. Two larger explosions occurred the next day. No further explosive activity was seen, but thermal anomalies were recorded by satellite-based instruments during June-December 2014 and March-November 2015.

Review of May-June 2014 activity. PVMBG reported that during January-29 May 2014 diffuse white plumes rose at most 25 m above the crater. On 30 May seismicity increased, with tremor starting at 0500 and becoming continuous at 1348. An eruption at 1555 generated an ash plume that rose 3 km and drifted W, causing ashfall over the sea. The Alert Level was raised to 3 (on a scale of 1-4). The island has no permanent settlements, and is only occupied during the growing and harvest seasons; civil authorities evacuated 135 people to the mainland. Based on satellite images, pilot observations, and the Indonesian Meteorological Office, the Darwin VAAC reported that the 30 May ash plume rose to an altitude of 15.2 km and drifted 440 km E and 750 km SE (figure 15).

Figure (see Caption) Figure 15. An ash plume rises from Sangeang Api during an eruption on 30 May 2014. Photo taken looking NE from Sumbawa Island. Courtesy of Australian Associated Press.

BNPB reported that on 31 May two larger explosions occurred at 1330 and 2242 hours. According to the VAAC, ash plumes from those explosions rose to altitudes of 13.7-15.2 km and drifted 280 km NW and other various directions. Later in the day the ash plumes became detached. Ashfall affected many areas in the Bima Regency on the mainland, including Wera, and prompted the evacuation of 7,328 people from four villages within a radius of 8 km from Sangeang Api. The Bima and Tambolaka airports were temporarily closed. According to a news article, all flights to and from the Darwin International Airport in Australia on 31 May were canceled.

The VAAC noted that ash plumes rose to an altitude of 4.3 km on 1 June 2014 and drifted W and SW. During 2-3 June ash plumes rose to altitudes of 3-4.3 km and drifted 45 km W. During clear conditions on 1-17 June, incandescence at the summit and white-and-gray plumes (100-1,500 m above the summit) were visible. On 1 June 2014 seismicity dramatically decreased, and as of 17 June was still declining. The Alert Level was reduced from 3 to 2 (on a scale of 1-4) on 17 June.

Activity during 2015. PVMBG observers at the Sangeang Api post in Desa Sangeang Darat, Bima, West Nusa Tenggara, reported that during 1 July-30 September 2015 diffuse white plumes rose up to 250 m above the crater rim. During 1 October-1 November 2015 white-to-gray plumes rose as high as 350 m. Beginning on 23 October occasional weak thumping noises were reported. Crater incandescence possibly indicated lava-dome growth or lava-flow advancement. The Alert Level remained at 2 (on a scale of 1-4); visitors and residents were warned not to approach the crater within a 1.5-km radius.

Thermal anomaly data. Nearly daily thermal alerts were measured by MODVOLC (using MODIS data) following the 30 May eruption from 7 June until about 27 December 2014. Alerts appeared again, frequently but not daily, between 17 March and 13 October 2015, with a final alert pixel on 5 November 2015. MIROVA measured low to medium radiative power thermal anomalies from early June 2014 until late November 2015.

Information Contacts: Pusat Vulkanologi dan Mitigasi Bencana Geologi (PVMBG, also known as Indonesian Center for Volcanology and Geological Hazard Mitigation, CVGHM), Jalan Diponegoro 57, Bandung 40122, Indonesia (URL: http://www.vsi.esdm.go.id/); Darwin Volcanic Ash Advisory Centre (VAAC), Bureau of Meteorology, Northern Territory Regional Office, PO Box 40050, Casuarina, NT 0811, Australia (URL: http://www.bom.gov.au/info/vaac/); The Guardian News (URL: https://www.theguardian.com/world/2014/may/31/indonesian-volcanic-ash-cloud-halts-flights-in-and-out-of-darwin); MIROVA (Middle InfraRed Observation of Volcanic Activity), a collaborative project between the Universities of Turin and Florence (Italy) supported by the Centre for Volcanic Risk of the Italian Civil Protection Department (URL: http://www.mirovaweb.it/); Hawai'i Institute of Geophysics and Planetology (HIGP), MODVOLC Thermal Alerts System, School of Ocean and Earth Science and Technology (SOEST), Univ. of Hawai'i, 2525 Correa Road, Honolulu, HI 96822, USA (URL: http://modis.higp.hawaii.edu/, http://modis.higp.hawaii.edu/).


September 2017 (BGVN 42:09) Citation IconCite this Report

Weak Strombolian activity and occasional weak ash plumes, 15 July-12 August 2017

Strong explosions at Sangeang Api on 30-31 May 2014 generated ash plumes that rose as high as 15 km altitude, followed by less intense activity that produced ash plumes during the first half of June 2014 and 1 July-1 November 2015 (BGVN 41:10). No further activity was reported by the Pusat Vulkanologi dan Mitigasi Bencana Geologi (PVMBG) and Darwin Volcanic Ash Advisory Centre (VAAC) until June 2017.

The MIROVA (Middle InfraRed Observation of Volcanic Activity) system detected thermal anomalies in MODIS satellite data near the summit during the second week of January 2017, when four were recorded (figure 16). The number increased significantly beginning with the latter half of February. Another increase in the number and power of the anomalies took place at the beginning of June 2017 and continued into mid-August.

Figure (see Caption) Figure 16. Thermal anomalies identified by the MIROVA system (radiative power) at Sangeang Api for the year ending 11 August 2017. Note that the anomaly lines in late 2016 are not on the island. Courtesy of MIROVA.

Thermal anomalies identified using the MODVOLC algorithm were first recorded on 25 February 2017. Over the same time period as the MIROVA data, through 11 August, there were 105 thermal alerts. Cumulatively, the locations of the alert pixels define an area extending from the summit crater to about 2.5 km down the E flank (figure 17).

Figure (see Caption) Figure 17. Thermal anomalies (alert pixels) identified by the MODVOLC system at Sangeang Api for 25 February-11 August 2017. The eastern-most pixels are at the summit area. Courtesy of HIGP - MODVOLC Thermal Alerts System.

According to PVMBG, a small Strombolian eruption at 1154 on 15 July 2017 generated an ash plume that rose 100-200 m above the crater rim and drifted SW. Seismicity had increased starting in April. Based on analyses of satellite imagery, PVMBG observations, and wind data, the Darwin VAAC reported that on 16 July an ash plume rose to an altitude of 2.1 km, or 200 m above the crater rim, and drifted NW. The Darwin VAAC also reported ash plumes to altitudes of 2.4-4.3 km on 19-20 July, 29-30 July, 7-8 August, and 12 August 2017; in most cases they drifted NW.

Information Contacts: Pusat Vulkanologi dan Mitigasi Bencana Geologi (PVMBG, also known as Indonesian Center for Volcanology and Geological Hazard Mitigation, CVGHM), Jalan Diponegoro 57, Bandung 40122, Indonesia (URL: http://www.vsi.esdm.go.id/); Darwin Volcanic Ash Advisory Centre (VAAC), Bureau of Meteorology, Northern Territory Regional Office, PO Box 40050, Casuarina, NT 0811, Australia (URL: http://www.bom.gov.au/info/vaac/); Hawai'i Institute of Geophysics and Planetology (HIGP) - MODVOLC Thermal Alerts System, School of Ocean and Earth Science and Technology (SOEST), Univ. of Hawai'i, 2525 Correa Road, Honolulu, HI 96822, USA (URL: http://modis.higp.hawaii.edu/); MIROVA (Middle InfraRed Observation of Volcanic Activity), a collaborative project between the Universities of Turin and Florence (Italy) supported by the Centre for Volcanic Risk of the Italian Civil Protection Department (URL: http://www.mirovaweb.it/).


November 2018 (BGVN 43:11) Citation IconCite this Report

Ongoing crater activity and thermal anomalies during September 2017-October 2018

A significant increase in the number of thermal anomalies at Sangeang Api was recorded during February and June through mid-August 2017, along with a small Strombolian eruption in mid-July that generated an ash plume (BGVN 42:09). The high number of thermal anomalies continued through at least 20 October 2018. The current report summarizes activity between 1 September 2017 and 20 October 2018. The volcano is monitored by the Pusat Vulkanologi dan Mitigasi Bencana Geologi (PVMBG) and Darwin Volcanic Ash Advisory Centre (VAAC).

Based on a Volcano Observatory Notice for Aviation (VONA) from PVMBG, on 9 May 2018 a gas emission was observed at 1807 that rose to an altitude of 4,150 m and drifted W. Consequently, the Aviation Color Code was raised from unassigned to Yellow. Clear thermal satellite imagery the next day showed hot material traveling about 500 m SE out of the summit crater and continuing another 500 m down the E flank (figure 18).

Figure (see Caption) Figure 18. Sentinel-2 satellite image of Sangeang Api on 10 May 2018. This "Atmospheric penetration" view (bands 12, 11, and 8A) highlights hot material extending more than a kilometer from the vent in the summit crater to the SE and onto the E flank. Courtesy of Sentinel Hub.

Based on another VONA from PVMBG, an ash emission at 1338 on 15 October 2018 rose 250 m above the summit and drifted SW, W, and NW. The VONA noted that the ash emission possibly rose higher than what a ground observer had estimated. Seismic data was dominated by signals indicating emissions as well as local tectonic earthquakes. The Aviation Color Code was raised from Yellow to Orange.

During the reporting period, MODIS satellite instruments using the MODVOLC algorithm recorded thermal anomalies between 3 and 12 days per month, many of which had multiple pixels. October 2017 had the greatest number of days with hotspots (12), while the lowest number was recorded during December 2017 through February 2018 (3-4 days per month). The vast majority of anomalies issued from the summit; a few were along the E flanks. The MIROVA (Middle InfraRed Observation of Volcanic Activity) volcano hotspot detection system, also based on analysis of MODIS data, recorded numerous hotspots during the previous 12 months through mid-October 2018, except for the second half of January 2018 (figure 19). Almost all recorded MIROVA anomalies were within 5 km of the volcano and of low to moderate radiative power.

Figure (see Caption) Figure 19. Thermal anomalies identified by the MIROVA system (Log Radiative Power) at Sangeang Api for the year ending 19 October 2018. Courtesy of MIROVA.

Information Contacts: Pusat Vulkanologi dan Mitigasi Bencana Geologi (PVMBG, also known as Indonesian Center for Volcanology and Geological Hazard Mitigation, CVGHM), Jalan Diponegoro 57, Bandung 40122, Indonesia (URL: http://www.vsi.esdm.go.id/); Darwin Volcanic Ash Advisory Centre (VAAC), Bureau of Meteorology, Northern Territory Regional Office, PO Box 40050, Casuarina, NT 0811, Australia (URL: http://www.bom.gov.au/info/vaac/); Hawai'i Institute of Geophysics and Planetology (HIGP) - MODVOLC Thermal Alerts System, School of Ocean and Earth Science and Technology (SOEST), Univ. of Hawai'i, 2525 Correa Road, Honolulu, HI 96822, USA (URL: http://modis.higp.hawaii.edu/); MIROVA (Middle InfraRed Observation of Volcanic Activity), a collaborative project between the Universities of Turin and Florence (Italy) supported by the Centre for Volcanic Risk of the Italian Civil Protection Department (URL: http://www.mirovaweb.it/); Sentinel Hub Playground (URL: https://www.sentinel-hub.com/explore/sentinel-playground).


May 2019 (BGVN 44:05) Citation IconCite this Report

Ongoing frequent explosions with ash plumes, Strombolian activity, and block avalanches, November 2018-April 2019

Sangeang Api is a small 13-km-wide island volcano off the NE coast of Sumbawa Island, part of Indonesia's Lesser Sunda Islands. Intermittent historical eruptions have been recorded since 1512, most of them during in the 20th century. Ash plumes, Strombolian activity and pyroclastic and lava flows during 1985-1987 from the Doro Api summit crater were the first activity in 20 years and led to the evacuation of over 1,200 residents on the island. Explosive activity resumed for about two years during 1997-1999; no further activity was reported until increased seismicity and white emissions were noted in mid-2009. This activity was intermittent from 2009 through early 2014.

On 30 and 31 May 2014, Pusat Vulkanologi dan Mitigasi Bencana Geologi (PVMBG, or CVGHM) reported large explosions with ash plumes that rose to around 15 km altitude and pyroclastic flows down the flanks (BGVN 39:03, 41:10). The massive ash plume drifted SE, closing airports as far away as Darwin, Australia. The ashfall caused airline disruption and evacuation of thousands in villages on nearby Sumbawa Island. Strong thermal anomalies appeared after the explosions and lasted for the rest of 2014, indicative of flow activity down the E flank; mostly steam plumes, with occasional ash emissions were reported during 2015. Renewed thermal activity appeared in satellite data in mid-January 2017. The thermal signature increased through July 2017 when Strombolian activity and ash emissions were reported (BGVN 42:09). A high level of thermal activity continued through October 2018, with satellite imagery confirming incandescent activity on the E flank, and PVMBG reporting ash emissions that rose a few kilometers above the summit (BGVN 43:11).

During October 2018-April 2019, covered in this report, elevated thermal activity was recorded with satellite data and imagery, and visitors to the island recorded ash plumes, Strombolian activity, lava bombs, and a blocky avalanche flow down the E flank from the pyroclastic cone inside Doro Api cone. Information comes from satellite thermal data and imagery, and reports from visitors to the island. Indonesia's Pusat Vulkanologi dan Mitigasi Bencana Geologi (PVMBG) listed Sangeang Api at Alert Level II for the period. There were no reports from the Darwin VAAC.

Thermal activity became more intermittent during December 2018-March 2019 compared with the previous six months, and then increased again in April according to the MIROVA project thermal data (figure 20). The MODVOLC thermal alerts showed a similar pattern, with a decrease in the number of monthly alerts during December through March. In spite of this, a strong thermal signal was still apparent near the summit throughout the period (figure 21). Sentinel-2 satellite images confirmed the presence of hot material at the summit and down the E-flank ravine throughout the period (figure 22).

Figure (see Caption) Figure 20. Thermal activity at Sangeang Api persisted during November 2018-April 2019. Activity was more intermittent from December 2018 through March 2019 but increased again in frequency and intensity in April 2019. Courtesy of MIROVA.
Figure (see Caption) Figure 21. MODVOLC thermal alert images of Sangeang Api for each month from November 2018-April 2019 indicated persistent thermal activity each month, concentrated at the summit and on the upper part of the E flank. Courtesy of Hawai'i Institute of Geophysics and Planetology (HIGP) - MODVOLC Thermal Alerts System.
Figure (see Caption) Figure 22. Sentinel-2 satellite infrared images confirmed thermal activity at the summit crater and down the ravine on the E flank of Sangeang Api during October 2018 through April 2019. The activity migrated and varied in intensity, indicative of ongoing activity throughout the period. Top left: 12 October 2018. Top right: 27 October 2018. Middle left: 16 November 2018. Middle right: 21 December 2018. Bottom left: 14 February 2019. Bottom Right: 20 April 2019. Courtesy of Sentinel Hub Playground ('Atmospheric Penetration' rendering with bands 12, 11, and 8A).

A Google Earth image dated 7 October 2018 shows dark lava in the drainage on the SE flank extending to within 1 km of the shoreline (figure 23). A visit to Sangeang Api by photographer Martin Rietze during 25 September-3 October 2018 provided excellent ground and drone-based photographic and video documentation of the eruptive activity at that time (see information contacts for link to video footage). Regular small ash emissions were recorded multiple times per day from a pyroclastic cone inside the Doro Api cone (figure 24); the explosions produced volcanic bombs that traveled hundreds of meters down the flanks of Doro Api (figure 25) as well as sending lava fragments down all sides of the pyroclastic cone (figures 26 and 27). Steam and ash rose a few hundred meters above the summit of the pyroclastic cone and was incandescent after dark (figures 28 and 29).

Figure (see Caption) Figure 23. A Google Earth image of the SE flank of Sangeang Api taken on 7 October 2018 shows dark channels of lava descending the ravine to within about 1 km of the shore. Data from SIO, NOAA, U.S. Navy, NGA, GEBCO, Copyright 2018, Google, 2019 Maxar Technologies. Courtesy of Google Earth.
Figure (see Caption) Figure 24. A view from the SW of Sangeang Api island with the two cones of the volcano taken during a 25 September-3 October 2018 expedition. In the foreground is inactive Doro Mantai and, in the background, a small ash plume rises from the active Doro Api cone. Copyrighted photo by Martin Rietze (used with permission).
Figure (see Caption) Figure 25. Explosions with ash plumes sent ejecta hundreds of meters down the W flank of Doro Api (left), the active cone at Sangeang Api, photographed during a 25 September-3 October 2018 expedition. Copyrighted photo by Martin Rietze (used with permission).
Figure (see Caption) Figure 26. A large pyroclastic cone fills the summit crater of Doro Api cone on Sangeang Api, photographed during a 25 September-3 October 2018 expedition. Copyrighted photo by Martin Rietze (used with permission).
Figure (see Caption) Figure 27. Ash explosions sent plumes to a few hundred meters above the summit of Sangeang Api's Doro Api cone, and large bombs and tephra fell around the flanks of the cone. Photographed during a 25 September-3 October 2018 expedition. Copyrighted photo by Martin Rietze (used with permission).
Figure (see Caption) Figure 28. Ash and steam rose from the pyroclastic cone inside Doro Api, the active cone at Sangeang Api. Photographed during a 25 September-3 October 2018 expedition. Avalanche blocks form channels of lava in the ravine on the E flank (right). View is from the SW, taken by drone. Copyrighted photo by Martin Rietze (used with permission).
Figure (see Caption) Figure 29. Incandescence in the ash plumes rising from the pyroclastic cone inside the Doro Api crater was visible at dusk at Sangeang Api when photographed during a 25 September-3 October 2018 expedition. Copyrighted photo by Martin Rietze (used with permission).

Incandescent bombs and blocks from Strombolian activity cascaded down the flanks of the pyroclastic cone and also reached outside of the Doro Api crater, landing on the W flank (figures 30 and 31). Steaming tephra on the flanks of the pyroclastic cone was visible during daylight hours (figure 32); the active Doro Api cone is near the center of the island, the inactive Doro Mantai is on the SE flank. In a nighttime view of Doro Api as seen from the summit of Doro Mantai, the incandescent ejecta is clearly visible hundreds of meters from the erupting pyroclastic cone (figure 33). Video footage showed incandescent lava emerging from a fissure near the base of the pyroclastic cone, and a blocky avalanche on the E flank of the cone; as blocks rolled down the slope, incandescence was visible just below the surface.

Figure (see Caption) Figure 30. Incandescent blocks and bombs were visible at night descending the flank of the pyroclastic cone inside the crater of the Doro Api cone at Sangeang Api when photographed during a 25 September-3 October 2018 expedition. Copyrighted photo by Martin Rietze (used with permission).
Figure (see Caption) Figure 31. Strombolian activity lit up the night sky and scattered bombs around the flanks of the pyroclastic cone inside of the Doro Api cone at Sangeang Api when photographed during a 25 September-3 October 2018 expedition. Fragments also landed on the outer flank of Doro Api (left). Copyrighted photo by Martin Rietze (used with permission).
Figure (see Caption) Figure 32. Steaming tephra surrounded the flanks of the pyroclastic cone inside the Doro Api cone on Sangeang Api when photographed during a 25 September-3 October 2018 expedition. The view, taken by drone, is from the NW, and the quiet Doro Mantai peak lies SE of the active cone closer to the coast. Copyrighted photo by Martin Rietze (used with permission).
Figure (see Caption) Figure 33. This nighttime view of Doro Api cone on Sangeang Api was taken from the summit of adjacent Doro Mantai to the SE during a 25 September-3 October 2018 expedition. Ash rose from the vent at the top of the pyroclastic cone, and incandescent ejecta descended the flanks of the pyroclastic cone, covered the inner walls of the Doro Api summit crater, and also fell outside of the crater onto the W flank of Doro Api (left). In addition, lava emerged from a fissure near the base of the cone (lower right). Copyrighted photo by Martin Rietze (used with permission).

Blocks of lava formed an avalanche down the ravine on the E flank of Doro Api; the avalanche formed channels tens of meters wide on the steep slope (figure 34) when photographed by drone in early October 2018. The PVMBG webcam located on nearby Sumbawa island about 10 km SW captured an image of a small ash emission rising from the Doro Api summit in late October (figure 35). Visitors to the island in November recorded continued activity in the form of ash plumes and incandescent lava emerging from a fissure on the flank of the pyroclastic cone (figure 36).

Figure (see Caption) Figure 34. Fresh blocky lava on the E flank of Doro Api on Sangeang Api was visible in drone images taken by visitors in early October 2019. Bushes in bottom center of the image suggest that the channels of lava blocks are tens of meters across. Courtesy of Doro Adventures.
Figure (see Caption) Figure 35. The PVMBG webcam located about 10 km SW on nearby Sumbawa island captured an ash emission from the Doro Api cone at Sangeang Api on 29 October 2018. Courtesy of PVMBG and Øystein Lund Andersen.
Figure (see Caption) Figure 36. Visitors to Sangeang Api in November 2018 witnessed incandescent bombs and lava emerging from a fissure on the flank of the pyroclastic cone inside Doro Api crater. Courtesy of 80 Jours Voyages.

Information Contacts: Pusat Vulkanologi dan Mitigasi Bencana Geologi (PVMBG, also known as Indonesian Center for Volcanology and Geological Hazard Mitigation, CVGHM), Jalan Diponegoro 57, Bandung 40122, Indonesia (URL: http://www.vsi.esdm.go.id/); MAGMA Indonesia, Kementerian Energi dan Sumber Daya Mineral (URL: https://magma.vsi.esdm.go.id/); MIROVA (Middle InfraRed Observation of Volcanic Activity), a collaborative project between the Universities of Turin and Florence (Italy) supported by the Centre for Volcanic Risk of the Italian Civil Protection Department (URL: http://www.mirovaweb.it/); Hawai'i Institute of Geophysics and Planetology (HIGP) - MODVOLC Thermal Alerts System, School of Ocean and Earth Science and Technology (SOEST), Univ. of Hawai'i, 2525 Correa Road, Honolulu, HI 96822, USA (URL: http://modis.higp.hawaii.edu/); Google Earth (URL: https://www.google.com/earth/); Sentinel Hub Playground (URL: https://www.sentinel-hub.com/explore/sentinel-playground); Martin Rietze, Taubenstr. 1, D-82223 Eichenau, Germany (URL: https://mrietze.com/, Videos at https://www.youtube.com/channel/UC5LzAA_nyNWEUfpcUFOCpJw/videos); Øystein Lund Andersen (Twitter: @OysteinLAnderse, https://twitter.com/OysteinLAnderse, URL: http://www.oysteinlundandersen.com); 80 Jours Voyages, Lyon, France (Twitter: https://twitter.com/jours_80, URL: https://80joursvoyages.com/); Doro Adventures (Twitter: https://twitter.com/DoroAdventures, URL: http://doroadventures.com/).


February 2020 (BGVN 45:02) Citation IconCite this Report

Ash emissions and lava flow extrusion continue during May 2019 through January 2020

Sangeang Api is located in the eastern Sunda-Banda Arc in Indonesia, forming a small island in the Flores Strait, north of the eastern side of West Nusa Tenggara. It has been frequently active in recent times with documented eruptions spanning back to 1512. The edifice has two peaks – the active Doro Api cone and the inactive Doro Mantori within an older caldera (figure 37). The current activity is focused at the summit of the cone within a horseshoe-shaped crater at the summit of Doro Api. This bulletin summarizes activity during May 2019 through January 2020 and is based on Darwin Volcanic Ash Advisory Center (VAAC) reports, Pusat Vulkanologi dan Mitigasi Bencana Geologi (PVMBG, or CVGHM) MAGMA Indonesia Volcano Observatory Notice for Aviation (VONA) reports, and various satellite data.

Figure (see Caption) Figure 37. A PlanetScope satellite image of Sangeang Api with the active Doro Api and the inactive Doro Mantori cones indicated, and the channel SE of the active area that contains recent lava flows and other deposits. December 2019 monthly mosaic copyright of Planet Labs 2019.

Thermal anomalies were visible in Sentinel-2 satellite thermal images on 4 and 5 May with some ash and gas emission visible; bright pixels from the summit of the active cone extended to the SE towards the end of the month, indicating an active lava flow (figure 38). Multiple small emissions with increasing ash content reached 1.2-2.1 km altitude on 17 June. The emissions drifted W and WNW, and a thermal anomaly was also visible. On the 27th ash plumes rose to 2.1 km and drifted NW and the thermal anomaly persisted. One ash plume reached 2.4 km and drifted NW on the 29th, and steam emissions were ongoing. Satellite images showed two active lava flows in June, an upper and a lower flow, with several lobes descending the same channel and with lateral levees visible in satellite imagery (figure 39). The lava extrusion appeared to have ceased by late June with lower temperatures detected in Sentinel-2 thermal data.

Figure (see Caption) Figure 38. Sentinel-2 satellite thermal images of Sangeang Api on 20 May and 9 June 2019 show an active lava flow from the summit, traveling to the SE. False color (urban) image (bands 12, 11, 4) courtesy of Sentinel Hub Playground.
Figure (see Caption) Figure 39. PlanetScope satellite images of Sangeang Api show new lava flows during June and July, with white arrows indicating the flow fronts. Copyright Planet Labs 2019.

During 4-5 July the Darwin VAAC reported ash plumes reaching 2.1-2.3 km altitude and drifting SW and W. Activity continued during 6-9 July with plumes up to 4.6 km drifting N, NW, and SW. Thermal anomalies were noted on the 4th and 8th. Plumes rose to 2.1-3 km during 10-16th, and to a maximum altitude of 4.6 km during 17-18 and 20-22. Similar activity was reported during 24-30 July with plumes reaching 2.4-3 km and dispersing NW, W, and SW. The upper lava flow had increased in length since 15 June (see figure 39).

During 31 July through 3 September ash plumes continued to reach 2.4-3 km altitude and disperse in multiple directions. Similar activity was reported throughout September. Thermal anomalies also persisted through July-September, with evidence of hot avalanches in Sentinel-2 thermal satellite imagery on 23 August, and 9, 12, 22, and 27 September. Thermal anomalies suggested hot avalanches or lava flows during October (figure 40). During 26-28 October short-lived ash plumes were reported to 2.1-2.7 km above sea level and dissipated to the NW, WNW, and W. Short-lived explosions produced ash plumes up to 2.7-3.5 km altitude were noted during 30-31 October and 3-4 November 2019.

Figure (see Caption) Figure 40. Sentinel-2 satellite thermal images of Sangeang Api on 7 and 22 October 2019 show an area of elevated temperatures trending from the summit of the active cone down the SE flank. False color (urban) image rendering (bands 12, 11, 4) courtesy of Sentinel Hub Playground.

Discrete explosions produced ash plumes up to 2.7-3.5 km altitude during 3-4 November, and during the 6-12th the Darwin VAAC reported short-lived ash emissions reaching 3 km altitude. Thermal anomalies were visible in satellite images during 6-8 November. A VONA was released on 14 November for an ash plume that reached about 2 km altitude and dispersed to the west. During 14-19 November the Darwin VAAC reported short-lived ash plumes reaching 2.4 km that drifted NW and W. Additional ash plumes were observed reaching a maximum altitude of 2.4 km during 20-26 November. Thermal anomalies were detected during the 18-19th, and on the 27th.

Ash plumes were recorded reaching 2.4 km during 4-5, 7-9, 11-13, and 17-19 December, and up to 3 km during 25-28 December. There were no reports of activity in early to mid-January 2020 until the Darwin VAAC reported ash reaching 3 km on 23 January. A webcam image on 15 January showed a gas plume originating from the summit. Several fires were visible on the flanks during May 2019 through January 2020, and this is seen in the MIROVA log thermal plot with the thermal anomalies greater than 5 km away from the crater (figure 41).

Figure (see Caption) Figure 41. MIROVA log plot of radiative power indicates the persistent activity at Sangeang Api during April 2019 through March 2020. There was a slight decline in September-October 2019 and again in February 2020. Courtesy of MIROVA.

Information Contacts: Pusat Vulkanologi dan Mitigasi Bencana Geologi (PVMBG, also known as Indonesian Center for Volcanology and Geological Hazard Mitigation, CVGHM), Jalan Diponegoro 57, Bandung 40122, Indonesia (URL: http://www.vsi.esdm.go.id/); MIROVA (Middle InfraRed Observation of Volcanic Activity), a collaborative project between the Universities of Turin and Florence (Italy) supported by the Centre for Volcanic Risk of the Italian Civil Protection Department (URL: http://www.mirovaweb.it/); Sentinel Hub Playground (URL: https://www.sentinel-hub.com/explore/sentinel-playground); Planet Labs, Inc. (URL: https://www.planet.com/).


August 2020 (BGVN 45:08) Citation IconCite this Report

Two ash plumes and small thermal anomalies during February-June 2020

Sangeang Api is a 13-km-wide island located off the NE coast of Sumbawa Island, part of Indonesia's Lesser Sunda Islands. Documentation of historical eruptions date back to 1512. The most recent eruptive episode began in July 2017 and included frequent Strombolian explosions, ash plumes, and block avalanches. The previous report (BGVN 45:02) described activity consisting of a new lava flow originating from the active Doro Api summit crater, short-lived explosions, and ash-and-gas emissions. This report updates information during February through July 2020 using information from the Darwin Volcanic Ash Advisory Center (VAAC) reports, Pusat Vulkanologi dan Mitigasi Bencana Geologi (PVMBG, or CVGHM) reports, and various satellite data.

Volcanism during this reporting period was relatively low compared to the previous reports (BGVN 44:05 and BGVN 45:02). A Darwin VAAC notice reported an ash plume rose 2.1 km altitude and drifted E on 10 May 2020. Another ash plume rose to a maximum of 3 km altitude drifting NE on 10 June, as seen in HIMAWARI-8 satellite imagery.

The MIROVA (Middle InfraRed Observation of Volcanic Activity) analysis of MODIS satellite data detected a total of 12 low power thermal anomalies within 5 km from the summit during February through May 2020 (figure 42). No thermal anomalies were recorded during June and July according to the MIROVA graph. Though the MODVOLC algorithm did not detect any thermal signatures between February to July, many small thermal hotspots within the summit crater could be seen in Sentinel-2 thermal satellite imagery (figure 43).

Figure (see Caption) Figure 42. Thermal anomalies at Sangeang Api from 10 August 2019 through July 2020 recorded by the MIROVA system (Log Radiative Power) were infrequent and low power during February through May 2020. No thermal anomalies were detected during June and July. Courtesy of MIROVA.
Figure (see Caption) Figure 43. Sentinel-2 thermal satellite imagery using “Atmospheric penetration” (bands 12, 11, 8A) rendering showed small thermal hotspots (orange-yellow) at the summit of Sangeang Api during February through June 2020. Courtesy of Sentinel Hub Playground.

Information Contacts: Pusat Vulkanologi dan Mitigasi Bencana Geologi (PVMBG, also known as Indonesian Center for Volcanology and Geological Hazard Mitigation, CVGHM), Jalan Diponegoro 57, Bandung 40122, Indonesia (URL: http://www.vsi.esdm.go.id/); Darwin Volcanic Ash Advisory Centre (VAAC), Bureau of Meteorology, Northern Territory Regional Office, PO Box 40050, Casuarina, NT 0811, Australia (URL: http://www.bom.gov.au/info/vaac/); MIROVA (Middle InfraRed Observation of Volcanic Activity), a collaborative project between the Universities of Turin and Florence (Italy) supported by the Centre for Volcanic Risk of the Italian Civil Protection Department (URL: http://www.mirovaweb.it/); Hawai'i Institute of Geophysics and Planetology (HIGP) - MODVOLC Thermal Alerts System, School of Ocean and Earth Science and Technology (SOEST), Univ. of Hawai'i, 2525 Correa Road, Honolulu, HI 96822, USA (URL: http://modis.higp.hawaii.edu/); Sentinel Hub Playground (URL: https://www.sentinel-hub.com/explore/sentinel-playground).


March 2022 (BGVN 47:03) Citation IconCite this Report

Small ash plume on 17 February 2022

Sangeang Api is a complex volcano on the small island of Sangeang in the Lesser Sunda Islands, Indonesia, consisting of two volcanic cones. After a major explosion in May 2014, activity continued until November 2015, with thermal anomalies indicating possible lava dome growth or lava flows (BGVN 39:02 and 41:10). Another eruptive period during July 2017 into June 2020 included occasional weak ash explosions with ash plumes and emissions, hot material discharged from the summit crater, periods of numerous thermal anomalies, summit incandescence, and infrequent Strombolian activity (BGVN 42:09, 43:11, 44:05, 45:02, and 45:08). The volcano is monitored by Pusat Vulkanologi dan Mitigasi Bencana Geologi (PVMBG, or CVGHM), the Darwin Volcanic Ash Advisory Center (VAAC), and by various satellites.

The only documented activity during August 2020-February 2022 was an ash plume on 17 February 2022 reported by the Darwin VAAC that rose to an altitude of 4-4.9 km (~3 km above the summit) and drifted SW and WSW. During August 2020-February 2022, Sentinel-2 satellite images during this time were usually obscured by weather clouds, but no thermal signals or volcanic activity were observed when there were clear views. During May 2021 through February 2022, the MIROVA (Middle InfraRed Observation of Volcanic Activity) volcano hotspot detection system recorded ten scattered hotspots within 5 km of the summit; the cause of the weak anomalies is unknown.

Information Contacts: Pusat Vulkanologi dan Mitigasi Bencana Geologi (PVMBG, also known as Indonesian Center for Volcanology and Geological Hazard Mitigation, CVGHM), Jalan Diponegoro 57, Bandung 40122, Indonesia (URL: http://www.vsi.esdm.go.id/); Darwin Volcanic Ash Advisory Centre (VAAC), Bureau of Meteorology, Northern Territory Regional Office, PO Box 40050, Casuarina, NT 0811, Australia (URL: http://www.bom.gov.au/info/vaac/); MIROVA (Middle InfraRed Observation of Volcanic Activity), a collaborative project between the Universities of Turin and Florence (Italy) supported by the Centre for Volcanic Risk of the Italian Civil Protection Department (URL: http://www.mirovaweb.it/); Sentinel Hub Playground (URL: https://www.sentinel-hub.com/explore/sentinel-playground).

Eruptive History

There is data available for 20 confirmed eruptive periods.

2022 Feb 17 - 2022 Feb 17 Confirmed Eruption (Explosive / Effusive) VEI: 2

Episode 1 | Eruption (Explosive / Effusive)
2022 Feb 17 - 2022 Feb 17 Evidence from Observations: Reported
 On 17 February ash plumes rose to altitudes of 4-4.9 km (2-3 km above the summit) and drifted SW and WSW.

List of 2 Events for Episode 1

Start Date End Date Event Type Event Remarks
2022 Feb 17    - - - - Ash Plume Ash plumes rose to altitudes of 4-4.9 km and drifted SW and WSW.
2022 Feb 17    - - - - VEI (Explosivity Index) VEI 2

2017 Feb 25 - 2020 Jun 10 Confirmed Eruption (Explosive / Effusive) VEI: 2

Episode 1 | Eruption (Explosive / Effusive) Summit crater, Doro Api cone
2017 Feb 25 - 2020 Jun 10 Evidence from Observations: Reported

List of 189 Events for Episode 1 at Summit crater, Doro Api cone

Start Date End Date Event Type Event Remarks
2017 Feb 25 2017 Feb 27 Thermal Anomaly Two MODVOLC thermal alerts were issued.
2017 Mar 6    - - - - Thermal Anomaly Two MODVOLC thermal alerts were issued.
2017 Mar 10    - - - - Thermal Anomaly A MODVOLC thermal alert was issued.
2017 Mar 13    - - - - Thermal Anomaly A MODVOLC thermal alert was issued.
2017 Mar 17    - - - - Thermal Anomaly Two MODVOLC thermal alerts were issued.
2017 Mar 24    - - - - Thermal Anomaly Three MODVOLC thermal alerts were issued.
2017 Mar 31    - - - - Thermal Anomaly A MODVOLC thermal alert was issued.
2017 Apr 9    - - - - Thermal Anomaly A MODVOLC thermal alert was issued.
2017 Apr 14 2017 Apr 18 Thermal Anomaly Seven MODVOLC thermal alerts were issued.
2017 Apr 27    - - - - Thermal Anomaly Three MODVOLC thermal alerts were issued.
2017 Apr 30 2017 May 2 Thermal Anomaly Four MODVOLC thermal alerts were issued.
2017 May 8    - - - - Degassing Based on HIMAWARI-8 and Pirep information, the Darwin VAAC noted a pilot report of ash at about 0000 UTC. Ash was not discernible in HIMAWARI-8 visible, IR or multispectral satellite imagery.
2017 May 9    - - - - Degassing Based on HIMAWARI-8 and Airep information, the Darwin VAAC noted ash was reported at 0915 UTC at 3.7 km altitude. Ash was unidentifiable on satellite imagery in mostly clear conditions.
2017 May 16 2017 May 20 Thermal Anomaly Three MODVOLC thermal alerts were issued.
2017 Jun 3 2017 Jun 5 Thermal Anomaly Five MODVOLC thermal alerts were issued.
2017 Jun 7    - - - - Degassing Based on HIMAWARI-8 information, the Darwin VAAC reported ash observed at 0920 UTC extending 75 km W at 2.1 km altitude. A possible minor eruption of ash was reported. A report from CVGHM at 1130 UTC indicates that the plume was likely a steam and gas emission. No seismic or ground observations indicate eruption of ash.
2017 Jun 10    - - - - Thermal Anomaly Three MODVOLC thermal alerts were issued.
2017 Jun 15    - - - - Thermal Anomaly A MODVOLC thermal alert was issued.
2017 Jun 21    - - - - Thermal Anomaly Two MODVOLC thermal alerts were issued.
2017 Jun 24 2017 Jun 30 Thermal Anomaly Nine MODVOLC thermal alerts were issued.
2017 Jul 3    - - - - Thermal Anomaly Two MODVOLC thermal alerts were issued.
2017 Jul 7 2017 Jul 9 Thermal Anomaly Seven MODVOLC thermal alerts were issued.
2017 Jul 12 2017 Jul 16 Thermal Anomaly Seven MODVOLC thermal alerts were issued.
2017 Jul 15    - - - - Ash Plume PVMBG reported a small eruption at Sangeang Api at 1154 characterized by Strombolian activity, and an ash plume that rose 100-200 m above the crater rim and drifted SW.
2017 Jul 15    - - - - Incandescent ejecta PVMBG reported a small eruption at Sangeang Api at 1154 characterized by Strombolian activity, and an ash plume that rose 100-200 m above the crater rim and drifted SW.
2017 Jul 15    - - - - Degassing Based VONA information, the Darwin VAAC noted an eruption reported at 0345 UTC moving SW at 2.1 km altitude. Ash was not identifiable in satellite imagery in clear conditions.
2017 Jul 16    - - - - Ash Plume Based on HIMAWARI-8 and CVGHM information, the Darwin VAAC reported ash observed at 0940 UTC extending NW at 2.1 km altitude. CVGHM reported an emission to 200 m above the summit. Ash was discernible and moving NW.
2017 Jul 19    - - - - Ash Plume Based on HIMAWARI-8, and CVGHM VONA information, the Darwin VAAC reported an ash emissions at 0758 UTC moving NW at 4.3 km altitude. Ash was observed moving NW in HIMAWARI-8 imagery at 0830 UTC at 2.4 km altitude. It was not identifiable in satellite imagery at 1140 UTC.
2017 Jul 19 2017 Jul 25 Thermal Anomaly Twelve MODVOLC thermal alerts were issued.
2017 Jul 19    - - - - VEI (Explosivity Index) VEI 2
2017 Jul 28 2017 Jul 30 Thermal Anomaly Ten MODVOLC thermal alerts were issued.
2017 Jul 29    - - - - Ash Plume Based on HIMAWARI-8 and Pirep information, the Darwin VAAC noted a pilot report of ash at 0853 UTC moving NW at 2.7 km altitude. Minor emissions could be seen on satellite imagery. Ash was last observed at 0940 UTC. Ash was unidentifiable on overnight imagery at 1520 UTC, but a hotspot was observed.
2017 Jul 30    - - - - Ash Plume Based on HIMAWARI-8 information, the Darwin VAAC reported discrete eruptions at 0220 UTC and 0830 UTC moving NW at 2.4 km altitude.
2017 Aug 6 2017 Aug 8 Thermal Anomaly Eight MODVOLC thermal alerts were issued.
2017 Aug 7    - - - - Ash Plume Based on HIMAWARI-8 information, the Darwin VAAC reported minor emissions at 0940 UTC moving WSW at 2.4 km altitude.
2017 Aug 11 2017 Aug 15 Thermal Anomaly Six MODVOLC thermal alerts were issued.
2017 Aug 12    - - - - Ash Plume Based on HIMAWARI-8 information, the Darwin VAAC reported ash observed at 0850 UTC extending NW at 2.7 km altitude. Ash was discernible on HIMAWARI-8 true color imagery.
2017 Aug 20 2017 Aug 24 Thermal Anomaly Eleven MODVOLC thermal alerts were issued.
2017 Aug 29 2017 Sep 2 Thermal Anomaly Ten MODVOLC thermal alerts were issued.
2017 Sep 7 2017 Sep 9 Thermal Anomaly Six MODVOLC thermal alerts were issued.
2017 Sep 14 2017 Sep 18 Thermal Anomaly Six MODVOLC thermal alerts were issued.
2017 Sep 23 2017 Sep 25 Thermal Anomaly Four MODVOLC thermal alerts were issued.
2017 Sep 30 2017 Oct 4 Thermal Anomaly Six MODVOLC thermal alerts were issued.
2017 Oct 9 2017 Oct 13 Thermal Anomaly Eleven MODVOLC thermal alerts were issued.
2017 Oct 16 2017 Oct 20 Thermal Anomaly Seven MODVOLC thermal alerts were issued.
2017 Oct 23 2017 Oct 27 Thermal Anomaly Seven MODVOLC thermal alerts were issued.
2017 Oct 30 2017 Nov 3 Thermal Anomaly Seven MODVOLC thermal alerts were issued.
2017 Nov 10 2017 Nov 12 Thermal Anomaly Four MODVOLC thermal alerts were issued.
2017 Nov 15 2017 Nov 19 Thermal Anomaly Five MODVOLC thermal alerts were issued.
2017 Nov 26    - - - - Thermal Anomaly Two MODVOLC thermal alerts were issued.
2017 Dec 3    - - - - Thermal Anomaly A MODVOLC thermal alert was issued.
2017 Dec 10 2017 Dec 14 Thermal Anomaly Five MODVOLC thermal alerts were issued.
2017 Dec 23    - - - - Thermal Anomaly A MODVOLC thermal alert was issued.
2018 Jan 4 2018 Jan 8 Thermal Anomaly Three MODVOLC thermal alerts were issued.
2018 Jan 15    - - - - Thermal Anomaly A MODVOLC thermal alert was issued.
2018 Feb 21 2018 Feb 25 Thermal Anomaly Three MODVOLC thermal alerts were issued.
2018 Mar 9 2018 Mar 11 Thermal Anomaly Eight MODVOLC thermal alerts were issued.
2018 Mar 16    - - - - Thermal Anomaly A MODVOLC thermal alert was issued.
2018 Mar 20    - - - - Thermal Anomaly Two MODVOLC thermal alerts were issued.
2018 Mar 27 2018 Apr 5 Thermal Anomaly Fifteen MODVOLC thermal alerts were issued.
2018 Apr 10 2018 Apr 12 Thermal Anomaly Four MODVOLC thermal alerts were issued.
2018 Apr 17 2018 Apr 19 Thermal Anomaly Three MODVOLC thermal alerts were issued.
2018 Apr 26    - - - - Thermal Anomaly A MODVOLC thermal alert was issued.
2018 Apr 30    - - - - Thermal Anomaly A MODVOLC thermal alert was issued.
2018 May 5 2018 May 12 Thermal Anomaly Six MODVOLC thermal alerts were issued.
2018 May 9    - - - - Ash Plume Based on CVGHM and HIMAWARI-8 information, at 1130 UTC the Darwin VAAC noted a report of an ash emission at 1007 UTC moving W at 4.3 km altitude. Minor ash/smoke was reported. Ash was not identifiable in satellite data. A hotspot was observed at the summit on NIR imagery.
2018 May 10    - - - - Avalanche Sentinel-2 satellite imagery indicated hot material extending more than a kilometer from the vent in the summit crater to the SE and onto the E flank.
2018 May 28 2018 May 30 Thermal Anomaly Four MODVOLC thermal alerts were issued.
2018 Jun 6 2018 Jun 8 Thermal Anomaly Four MODVOLC thermal alerts were issued.
2018 Jun 13    - - - - Thermal Anomaly Two MODVOLC thermal alerts were issued.
2018 Jun 17    - - - - Thermal Anomaly Two MODVOLC thermal alerts were issued.
2018 Jun 22    - - - - Thermal Anomaly A MODVOLC thermal alert was issued.
2018 Jun 27 2018 Jul 1 Thermal Anomaly Four MODVOLC thermal alerts were issued.
2018 Jul 6 2018 Jul 10 Thermal Anomaly Four MODVOLC thermal alerts were issued.
2018 Jul 15 2018 Jul 17 Thermal Anomaly Two MODVOLC thermal alerts were issued.
2018 Jul 22 2018 Jul 26 Thermal Anomaly Five MODVOLC thermal alerts were issued.
2018 Jul 31 2018 Aug 2 Thermal Anomaly Four MODVOLC thermal alerts were issued.
2018 Aug 13    - - - - Thermal Anomaly A MODVOLC thermal alert was issued.
2018 Aug 16 2018 Aug 18 Thermal Anomaly Five MODVOLC thermal alerts were issued.
2018 Aug 25 2018 Aug 27 Thermal Anomaly Two MODVOLC thermal alerts were issued.
2018 Sep 8    - - - - Thermal Anomaly Two MODVOLC thermal alerts were issued.
2018 Sep 12    - - - - Thermal Anomaly Three MODVOLC thermal alerts were issued.
2018 Sep 15 2018 Sep 21 Thermal Anomaly Twelve MODVOLC thermal alerts were issued.
2018 Sep 24 2018 Oct 1 Thermal Anomaly Nine MODVOLC thermal alerts were issued.
2018 Sep 25
(on or after)
2018 Oct 3
(on or before)
Explosion Photographer Martin Rietze provided excellent ground and drone-based photographic and video documentation of the eruptive activity (BGVN 44:05). Explosions produced volcanic bombs that traveled hundreds of meters down the flanks of Doro Api as well as sending lava fragments down all sides of the pyroclastic cone. Steaming tephra on the flanks of the pyroclastic cone was visible during daylight hours.
2018 Sep 25
(on or after)
2018 Oct 3
(on or before)
Fissure Photographer Martin Rietze provided excellent ground and drone-based photographic and video documentation of the eruptive activity (BGVN 44:05). Video footage showed incandescent lava emerging from a fissure near the base of the pyroclastic cone.
2018 Sep 25
(on or after)
2018 Oct 3
(on or before)
Ash Plume Photographer Martin Rietze provided excellent ground and drone-based photographic and video documentation of the eruptive activity (BGVN 44:05). Regular small ash emissions were recorded multiple times per day from a pyroclastic cone inside the Doro Api cone. Steam and ash rose a few hundred meters above the summit of the pyroclastic cone and was incandescent after dark.
2018 Sep 25
(on or after)
2018 Oct 3
(on or before)
Incandescent ejecta Photographer Martin Rietze provided excellent ground and drone-based photographic and video documentation of the eruptive activity (BGVN 44:05). Explosions produced volcanic bombs that traveled hundreds of meters down the flanks of Doro Api as well as sending lava fragments down all sides of the pyroclastic cone. Incandescent bombs and blocks from Strombolian activity cascaded down the flanks of the pyroclastic cone and also reached outside of the Doro Api crater, landing on the W flank. In a nighttime view of Doro Api as seen from the summit of Doro Mantai, the incandescent ejecta was clearly visible hundreds of meters from the erupting pyroclastic cone.
2018 Sep 25
(on or after)
2018 Oct 3 Lava flow Photographer Martin Rietze provided excellent ground and drone-based photographic and video documentation of the eruptive activity (BGVN 44:05). Video footage showed incandescent lava emerging from a fissure near the base of the pyroclastic cone.
2018 Sep 25
(on or after)
2018 Oct 3
(on or before)
Cinder Cone Photographer Martin Rietze provided excellent ground and drone-based photographic and video documentation of the eruptive activity (BGVN 44:05). Regular small ash emissions were recorded multiple times per day from a pyroclastic cone inside the Doro Api cone; the explosions produced volcanic bombs that traveled hundreds of meters down the flanks of Doro Api as well as sending lava fragments down all sides of the pyroclastic cone. Steam and ash rose a few hundred meters above the summit of the pyroclastic cone and was incandescent after dark. Incandescent bombs and blocks from Strombolian activity cascaded down the flanks of the pyroclastic cone and also reached outside of the Doro Api crater, landing on the W flank. Steaming tephra on the flanks of the pyroclastic cone was visible during daylight hours. In a nighttime view of Doro Api as seen from the summit of Doro Mantai, the incandescent ejecta is clearly visible hundreds of meters from the erupting pyroclastic cone. Video footage showed incandescent lava emerging from a fissure near the base of the pyroclastic cone, and a blocky avalanche on the E flank of the cone; as blocks rolled down the slope, incandescence was visible just below the surface.
2018 Sep 25
(on or after)
2018 Oct 3
(on or before)
Avalanche Photographer Martin Rietze provided excellent ground and drone-based photographic and video documentation of the eruptive activity (BGVN 44:05). Explosions produced volcanic bombs that traveled hundreds of meters down the flanks of Doro Api as well as sending lava fragments down all sides of the pyroclastic cone. Incandescent bombs and blocks from Strombolian activity cascaded down the flanks of the pyroclastic cone and also reached outside of the Doro Api crater, landing on the W flank. Video footage showed a blocky avalanche on the E flank of the cone; as blocks rolled down the slope, incandescence was visible just below the surface.
2018 Sep 25
(on or after)
2018 Oct 3
(on or before)
Tephra Photographer Martin Rietze provided excellent ground and drone-based photographic and video documentation of the eruptive activity (BGVN 44:05). Steaming tephra on the flanks of the pyroclastic cone was visible during daylight hours. In a nighttime view of Doro Api as seen from the summit of Doro Mantai, the incandescent ejecta is clearly visible hundreds of meters from the erupting pyroclastic cone.
2018 Sep 25
(on or after)
2018 Oct 3
(on or before)
Bombs Photographer Martin Rietze provided excellent ground and drone-based photographic and video documentation of the eruptive activity (BGVN 44:05). Explosions produced volcanic bombs that traveled hundreds of meters down the flanks of Doro Api as well as sending lava fragments down all sides of the pyroclastic cone. Incandescent bombs and blocks from Strombolian activity cascaded down the flanks of the pyroclastic cone and also reached outside of the Doro Api crater, landing on the W flank.
2018 Sep 25
(on or after)
2018 Oct 3
(on or before)
Incandescence Photographer Martin Rietze provided excellent ground and drone-based photographic and video documentation of the eruptive activity (BGVN 44:05). Steam and ash rose a few hundred meters above the summit of the pyroclastic cone and was incandescent after dark. Video footage showed incandescent lava emerging from a fissure near the base of the pyroclastic cone, and a blocky avalanche on the E flank of the cone; as blocks rolled down the slope, incandescence was visible just below the surface.
2018 Oct 1
(on or after)
2018 Oct 15
(on or before)
Avalanche Blocks of lava formed an avalanche down the ravine on the E flank of Doro Api; the avalanche formed channels tens of meters wide on the steep slope when photographed by drone in early October 2018.
2018 Oct 5 2018 Oct 7 Thermal Anomaly Eight MODVOLC thermal alerts were issued.
2018 Oct 7
(on or before)
   - - - - Observation A Google Earth image of the SE flank of Sangeang Api taken on 7 October 2018 shows dark channels of lava descending the ravine to within about 1 km of the shore.
2018 Oct 10 2018 Oct 14 Thermal Anomaly Six MODVOLC thermal alerts were issued.
2018 Oct 12    - - - - Avalanche Sentinel-2 satellite infrared images (Atmospheric Penetration rendering with bands 12, 11, and 8A) confirmed thermal activity at the summit crater and down the ravine on the E flank.
2018 Oct 15    - - - - Ash Plume Based on HIMAWARI-8 information, at 0000 UTC the Darwin VAAC reported ash observed at 2330 UTC on 14 October moving WSW at 2.1 km altitude. Ongoing discrete ash eruptions were observed on animated visible and RGB satellite imagery. At 0600 UTC they reported ongoing discrete ash observed at 0200 UTC moving W at 2.1 km altitude. At 0000 UTC on 16 October they reported ash last observed at 0920 UTC on 15 October at 2.1 km altitude.
2018 Oct 21    - - - - Thermal Anomaly Two MODVOLC thermal alerts were issued.
2018 Oct 26 2018 Oct 28 Thermal Anomaly Three MODVOLC thermal alerts were issued.
2018 Oct 27    - - - - Avalanche Sentinel-2 satellite infrared images (Atmospheric Penetration rendering with bands 12, 11, and 8A) confirmed thermal activity at the summit crater and down the ravine on the E flank.
2018 Oct 29    - - - - Ash Plume The PVMBG webcam located about 10 km SW on nearby Sumbawa island captured an ash emission from the Doro Api cone.
2018 Nov 1
(on or after)
2018 Nov 30
(on or before)
Fissure Visitors to the island in November recorded continued activity in the form of ash plumes and incandescent lava emerging from a fissure on the flank of the pyroclastic cone.
2018 Nov 1
(on or after)
2018 Nov 30
(on or before)
Ash Plume Visitors to the island in November recorded continued activity in the form of ash plumes and incandescent lava emerging from a fissure on the flank of the pyroclastic cone.
2018 Nov 1
(on or after)
2018 Nov 30
(on or before)
Incandescent ejecta Visitors to Sangeang Api in November 2018 witnessed incandescent bombs and lava emerging from a fissure on the flank of the pyroclastic cone inside Doro Api crater.
2018 Nov 1
(on or after)
2018 Nov 30
(on or before)
Lava flow Visitors to the island in November recorded continued activity in the form of ash plumes and incandescent lava emerging from a fissure on the flank of the pyroclastic cone.
2018 Nov 1
(on or after)
2018 Nov 30
(on or before)
Cinder Cone Visitors to Sangeang Api in November 2018 witnessed incandescent bombs and lava emerging from a fissure on the flank of the pyroclastic cone inside Doro Api crater.
2018 Nov 2 2018 Nov 6 Thermal Anomaly Five MODVOLC thermal alerts were issued.
2018 Nov 11 2018 Nov 13 Thermal Anomaly Three MODVOLC thermal alerts were issued.
2018 Nov 16    - - - - Avalanche Sentinel-2 satellite infrared images (Atmospheric Penetration rendering with bands 12, 11, and 8A) confirmed thermal activity at the summit crater and down the ravine on the E flank.
2018 Nov 18 2018 Nov 22 Thermal Anomaly Five MODVOLC thermal alerts were issued.
2018 Nov 25 2018 Nov 27 Thermal Anomaly Five MODVOLC thermal alerts were issued.
2018 Dec 3    - - - - Thermal Anomaly A MODVOLC thermal alert was issued.
2018 Dec 6 2018 Dec 8 Thermal Anomaly Seven MODVOLC thermal alerts were issued.
2018 Dec 21    - - - - Avalanche Sentinel-2 satellite infrared images (Atmospheric Penetration rendering with bands 12, 11, and 8A) confirmed thermal activity at the summit crater and down the ravine on the E flank.
2019 Jan 5 2019 Jan 12 Thermal Anomaly Seven MODVOLC thermal alerts were issued.
2019 Jan 30    - - - - Thermal Anomaly A MODVOLC thermal alert was issued.
2019 Feb 15 2019 Feb 19 Thermal Anomaly Eight MODVOLC thermal alerts were issued.
2019 Feb 24    - - - - Thermal Anomaly A MODVOLC thermal alert was issued.
2019 Mar 1 2019 Mar 3 Thermal Anomaly Two MODVOLC thermal alerts were issued.
2019 Mar 10 2019 Mar 12 Thermal Anomaly Two MODVOLC thermal alerts were issued.
2019 Mar 30 2019 Apr 1 Thermal Anomaly Four MODVOLC thermal alerts were issued.
2019 Apr 4 2019 Apr 6 Thermal Anomaly Two MODVOLC thermal alerts were issued.
2019 Apr 13    - - - - Thermal Anomaly A MODVOLC thermal alert was issued.
2019 Apr 18 2019 Apr 24 Thermal Anomaly Seven MODVOLC thermal alerts were issued.
2019 May 6 2019 May 8 Thermal Anomaly Four MODVOLC thermal alerts were issued.
2019 May 15 2019 May 19 Thermal Anomaly FIve MODVOLC thermal alerts were issued.
2019 May 20    - - - - Lava flow Sentinel-2 satellite thermal images show an active lava flow from the summit, traveling to the SE.
2019 May 24    - - - - Thermal Anomaly Two MODVOLC thermal alerts were issued.
2019 May 31    - - - - Thermal Anomaly Two MODVOLC thermal alerts were issued.
2019 Jun 2 2019 Jun 4 Thermal Anomaly Two MODVOLC thermal alerts were issued.
2019 Jun 7 2019 Jun 11 Thermal Anomaly Six MODVOLC thermal alerts were issued.
2019 Jun 9    - - - - Lava flow Sentinel-2 satellite thermal images show an active lava flow from the summit, traveling to the SE.
2019 Jun 14 2019 Jun 18 Thermal Anomaly Seven MODVOLC thermal alerts were issued.
2019 Jun 17    - - - - Ash Plume Based on HIMAWARI-8 information, at 0800 UTC the Darwin VAAC reported that multiple discrete eruptions were observed over the previous hour with increasing ash content. Ash was moving W at 2.1 km altitude. At 1055 UTC they reported that ash was not identifiable on satellite data under clear skies. Seismic activity had decreased but a hotspot remained.
2019 Jun 25 2019 Jun 27 Thermal Anomaly Four MODVOLC thermal alerts were issued.
2019 Jun 27    - - - - Ash Plume Based on HIMAWARI-8 information, at 0130 UTC the Darwin VAAC reported intermittent discrete eruptions observed in satellite imagery with ash moving NW at 2.1 km altitude. At 0730 UTC they reported intermittent discrete eruptions observed in satellite imagery with ash moving NW at 2.1 km altitude. A hotspot was visible in satellite imagery. At 1150 UTC they reported that ash was last observed at 0940 UTC extending NW at 2.1 km altitude.
2019 Jun 29    - - - - Ash Plume Based on VOLCAT and HIMAWARI-8 information, at 0040 UTC the Darwin VAAC reported a discrete ash puff moving NW at 2.4 km altitude with continuous steam emissions ongoing. At 0400 UTC they reported that ash was last observed at 0330 UTC moving NW at 2.4 km altitude.
2019 Jul 4    - - - - Ash Plume Based on VOLCAT and HIMAWARI-8 information, at 1407 UTC the Darwin VAAC reported a discrete ash puff moving SW at 2.1 km altitude observed at 1340 UTC. The ash cloud was observed on RGB and IR satellite imagery. A strong hotspot remained at the summit. At 1620 UTC they reported that ash was no longer identifiable from satellite data. Smoke/steam emissions remained likely due to a strong hotspot at the summit.
2019 Jul 4 2019 Jul 7 Thermal Anomaly Eleven MODVOLC thermal alerts were issued.
2019 Jul 5 2019 Jul 9 Ash Plume Based on HIMAWARI-8 and Pilot Report information, at 1240 UTC the Darwin VAAC reported intermittent ash emissions observed in satellite imagery with ash moving W at 2.4 km altitude. Ash was regularly discernible on RGB satellite imagery and quickly dissipating. At 1840 UTC they reported weak intermittent ash emissions regularly discernible on RGB satellite imagery with ash moving W at 2.4 km altitude and quickly dissipating. At 0040 UTC on 6 July they reported weak intermittent ash emissions regularly discernible on Visible satellite imagery with ash moving W at 2.4 km altitude and quickly dissipating. At 0257 UTC they reported intermittent ash emissions regularly discernible on Visible satellite imagery with ash moving NW at 4.6 km altitude and dissipating. At 0810 UTC they reported intermittent ash emissions discernible on visible satellite imagery radiating out to the N at 4.6 km altitude and dissipating. At 1405 UTC they reported multiple discrete ash emissions partially discernible on RGB satellite imagery moving N at 3.0 km altitude. At 2005 UTC they reported multiple discrete ash emissions partially discernible on RGB satellite imagery moving N at 3.0 km altitude. At 0200 UTC on 7 July they reported multiple discrete ash emissions partially discernible on recent satellite imagery moving NW at 3.0 km altitude and rapidly dissipating. At 0800 UTC they reported multiple discrete ash emissions partially discernible on recent satellite imagery moving NW at 3.0 km altitude and rapidly dissipating. At 1400 UTC they reported multiple discrete ash emissions discernible on RGB and IR satellite imagery moving NW at 3.0 km altitude and rapidly dissipating. At 1600 UTC they reported multiple discrete ash emissions NO LONGER discernible on satellite imagery due to meteoric clouds and darkness. At 0055 UTC on 8 July they reported continuous minor ash emissions observed on satellite imagery moving NNW at 3.0 km altitude and discrete ash emissions observed moving SW at 2.1 km altitude. At 0655 UTC they reported discrete ash emissions observed on satellite imagery moving NNW at 3.0 km alitutde. At 0954 UTC they reported discrete ash eruptions observed on satellite imagery at 0930 UTC moving NW at 3.0 km alitutde. Ash was also observed moving slowly S and E at 2.1 km altitude. At 1500 UTC they reported that discrete ash eruptions were last observed on satellite imagery at 1020 UTC moving NW at 3.0 km altitude. A large hotspot was observed at 1120 UTC. At 2100 UTC they reported that discrete ash eruptions were last observed on satellite imagery at 1950 UTC moving NW at 3.0 km altitude. The last hotspot was observed at 1840 UTC. At 0127 UTC on 9 July they reported that discrete ash eruptions were last observed on satellite imagery at 1950 UTC on 8 July moving NW at 3.0 km. altitude.
2019 Jul 11    - - - - Ash Plume Based on HIMAWARI-8 information, at 0046 UTC the Darwin VAAC reported continuous ash emissions discernible on visible satellite imagery with ash moving SW at 3.0 km altitude. At 0252 UTC they reported that ash was last observed in satellite imagery at 0230 UTC.
2019 Jul 11    - - - - Ash Plume Based on HIMAWARI-8 information, at 0941 UTC the Darwin VAAC reported a discrete eruption observed on satellite imagery at 0850 UTC with ash moving SW at 2.7 km altitude. At 1446 UTC they reported that ash was no longer identifiable in satellite imagery.
2019 Jul 11 2019 Jul 13 Thermal Anomaly Five MODVOLC thermal alerts were issued.
2019 Jul 12 2019 Jul 15 Ash Plume Based on HIMAWARI-8 information, at 0125 UTC the Darwin VAAC reported continuous ash emission extending NW at 2.1 km altitude observed in satellite imagery. The latest satellite imagery indicated that the ash content had increased. At 0725 UTC they reported that continuous ash emissions extending N and E at 3.0 km altitude were observed in satellite imagery. At 1325 UTC they reported ash observed in satellite imagery at 1300 UTC extending N at 2.4 km altitude. The plume height was lowered based on IR Temperature data. At 1925 UTC they reported ash observed in RGB satellite imagery at 1900 UTC extending N at 2.4 km altitude. At 0125 UTC on 13 July they reported continuous ash emissions observed in satellite imagery extending W at 2.4 km altitude. At 0725 UTC they reported continuous ash emissions observed in satellite imagery extending W at 2.4 km altitude. At 1325 UTC they reported ash emissions observed on RGB satellite imagery at 1300 extending W and SW at 2.4 km altitude. At 1925 UTC they reported ash emissions last observed on RGB satellite imagery at 1710 UTC extending WSW at 2.4 km altitude. At 0125 UTC on 14 July they reported continuous discrete eruptions with ash observed moving W at 2.4 km altitude on the latest visible and RGB satellite imagery. At 0710 UTC they reported continuous discrete eruptions with ash observed moving W at 2.4 km altitude on the latest visible and RGB satellite imagery. At 1310 UTC they reported continuous discrete eruptions with ash observed moving W at 2.4 km altitude on the latest RGB satellite imagery. At 1910 UTC they reported continuous discrete eruptions with ash observed moving W at 2.4 km altitude on the latest RGB satellite imagery. At 0110 UTC on 15 July they reported continuous discrete eruptions with ash observed moving W at 2.4 km altitude on the latest visible satellite imagery. At 0710 UTC they reported continuous discrete eruptions with ash observed moving W to SW at 2.4 km altitude on the latest visible satellite imagery. At 1310 UTC they reported continuous discrete eruptions with ash observed moving W to SW at 2.4 km altitude on the latest RGB satellite imagery. At 1910 UTC they reported that ash emission was not discernible due to meteoric clouds but expected to be ongoing. At 0110 UTC on 16 July they reported that ash emission was not discernible due to meteoric clouds but expected to be ongoing. At 0315 UTC they reported that ash was last observed moving W at 2.4 km altitude at 1320 UTC on 15 July. Only minor steam emissions remained.
2019 Jul 16 2019 Jul 17 Ash Plume Based on HIMAWARI-8 information, at 0750 UTC the Darwin VAAC reported minor discrete ash emissions discernible in satellite imagery extending SW at 2.4 km altitude and dissipating quickly. At 1350 UTC the Darwin VAAC reported minor discrete ash emissions were last observed in satellite imagery moving SW at 2.4 km altitude at 1020 UTC. A hotspot remained. At 1950 UTC they reported minor intermittent discrete ash emissions were last observed in satellite imagery moving SW at 2.4 km altitude at 1720 UTC. A hotspot remained. At 0150 UTC on 17 July they reported minor intermittent discrete ash emissions were last observed in satellite imagery moving SW at 2.4 km altitude at 2210 UTC on 16 July. A hotspot remained. At 0750 UTC they reported that ash emissions were last observed in satellite imagery moving SW at 2.4 km altitude at 2210 UTC on 16 July. Minor ongoing gas emissions remained.
2019 Jul 17 2019 Jul 18 Ash Plume Based on HIMAWARI-8 information, at 1005 UTC the Darwin VAAC reported intermittent discrete ash emissions observed on visible and RGB satellite imagery at 0940 UTC extending W to SW at 2.4 km altitude. At 1605 UTC they reported intermittent discrete ash emissions observed on visible and RGB satellite imagery at 1520 UTC extending W to SW at 2.4 km altitude. At 2205 UTC they reported intermittent discrete ash emissions observed on IR and RGB satellite imagery at 2150 UTC moving W to SW at 2.4 km altitude. At 0350 UTC on 18 July they reported that satellite imagery indicated that ash had dissipated.
2019 Jul 18    - - - - Ash Plume Based on HIMAWARI-8 information, at 0615 UTC the Darwin VAAC reported discrete ash emissions observed on satellite imagery moving WSW at 2.4 km altitude. At 1215 UTC they reported that multiple discrete ash emissions were last observed in satellite imagery at 0920 UTC moving W at 2.4 km altitude. A hotspot remained. At 1815 UTC they reported that multiple discrete ash emissions were last observed in satellite imagery at 0920 UTC moving W at 2.4 km altitude. At 0015 UTC on 19 July they reported that multiple discrete ash emissions were last observed in satellite imagery at 0920 UTC on 18 July moving W at 2.4 km altitude. At 0615 UTC they reported that multiple discrete ash emissions were last observed in satellite imagery at 0920 UTC on 18 July moving W at 2.4 km altitude. Ash was not discernible due to meteoric clouds. At 1018 UTC they reported that ash had not been discernible for the previous 24 hours.
2019 Jul 20 2019 Jul 25 Ash Plume Based on HIMAWARI-8 and PIREP information, at 0015 UTC the Darwin VAAC reported a discrete ash eruption observed in satellite imagery at 2320 UTC on 19 July moving WSW at 2.1 km altitude. The discrete ash cloud was observed on visible satellite imagery. At 0145 UTC they reported multiple minor discrete ash eruptions observed in satellite imagery at 0120 UTC moving W at 3.0 km altitude. PIREP reports ash to 4.6 km altitude but IR temp suggests 2.4. At 0730 UTC they reported multiple discrete ash eruptions observed in satellite imagery at 0700 UTC moving W at 4.3 km altitude. Plume height based on PIREP report at 0612 UTC. At 1330 UTC they reported that multiple discrete eruptions were last observed in satellite imagery at 1030 UTC moving W at 4.3 km altitude. At 1930 UTC they reported that multiple discrete eruptions were last observed in satellite imagery at 1030 UTC moving W at 4.3 km altitude. The plumes were weak and diffuse. At 0130 UTC on 21 July they reported that intermittent discrete ash emissions were observed in satellite imagery moving W at 3.7 km altitude. The plume height was dropped due to latest observed movement. At 0730 UTC they reported that intermittent discrete ash emissions were observed in satellite imagery moving W at 3.7 km altitude. At 1330 UTC they reported that intermittent ash emissions were observed in satellite imagery moving WNW at 3.7 km altitude. At 1930 UTC they reported that intermittent ash emissions were observed in satellite imagery moving WNW at 3.7 km altitude. At 0130 UTC on 22 July they reported that intermittent ash emissions were observed in visible satellite imagery moving WNW at 3.7 km altitude. At 0730 UTC they reported that intermittent ash emissions were observed in visible satellite imagery moving WNW at 3.7 km altitude. At 1330 UTC they reported that intermittent ash emissions were observed in IR/RGB satellite imagery moving WNW at 3.7 km altitude. At 1930 UTC they reported that intermittent ash emissions were observed in IR/RGB satellite imagery at 1820 UTC moving NW at 3.7 km altitude. At 0130 UTC on 23 July they reported that continuous discrete eruptions were observed in satellite imagery moving W to NW at 2.4 km altitude and dissipating. Height decreased based on ash movement and model winds. At 0730 UTC they reported that continuous discrete eruptions were observed in satellite imagery moving W to NW at 2.4 km altitude and dissipating. At 1330 UTC they reported that intermittent eruptions were observed in satellite imagery moving W at 2.4 km altitude and dissipating. At 1917 UTC they reported that intermittent eruptions were observed in satellite imagery moving W at 2.4 km altitude and dissipating. At 0105 UTC on 24 July they reported that intermittent eruptions were observed in satellite imagery at 0050 UTC moving W at 2.4 km altitude and dissipating. At 0705 UTC they reported that intermittent eruptions were observed in satellite imagery at 0640 UTC moving W at 2.4 km altitude and dissipating. At 1005 UTC they reported that intermittent eruptions were observed in satellite imagery moving W and SW at 2.4 km altitude and dissipating quickly. At 1605 UTC they reported that intermittent eruptions were observed in satellite imagery moving W and SW at 2.4 km altitude before dissipating quickly. At 2205 UTC they reported that intermittent eruptions were observed in satellite imagery moving WSW at 3.0 km altitude before dissipating quickly. At 0405 UTC on 25 July they reported that satellite imagery indicated that ash had dissipated. Only minor smoke emissions remained.
2019 Jul 20 2019 Jul 27 Thermal Anomaly Seven MODVOLC thermal alerts were issued.
2019 Jul 25 2019 Aug 24 Ash Plume Based on HIMAWARI-8 information, at 1200 UTC the Darwin VAAC reported intermittent eruption observed on satellite imagery moving W at 2.4 km altitude and dissipating. At 1800 UTC they reported intermittent eruptions observed on satellite imagery moving W at 2.4 km altitude and dissipating. At 0000 UTC on 26 July they reported intermittent eruptions observed on satellite imagery moving W at 2.4 km altitude and dissipating. At 0551 UTC they reported intermittent eruptions observed on satellite imagery moving W at 2.4 km altitude and dissipating. At 1151 UTC they reported regular intermittent eruptions observed on satellite imagery moving WSW at 2.4 km altitude and quickly dissipating. At 1751 UTC they reported regular intermittent eruptions observed on satellite imagery moving WSW at 2.4 km altitude and quickly dissipating. At 2311 UTC they reported regular intermittent eruptions observed on satellite imagery moving WSW at 2.4 km altitude and quickly dissipating. At 2330 UTC they reported regular intermittent eruptions observed on satellite imagery moving WSW at 2.4 km altitude and quickly dissipating. At 0526 UTC on 27 July they reported regular intermittent eruptions observed on satellite imagery moving NW at 2.4 km altitude and quickly dissipating. At 1126 UTC they reported regular intermittent weak eruptions observed on RGB satellite imagery moving NNW at 2.4 km altitude and quickly dissipating. At 1726 UTC they reported regular intermittent weak eruptions observed on RGB satellite imagery moving N at 2.4 km altitude and quickly dissipating. At 2326 UTC they reported regular intermittent weak eruptions observed on RGB and visible satellite imagery moving NW at 2.4 km altitude and quickly dissipating. At 0526 UTC on 28 July they reported regular intermittent weak eruptions observed on RGB and visible satellite imagery moving WNW at 2.4 km altitude and quickly dissipating. At 1126 UTC they reported regular intermittent weak eruptions observed on RGB and visible satellite imagery moving WNW at 2.4 km altitude and quickly dissipating. At 1726 UTC they reported regular intermittent weak eruptions observed on RGB and visible satellite imagery moving WNW at 2.4 km altitude and quickly dissipating. At 2326 UTC they reported regular intermittent weak eruptions last observed on satellite imagery at 0930. Regular hotspots observed at summit. At 0526 UTC on 29 July they reported regular intermittent weak eruptions observed on satellite imagery moving WNW at 2.4 km altitude and quickly dissipating. Regular hotspots were observed at the summit. At 1126 UTC they reported regular intermittent weak eruptions observed on satellite imagery moving WNW at 2.4 km altitude and quickly dissipating. At 1725 UTC they reported regular intermittent weak eruptions observed on RGB satellite imagery moving WNW at 2.4 km altitude and quickly dissipating. At 2325 UTC they reported regular intermittent weak eruptions observed on RGB satellite imagery moving WNW at 2.4 km altitude and quickly dissipating. At 0525 UTC on 30 July they reported regular intermittent weak eruptions observed on RGB satellite imagery moving WNW at 2.4 km altitude and quickly dissipating. At 1125 UTC they reported regular intermittent weak eruptions last identifiable in satellite imagery at 0940 UTC moving WNW at 2.4 km altitude and quickly dissipating. At 1725 UTC they reported regular intermittent weak eruptions last identifiable in satellite imagery at 0940 UTC moving WNW at 2.4 km altitude and quickly dissipating. At 2300 UTC they reported regular intermittent weak eruptions observed on satellite imagery moving WNW at 2.4 km altitude and quickly dissipating. At 0500 UTC on 31 July they reported regular intermittent weak eruptions observed on satellite imagery moving W at 2.4 km altitude and quickly dissipating. At 1100 UTC they reported regular intermittent weak eruptions observed on satellite imagery moving W at 2.4 km altitude and quickly dissipating. At 1700 UTC they reported regular intermittent weak eruptions discernible on multispectral satellite imagery moving WSW at 2.4 km altitude and quickly dissipating. At 2300 UTC they reported regular intermittent weak eruptions discernible on multispectral satellite imagery moving WSW at 2.4 km altitude and quickly dissipating. At 0500 UTC on 1 August they reported regular intermittent weak eruptions observed on visible satellite imagery moving W at 2.4 km altitude and quickly dissipating. At 1100 UTC they reported regular intermittent weak eruptions observed on visible satellite imagery moving W at 2.4 km altitude and quickly dissipating. At 1700 UTC they reported regular intermittent weak eruptions observed on visible satellite imagery moving W at 2.4 km altitude and quickly dissipating. At 2300 UTC they reported regular intermittent weak eruptions observed on visible satellite imagery moving NW at 2.4 km altitude and quickly dissipating. At 0500 UTC on 2 August they reported regular intermittent weak eruptions observed on visible satellite imagery moving NW at 2.4 km altitude and quickly dissipating. At 1043 UTC they reported regular intermittent weak eruptions observed on visible satellite imagery moving NW at 2.4 km altitude and quickly dissipating. At 1643 UTC they reported regular intermittent weak eruptions observed on satellite imagery moving NW at 2.4 km altitude and quickly dissipating. At 2233 UTC they reported regular intermittent weak eruptions were last observed on visible satellite imagery at 1700 UTC moving NW at 2.4 km altitude and quickly dissipating. At 0433 UTC on 3 August they reported regular intermittent weak eruptions were last observed on satellite imagery at 0300 UTC moving NW at 2.4 km altitude and quickly dissipating. At 1033 UTC they reported regular intermittent weak eruptions were last observed on satellite imagery at 0900 UTC moving W and NW at 2.4 km altitude and quickly dissipating. At 1633 UTC they reported regular intermittent weak eruptions were last observed on RGB satellite imagery at 1600 UTC moving W at 2.4 km altitude and quickly dissipating. At 2233 UTC they reported regular intermittent weak eruptions were last observed on RGB satellite imagery at 1600 UTC moving W at 2.4 km altitude and quickly dissipating. At 0433 UTC on 4 August they reported regular intermittent weak eruptions observed on RGB satellite imagery moving SW at 2.4 km altitude and quickly dissipating. At 1033 UTC they reported regular intermittent weak eruptions observed on RGB satellite imagery moving W at 2.4 km altitude and quickly dissipating. At 1620 UTC they reported regular intermittent weak eruptions observed on RGB satellite imagery moving SW at 2.4 km altitude and quickly dissipating. At 2220 UTC they reported regular intermittent weak eruptions observed on RGB satellite imagery moving SW at 2.4 km altitude and quickly dissipating. At [0420] UTC on 5 August they reported weak eruptions observed on visible satellite imagery moving SE at 3.0 km altitude. Top height updated based on latest HIMAWARI-8 visible image. At 0115 UTC on 5 August they reported weak eruptions observed on visible satellite imagery moving SE at 3.0 km altitude. At 0715 UTC they reported intermittent ash observed on satellite imagery at 0640 UTC moving SE at 3.0 km altitude. At 1315 UTC they reported intermittent ash partially discernible on satellite imagery at 1250 UTC moving SE at 3.0 km altitude. At 1915 UTC they reported a weak ash signal in small discrete puffs discernible on satellite imagery at 1850 UTC moving SE at 3.0 km altitude and quickly dissipating. At 0115 UTC on 8 August they reported a weak ash signal in small discrete puffs discernible on satellite imagery at 0050 UTC moving SW at 2.4 km altitude and quickly dissipating. At 0715 UTC they reported a weak ash signal in small discrete puffs discernible on satellite imagery at 0650 UTC moving SW at 2.4 km altitude and quickly dissipating. At 1317 UTC they reported a weak ash signal in small discrete puffs discernible on satellite imagery moving S at 2.4 km altitude and quickly dissipating. At 1919 UTC they reported a weak ash signal in small discrete puffs discernible on multispectral satellite imagery moving W at 2.4 km altitude and quickly dissipating. At 0119 UTC on 7 August they reported a weak ash signal in small discrete puffs discernible on multispectral satellite imagery moving SE at 2.4 km altitude. At 0240 UTC they reported a weak ash signal in small discrete puffs discernible on multispectral satellite imagery moving SE at 2.4 km altitude. At 0840 UTC they reported a weak ash signal in small discrete puffs discernible on multispectral satellite imagery moving SE at 2.4 km altitude. At 1440 UTC they reported a weak ash signal in small discrete puffs discernible on multispectral satellite imagery moving S at 2.4 km altitude. At 1943 UTC they reported a weak ash signal in small discrete puffs discernible on multispectral satellite imagery moving S at 2.4 km altitude. At 0140 UTC on 8 August they reported a weak ash signal in small discrete puffs discernible on multispectral satellite imagery moving S at 2.4 km altitude. At 0740 UTC they reported a weak ash signal in small discrete puffs discernible on multispectral satellite imagery moving E at 2.4 km altitude. At 1340 UTC they reported a weak ash signal in small discrete puffs discernible on multispectral satellite imagery moving SE at 2.4 km altitude. At 1929 UTC they reported a weak ash signal in small discrete puffs discernible on multispectral satellite imagery moving E at 2.4 km altitude. At 0129 UTC on 9 August they reported continuous discrete emissions observed on visible satellite imagery moving E at 2.4 km altitude and dissipating. At 0729 UTC they reported continuous discrete emissions observed on visible satellite imagery moving E at 2.4 km altitude and dissipating. At 1329 UTC they reported continuous discrete emissions observed on RGB satellite imagery moving E at 2.4 km altitude and dissipating. At 1929 UTC they reported continuous discrete emissions observed on RGB satellite imagery moving E at 2.4 km altitude and dissipating. At 0129 UTC on 10 August they reported continuous discrete emissions observed on visible satellite imagery moving SW at 2.4 km altitude and dissipating. At 0700 UTC they reported continuous discrete weak emissions observed at 0630 UTC on visible satellite imagery moving SW at 2.4 km altitude and dissipating. At 1300 UTC they reported that ash emissions were last observed at 0920 UTC on satellite imagery moving SW at 2.4 km altitude. Ash was not discernible in satellite imagery due to meteoric clouds and darkness. At 1313 UTC they reported that ash emissions were last observed at 0920 UTC on satellite imagery moving SW at 2.4 km altitude. Ash was not discernible in satellite imagery due to meteoric clouds and darkness. At 1913 UTC they reported that ash emissions were last observed at 0920 UTC on satellite imagery moving SW at 2.4 km altitude. Ash was not discernible in satellite imagery due to meteoric clouds and darkness. At 0113 UTC on 11 August they reported that ash emissions were last observed at 0920 UTC on 10 August on satellite imagery moving SW at 2.4 km altitude. Ash was not discernible in satellite imagery due to meteoric clouds. At 0713 UTC they reported that ash emissions were last observed at 0700 UTC on satellite imagery moving SW at 2.4 km altitude. At 0905 UTC they reported that ash emissions were last observed at 0850 UTC on satellite imagery moving SSW at 2.4 km altitude. At 1455 UTC they reported a discrete ash eruption observed at 1430 UTC on RGB satellite imagery moving S at up to 3.0 km altitude. Plume height increased to 3.0 km altitude based on southward ash movement. At 2030 UTC they reported that ash was not discernible in satellite imagery due to meteoric clouds and darkness. Ash was last observed in satellite imagery moving S at 3.0 km altitude at 1430 UTC. At 0230 UTC on 12 August they reported that ash was not discernible in satellite imagery due to meteoric clouds and darkness. Ash was last observed in satellite imagery moving S at 3.0 km altitude at 1430 UTC on 11 August. At 0825 UTC they reported that intermittent ash emissions were partially discernible on visible satellite imagery extending W at 3.0 km altitude. At 1425 UTC they reported that ash was not identifiable on satellite imagery due to meteoric clouds and darkness. A hotspot remained. At 2025 UTC they reported that ash was not identifiable on satellite imagery due to meteoric clouds and darkness. A hotspot remained. At 0225 UTC on 13 August they reported that ash was partially identifiable on satellite imagery at 3.0 km altitude. Regular episodes of high seismicity were reported. At 0825 UTC they reported that ash was partially identifiable on satellite imagery moving W at 3.0 km altitude. Regular episodes of high seismicity were reported. At 1425 UTC they reported that ash was partially discernible on satellite imagery observed moving W at 3.0 km altitude at 1400 UTC. At 2025 UTC they reported that ash was partially discernible on RGB satellite imagery observed moving W at 3.0 km altitude at 2000 UTC. At 0215 UTC on 14 August they reported that ash was last observed on satellite imagery moving W at 3.0 km altitude at 2000 UTC on 23 August. At 0815 UTC they reported minor weak ash emissions observed on satellite imagery moving W at 3.0 km altitude and quickly dissipating. At 1240 UTC they reported ash emissions observed on satellite imagery at 1240 UTC moving W at 3.0 km altitude. At 2012 UTC they reported regular intermittent ash emissions last observed on RGB satellite imagery at 1720 UTC moving W at 3.0 km altitude. At 0212 UTC on 15 August they reported regular intermittent ash emissions observed on visible satellite imagery at 0410 UTC moving W at 3.0 km altitude. At 0812 UTC on they reported regular intermittent ash emissions observed on visible and RGB satellite imagery moving W at 3.0 km altitude. At 1404 UTC they reported regular intermittent ash emissions observed on RGB satellite imagery moving W at 3.0 km altitude and quickly dissipating. At 1946 UTC they reported regular intermittent ash emissions observed on RGB satellite imagery moving W at 3.0 km altitude and quickly dissipating. At 0146 UTC on 16 August they reported regular intermittent ash emissions observed on RGB satellite imagery moving W at 3.0 km altitude and quickly dissipating. At 0746 UTC they reported regular intermittent ash emissions observed on RGB satellite imagery moving W at 3.0 km altitude and quickly dissipating. At 1345 UTC they reported regular intermittent ash emissions observed on RGB satellite imagery moving W at 3.0 km altitude and quickly dissipating. At 1945 UTC they reported regular intermittent ash emissions observed on RGB satellite imagery moving W at 3.0 km altitude and quickly dissipating. At 0145 UTC on 17 August they reported regular intermittent ash emissions discernible on visible and RGB satellite imagery moving NW at 3.0 km altitude and quickly dissipating. At 0745 UTC they reported regular intermittent ash emissions observed on visible satellite imagery moving NW at 3.0 km altitude and quickly dissipating. At 1345 UTC they reported regular intermittent ash emissions observed on visible satellite imagery moving NW at 3.0 km altitude and quickly dissipating. At 1945 UTC they reported regular intermittent ash emissions observed on RGB satellite imagery moving WNW at 3.0 km altitude and quickly dissipating. At 0145 UTC on 18 August they reported regular intermittent ash emissions observed on visible satellite imagery moving W at 3.0 km altitude and quickly dissipating. At 0745 UTC they reported regular intermittent ash emissions observed on visible satellite imagery moving W at 2.4 km altitude and quickly dissipating. At 1345 UTC they reported regular intermittent ash emissions observed on RGB satellite imagery moving WSW at 3.0 km altitude and quickly dissipating. At 1945 UTC they reported regular intermittent ash emissions discernible on RGB satellite imagery moving W at 2.4 km altitude and quickly dissipating. At 0145 UTC on 19 August they reported regular intermittent ash emissions observed on visible satellite imagery moving W at 2.4 km altitude and quickly dissipating. At 0745 UTC they reported regular intermittent ash emissions observed on visible satellite imagery moving SW at 3.0 km altitude and quickly dissipating. At 1345 UTC they reported regular intermittent ash emissions moving W at 3.0 km altitude and quickly dissipating. At 1945 UTC they reported regular intermittent ash emissions discernible on satellite imagery moving WSW at 2.4 km altitude and quickly dissipating. At 0145 UTC on 20 August they reported regular intermittent ash emissions observed on satellite imagery moving W at 3.0 km altitude and quickly dissipating. At 0745 UTC they reported regular intermittent ash emissions observed on satellite imagery moving W at 3.0 km altitude and quickly dissipating. At 1345 UTC they reported regular intermittent ash emissions observed at 1310 UTC moving W at 3.0 km altitude and quickly dissipating. At 1945 UTC they reported a discrete eruption moving W at 3.0 km altitude last observed in satellite imagery at 1710 UTC. At 0145 UTC on 21 August they reported that ash was not discernible on latest satellite imagery due to meteoric clouds. At 0745 UTC they reported that ash was not discernible on latest satellite imagery due to meteoric clouds. Emissions were last observed in satellite imagery moving W at 3.0 km altitude at 0520 UTC. At 1345 UTC they reported that ash was not discernible on latest satellite imagery due to meteoric clouds and darkness. Emissions were last observed in satellite imagery moving W at 3.0 km altitude at 0520 UTC. At 1945 UTC they reported that ash was not discernible on latest satellite imagery due to meteoric clouds and darkness. Emissions were last observed in satellite imagery moving W at 3.0 km altitude at 0520 UTC. At 0145 UTC on 22 August they reported that discrete ash emissions were observed in satellite imagery at 0120 UTC extending W at 3.0 km altitude. At 0745 UTC they reported that discrete ash emissions were observed in satellite imagery at 0200 UTC extending W at 3.0 km altitude. At 1245 UTC they reported that discrete ash emissions were last observed in satellite imagery at 0230 UTC extending W at 3.0 km altitude. At 1845 UTC they reported that discrete ash emissions were last observed in satellite imagery at 0230 UTC extending W at 3.0 km altitude. Ash was not discernible on the latest satellite imagery. At 0045 UTC on 23 August they reported that discrete ash emissions were observed in satellite imagery at 0020 UTC extending W at 3.0 km altitude. At 0645 UTC they reported that discrete ash emissions were observed in satellite imagery at 0020 UTC extending W at 3.0 km altitude and dissipating. At 1245 UTC they reported that discrete ash emissions were last observed in satellite imagery at 0610 UTC extending W at 3.0 km altitude and dissipating. They were not discernible on the latest satellite imagery due to darkness. At 1845 UTC they reported that discrete ash emissions were last observed in satellite imagery at 0610 UTC extending W at 3.0 km altitude and dissipating. They were not discernible on the latest satellite imagery due meteoric clouds but were still expected. At 0020 UTC on 24 August they reported that ash emissions were last observed in satellite imagery at 0610 UTC on 23 August extending W at 3.0 km altitude and dissipating. Satellite imagery in clear conditions indicated that ash had dissipated.
2019 Jul 31    - - - - Thermal Anomaly Two MODVOLC thermal alerts were issued.
2019 Aug 7    - - - - Thermal Anomaly A MODVOLC thermal alert was issued.
2019 Aug 10    - - - - Ash Plume Based on HIMAWARI-8 information, at 0700 UTC the Darwin VAAC reported discrete ash emissions observed at 0630 UTC on visible satellite imagery moving S at 3.0 km altitude, expected to dissipate within 1 hour.
2019 Aug 10    - - - - Thermal Anomaly A MODVOLC thermal alert was issued.
2019 Aug 23    - - - - Avalanche Thermal anomalies revealed evidence of hot avalanches in Sentinel-2 thermal satellite imagery.
2019 Aug 24 2019 Sep 3 Ash Plume Based on HIMAWARI-8 information, at 0830 UTC the Darwin VAAC reported discrete ash emissions observed on satellite imagery at 0800 UTC moving W at 3.0 km altitude and dissipating. At 1442 UTC they reported that ash was not identifiable in satellite imagery due to meteoric clouds however ash was still expected. At 1956 UTC they reported that ash was not identifiable in satellite imagery due to meteoric clouds however ash was still expected. At 0156 UTC on 25 August they reported that weak discrete ash emissions were observed in satellite imagery moving NW at 3.0 km altitude. At 0756 UTC they reported that weak discrete ash emissions were observed in satellite imagery moving WNW at 3.0 km altitude. At 1356 UTC on they reported that weak discrete ash emissions were last observed in satellite imagery moving WNW at 3.0 km altitude at 0920 UTC. Ash was not discernible on satellite imagery. At 1956 UTC on they reported that weak discrete ash emissions were last observed in satellite imagery moving NW at 3.0 km altitude at 0920 UTC. Ash was not discernible on satellite imagery. At 0156 UTC on 26 August they reported that intermittent emissions as high as 3.0 km altitude continued moving W observed in satellite imagery. At 0756 UTC they reported that intermittent emissions as high as 3.0 km altitude continued moving W observed in satellite imagery. At 1356 UTC they reported that intermittent discrete emissions up to 3.0 km altitude were last observed at 0930 UTC. At 1956 UTC they reported that intermittent discrete emissions to 3.0 km altitude were last observed at 0930 UTC and expected to continue. At 0155 UTC on 27 August they reported that continuous discrete eruptions with ash observed moving WNW at up to 3.0 km altitude and dissipating were observed in satellite imagery at 0130 UTC. At 0755 UTC they reported that continuous weak discrete eruptions with ash observed moving WNW at up to 3.0 km altitude and dissipating were observed in satellite imagery at 0730 UTC. At 1355 UTC they reported that continuous weak discrete eruptions with ash observed moving WNW at up to 3.0 km altitude and dissipating were observed in satellite imagery. At 1955 UTC they reported that continuous weak discrete emissions with ash observed moving WNW at up to 3.0 km altitude and dissipating were observed in satellite imagery. At 0155 UTC on 28 August they reported that ash was unidentifiable in satellite imagery due to meteoric clouds. At 0755 UTC they reported that continuous weak discrete eruptions with ash observed moving W at up to 3.0 km altitude and dissipating were observed in satellite imagery. At 1355 UTC they reported that intermittent ash emissions moving W at up to 3.0 km altitude were observed in satellite imagery. At 1955 UTC they reported that intermittent discrete ash emissions moving W at up to 3.0 km altitude were observed in satellite imagery. At 0155 UTC on 29 August they reported that intermittent discrete ash emissions moving W at up to 3.0 km altitude were observed in satellite imagery. At 0755 UTC they reported that weak intermittent discrete ash emissions moving W at up to 3.0 km altitude were observed in satellite imagery. At 1355 UTC they reported that ash was unidentifiable on satellite imagery due to darkness. At 1955 UTC they reported that ash was unidentifiable on satellite imagery due to meteoric clouds and darkness. At 0155 UTC on 30 August they reported that weak intermittent eruptions with ash moving W at up to 3.0 km altitude were observed in satellite imagery. At 0755 UTC they reported that weak intermittent eruptions with ash moving SW at up to 3.0 km altitude were observed in satellite imagery. At 1354 UTC they reported that weak intermittent eruptions with ash moving SW at up to 3.0 km altitude were observed in satellite imagery. At 1954 UTC they reported that weak intermittent eruptions with ash moving SW at up to 3.0 km altitude were observed in satellite imagery. At 0154 UTC on 31 August they reported that weak intermittent eruptions with ash moving SW at up to 3.0 km altitude were observed in satellite imagery. At 0743 UTC they reported that weak intermittent eruptions with ash moving SW at up to 3.0 km altitude were observed in satellite imagery. At 1342 UTC they reported that weak intermittent eruptions with ash moving SW at up to 3.0 km altitude were observed in satellite imagery. At 1942 UTC they reported that weak intermittent eruptions with ash moving SW at up to 3.0 km altitude were observed in satellite imagery. At 0142 UTC on 1 September they reported that weak intermittent eruptions with ash moving SW at up to 3.0 km altitude were observed in satellite imagery. At 0742 UTC they reported that discrete ash emission were observed moving W at 3.0 km altitude at 0640 UTC on visible satellite imagery. At 1342 UTC they reported that weak intermittent eruptions with ash moving W at up to 3.0 km altitude were observed in satellite imagery. At 1932 UTC they reported that weak intermittent eruptions with ash moving NW at up to 3.0 km altitude were observed in satellite imagery. At 0132 UTC on 2 September they reported that discrete weak ash emission were observed moving NW at 3.0 km altitude at 0100 UTC on visible satellite imagery. At 0732 UTC they reported that discrete weak ash emission were observed moving NW at 3.0 km altitude at 0700 UTC on visible satellite imagery. At 1331 UTC they reported that weak intermittent eruptions with ash moving N at up to 3.0 km altitude were observed in satellite imagery. At 1920 UTC they reported that weak intermittent eruptions with ash moving N at up to 3.0 km altitude were observed in satellite imagery. At 0120 UTC on 3 September they reported that ash was discernible moving N at 3.0 km altitude at 0000 UTC on satellite imagery. At 0720 UTC they reported that ash was last observed moving N at 3.0 km altitude at 0010 UTC. At 1320 UTC they reported that minor ash was last observed close to the summit moving S at 0930 UTC, and had dissipated. Minor smoke emissions continued.
2019 Aug 26    - - - - Thermal Anomaly Three MODVOLC thermal alerts were issued.
2019 Sep 4    - - - - Thermal Anomaly A MODVOLC thermal alert was issued.
2019 Sep 5 2019 Sep 7 Ash Plume Based on HIMAWARI-8 information, at 1030 UTC the Darwin VAAC reported weak intermittent ash emissions observed on satellite imagery moving S at 3.0 km altitude. At 1619 UTC they reported weak intermittent ash emissions moving SSE at 3.0 km altitude. Ash was not identifiable in satellite imagery due to meteoric clouds. Intermittent hotspots indicate discrete eruption were likely continuing. At 0400 UTC on 6 September they reported weak intermittent ash emissions moving SE at 3.0 km altitude observed on visible satellite imagery. At 1000 UTC they reported continuous discrete weak ash emissions moving SE at 3.0 km altitude and dissipating observed on visible satellite imagery. At 1600 UTC they reported discrete ash emissions last observed moving S at 3.0 km altitude at 1000 UTC. At 2200 UTC they reported discrete ash emissions last observed moving S at 3.0 km altitude at 1000 UTC. At 0400 UTC on 7 September they reported discrete ash emissions last observed moving S at 3.0 km altitude. At 1000 UTC they reported minor weak ash emissions moving S at 3.0 km altitude and dissipating at 0930 UTC. At 1600 UTC they reported minor weak ash emissions moving S at 3.0 km altitude and dissipating last observed at 0930 UTC. At 2200 UTC they reported minor weak ash emissions moving S at 3.0 km altitude and dissipating last observed at 0930 UTC. At 0400 UTC on 8 September they reported minor weak ash emissions moving S at 3.0 km altitude and dissipating last observed at 0930 UTC on 7 September.
2019 Sep 9    - - - - Avalanche Thermal anomalies were evidence of hot avalanches in Sentinel-2 thermal satellite imagery.
2019 Sep 11    - - - - Ash Plume Based on HIMAWARI-8 information, at 1008 UTC the Darwin VAAC reported a minor weak ash eruption observed on RGB satellite imagery moving N at 3.0 km altitude. At 1552 UTC they reported that ash was last observed at 1030 UTC moving N at 3.0 km altitude.
2019 Sep 12    - - - - Avalanche Thermal anomalies were evidence of hot avalanches.
2019 Sep 22    - - - - Avalanche Thermal anomalies were evidence of hot avalanches in Sentinel-2 thermal satellite imagery.
2019 Sep 27    - - - - Avalanche Thermal anomalies were evidence of hot avalanches in Sentinel-2 thermal satellite imagery.
2019 Oct 6    - - - - Thermal Anomaly A MODVOLC thermal alert was issued.
2019 Oct 7    - - - - Lava flow Sentinel-2 satellite thermal images of Sangeang Api showed an area of elevated temperatures trending from the summit of the active cone down the SE flank.
2019 Oct 15    - - - - Thermal Anomaly Two MODVOLC thermal alerts were issued.
2019 Oct 22    - - - - Lava flow Sentinel-2 satellite thermal images of Sangeang Api showed an area of elevated temperatures trending from the summit of the active cone down the SE flank.
2019 Oct 22    - - - - Thermal Anomaly Two MODVOLC thermal alerts were issued.
2019 Oct 26    - - - - Ash Plume Based on HIMAWARI-8 information, at 1130 UTC the Darwin VAAC reported discrete ash emissions observed on animated RGB imagery, moving NW at 2.1 km altitude and dissipating about 25 km NW. At 1730 UTC they reported that ash was not identified on current satellite imagery but regular discrete ash eruptions had occurred over the previous six hours, dissipating about 25 km from the summit. Regular hotspots were observed. At 2255 UTC they reported that ash was last observed in satellite imagery at 1320 UTC at 2.1 m altitude. Minor steam emissions remained.
2019 Oct 27 2019 Oct 28 Ash Plume Based on HIMAWARI-8 information, at 0800 UTC the Darwin VAAC reported multiple discrete ash emissions observed on satellite imagery, moving NW at 2.1 km altitude and dissipating quickly. At 1400 UTC they reported regular discrete ash emissions observed on RGB satellite imagery moving W at 2.1 km altitude and dissipating rapidly. At 2000 UTC they reported regular discrete ash emissions observed on RGB satellite imagery moving W at 2.1 km altitude and dissipating rapidly. At 0200 UTC on 28 October they reported regular minor discrete ash emissions observed on visible and RGB satellite imagery moving WNW at 2.1 km altitude and dissipating rapidly. At 0700 UTC they reported that ash was last observed in satellite imagery at 0230 UTC and had dissipated. Minor steam emissions remained.
2019 Oct 28 2019 Nov 1 Ash Plume Based on HIMAWARI-8 information, at 0810 UTC the Darwin VAAC reported multiple discrete ash emissions clearly discernible on satellite imagery, moving NW at 2.1 km altitude. At 1320 UTC they reported regular discrete ash emissions observed on RGB satellite imagery moving W at 2.7 km altitude and dissipating rapidly. At 1920 UTC they reported minor discrete ash emissions observed on RGB satellite imagery moving W at 2.7 km altitude and dissipating rapidly. At 0120 UTC on 29 October they reported minor discrete ash emissions observed on visible satellite imagery moving NW at 2.7 km altitude and dissipating rapidly. At 0720 UTC they reported minor discrete ash emissions observed on visible satellite imagery at 0710 UTC moving NW at 2.7 km altitude and dissipating rapidly. At 1320 UTC they reported minor discrete ash emissions observed on satellite imagery moving WNW at 2.7 km altitude and dissipating rapidly. At 1920 UTC they reported minor discrete ash emissions observed on satellite imagery moving W at 2.7 km altitude and dissipating rapidly. At 0120 UTC on 30 October they reported minor discrete ash emissions identifiable on satellite imagery moving W at 2.7 km altitude and dissipating rapidly. At 0720 UTC they reported minor discrete ash emissions were last observed on satellite imagery at 0420 UTC moving W at 2.7 km altitude and dissipating rapidly and expected to continue. At 1320 UTC they reported minor discrete ash emissions were last observed on satellite imagery at 0420 UTC moving W at 2.7 km altitude and dissipating rapidly and were ongoing. At 1920 UTC they reported minor discrete ash emissions were last observed on satellite imagery at 1610 UTC moving SW at 2.7 km altitude and dissipating rapidly and were ongoing. At 0120 UTC on 31 October they reported minor discrete ash emissions were observed on satellite imagery at 0010 UTC moving W at 2.7 km altitude and dissipating rapidly. At 0720 UTC they reported that weak ash emissions were identifiable W of the volcano at 2.7 km altitude at 0600 UTC and dissipating rapidly. At 1320 UTC they reported that weak ash emissions were identifiable W of the volcano at 2.7 km altitude at 0600 UTC and dissipating rapidly. Ash was not identifiable in satellite imagery due to meteoric clouds. At 1920 UTC they reported that ash was not identifiable overnight in satellite imagery due to darkess. A hotspot remained on satellite imagery. Recent emissions were shortlived and dissipated rapidly. At 0120 UTC on 1 November they reported that ash was not discernible on clear satellite imagery. Steam or smoke emissions continued with a hot spot evident. Regular seismic activity was detected.
2019 Nov 3 2019 Nov 12 Ash Plume Based on HIMAWARI-8 information, at 2300 UTC on 2 November the Darwin VAAC reported weak intermittent ash emissions clearly identifiable on satellite imagery moving NW at 2.7 km altitude and quickly dissipating. At 0500 UTC on 3 November they reported weak intermittent ash emissions discernible on satellite imagery moving WNW at 2.7 km altitude and quickly dissipating. At 0844 UTC they reported weak intermittent ash emissions discernible on satellite imagery moving N at 3.4 km altitude and quickly dissipating. Plume height raised based on model guidance. At 1150 UTC they reported weak intermittent ash emissions recently occurring moving NW at 3.4 km altitude and quickly dissipating. Ash was not observed but a hotspot was present. At 1900 UTC they reported weak intermittent ash emissions last observed at 1400 UTC moving NW at 3.4 km altitude and quickly dissipating. Ash was not observed but a hotspot was present during the previous hour. At 0100 UTC on 4 November they reported weak intermittent ash emissions last observed at 0040 UTC moving NW at 2.7 km altitude and quickly dissipating. At 0700 UTC they reported weak intermittent ash emissions last observed at 0230 UTC moving NW at 3.4 km altitude and quickly dissipating. At 1300 UTC they reported weak intermittent ash emissions observed at 1220 UTC moving WSW at 3.4 km altitude and quickly dissipating. At 1900 UTC they reported weak intermittent ash emissions last observed at 1800 UTC moving W at 3.4 km altitude and quickly dissipating. Regular hotspots were observed at the summit. At 0100 UTC on 5 November they reported weak intermittent ash emissions moving WNW at 3.0 km altitude and quickly dissipating. Regular hotspots were observed at the summit. At 0700 UTC they reported weak intermittent ash emissions moving W at 3.0 km altitude and quickly dissipating. Regular hotspots were observed at the summit. At 1300 UTC they reported weak intermittent ash emissions moving W at 3.0 km altitude and quickly dissipating. At 1900 UTC they reported weak intermittent ash emissions moving W at 3.0 km altitude and quickly dissipating. Regular hotspots were observed at the summit. At 0108 UTC on 6 November they reported weak intermittent ash emissions observed in satellite imagery moving W at 3.0 km altitude and quickly dissipating. At 0715 UTC they reported weak intermittent ash emissions observed in satellite imagery moving NW at 3.0 km altitude and quickly dissipating. At 1330 UTC they reported weak intermittent ash emissions observed in satellite imagery moving W at 3.0 km altitude and quickly dissipating. At 1930 UTC they reported weak intermittent ash emissions moving W at 3.0 km altitude and quickly dissipating. Hotspot at the summit remains ongoing. At 0210 UTC on 7 November they reported weak intermittent ash emissions observed in satellite imagery at 0150 UTC moving NW at 3.0 km altitude and quickly dissipating. Hotspot at the summit remains ongoing. At 0740 UTC they reported weak intermittent ash emissions observed in satellite imagery at 0710 UTC moving NW at 3.0 km altitude and quickly dissipating. Hotspot at the summit remains ongoing. At 1320 UTC they reported weak intermittent ash emissions observed in satellite imagery at 1230 UTC moving W at 3.0 km altitude and quickly dissipating. Hotspot at the summit remains ongoing. At 1920 UTC they reported weak intermittent ash emissions observed in satellite imagery at 1750 UTC moving W at 3.0 km altitude and quickly dissipating. Hotspot at the summit remains ongoing. At 0120 UTC on 8 November they reported weak intermittent ash emissions observed in satellite imagery moving W at 3.0 km altitude and quickly dissipating. At 0720 UTC they reported weak intermittent ash emissions observed in satellite imagery moving W at 3.0 km altitude and quickly dissipating. At 1320 UTC they reported weak intermittent ash emissions last observed in satellite imagery at 0830 UTC moving W at 3.0 km altitude and quickly dissipating. Ash was not identifiable in satellite imagery due to meteoric clouds. At 1920 UTC they reported weak intermittent ash emissions last observed in satellite imagery at 0830 UTC moving W at 3.0 km altitude and quickly dissipating. Ash was not identifiable in satellite imagery due to meteoric clouds. A hotspot remained evident. At 0120 UTC on 9 November they reported weak intermittent ash emissions last observed in satellite imagery at 0830 UTC on 8 November moving W at 3.0 km altitude and quickly dissipating. Ash was not identifiable in satellite imagery due to meteoric clouds. At 0720 UTC they reported weak intermittent ash emissions observed in recent satellite imagery moving W at 3.0 km altitude and quickly dissipating. At 1320 UTC they reported weak intermittent ash emissions last observed in satellite imagery at 0730 UTC moving W at 3.0 km altitude and quickly dissipating. Ash was not identifiable in satellite imagery due to meteoric clouds. At 1920 UTC they reported minor intermittent ash emissions last observed in satellite imagery at 0730 UTC moving W at 3.0 km altitude and quickly dissipating. Ash was not identifiable in satellite imagery due to meteoric clouds. At 0120 UTC on 10 November they reported minor intermittent ash emissions observed in satellite imagery moving W at 3.0 km altitude and quickly dissipating. At 0720 UTC they reported minor discrete intermittent ash emissions observed in satellite imagery moving W at 3.0 km altitude and quickly dissipating. At 1320 UTC they reported minor discrete intermittent ash emissions observed in satellite imagery moving W at 3.0 km altitude and quickly dissipating. At 1920 UTC they reported minor discrete intermittent ash emissions observed in satellite imagery moving W at 3.0 km altitude and quickly dissipating. At 0120 UTC on 11 November they reported minor discrete intermittent ash emissions observed in satellite imagery moving SW at 3.0 km altitude and quickly dissipating. At 0720 UTC they reported minor discrete intermittent ash emissions unidentifiable in satellite imagery due to meteoric clouds. At 1320 UTC they reported minor intermittent ash emissions last observed in RGB satellite imagery moving W at 3.0 km altitude and quickly dissipating between 0910 and 1100 UTC. At 1920 UTC they reported minor discrete intermittent ash emissions last observed in satellite imagery moving W at 3.0 km altitude and quickly dissipating at 1000 UTC. At 0120 UTC on 12 November they reported that ash was last observed moving W at 2240 UTC on 11 November. Minor smoke emissions were possibly ongoing.
2019 Nov 5 2019 Nov 7 Thermal Anomaly Four MODVOLC thermal alerts were issued.
2019 Nov 14 2019 Nov 28 Ash Plume Based on HIMAWARI-8 information, at 0015 UTC the Darwin VAAC reported minor intermittent ash emissions last observed in visible and RGB satellite imagery at 0000 UTC moving W at 2.4 km altitude. At 0615 UTC they reported minor intermittent ash emissions ongoing with last discrete emission observed in visible and RGB satellite imagery at 0500 UTC moving WNW at 2.4 km altitude. At 1215 UTC they reported minor intermittent ash emissions identifiable on satellite imagery moving NW at 2.4 km altitude and quickly dissipating. At 1815 UTC they reported minor intermittent ash emissions identifiable on satellite imagery moving WNW at 2.4 km altitude and quickly dissipating. At 0015 UTC on 15 November they reported ongoing intermittent ash emissions identifiable on satellite imagery moving NW at 2.4 km altitude and dissipating rapidly. At 0615 UTC they reported ongoing intermittent ash emissions identifiable on satellite imagery moving NW at 2.4 km altitude and dissipating rapidly. At 1215 UTC they reported ongoing intermittent ash emissions identifiable on satellite imagery last observed at 0840 UTC moving NW at 2.4 km altitude and dissipating rapidly. Periodic large hotspots were observed. At 1730 UTC they reported ongoing intermittent ash emissions identifiable on RGB satellite imagery moving W at 2.4 km altitude and dissipating rapidly. At 2330 UTC they reported ongoing intermittent ash emissions identifiable on visible satellite imagery moving W at 2.4 km altitude and dissipating rapidly. At 0530 UTC on 16 November they reported ongoing intermittent ash emissions identifiable on visible satellite imagery moving W at 2.4 km altitude and dissipating rapidly. At 1130 UTC they reported ongoing intermittent ash emissions observed on RGB satellite imagery moving W at 2.4 km altitude and dissipating rapidly. At 1730 UTC they reported ongoing intermittent ash emissions observed on RGB satellite imagery moving W at 2.4 km altitude and dissipating rapidly. At 2350 UTC they reported ongoing intermittent ash emissions observed on RGB satellite imagery moving W at 2.4 km altitude and dissipating rapidly. At 0555 UTC on 17 November they reported ongoing intermittent ash emissions observed on RGB satellite imagery moving W at 2.4 km altitude and dissipating rapidly. At 1155 UTC they reported ongoing intermittent ash emissions last observed on satellite imagery at 0930UTC moving W at 2.4 km altitude and dissipating rapidly. At 1755 UTC they reported ongoing intermittent ash emissions observed on RGB satellite imagery moving W at 2.4 km altitude. At 2355 UTC they reported ongoing intermittent ash emissions clearly identifiable on the latest satellite imagery moving W at 2.4 km altitude. At 0555 UTC on 18 November they reported ongoing intermittent ash emissions discernible on satellite imagery moving W at 2.4 km altitude. At 1155 UTC they reported ongoing intermittent ash emissions discernible on satellite imagery at 1130 UTC moving W at 2.4 km altitude. At 1755 UTC they reported ongoing intermittent ash emissions last observed on satellite imagery at 1610 UTC moving W at 2.4 km altitude. Ash was not identifiable in satellite imagery due to meteoric clouds but a hot spot remained. At 2355 UTC they reported ongoing intermittent ash emissions discernible on satellite imagery moving SW at 2.4 km altitude. A hot spot remained visible. At 0555 UTC they reported ongoing intermittent ash emissions discernible on satellite imagery moving W at 2.4 km altitude. A hot spot remained visible. At 1155 UTC they reported ongoing intermittent ash emissions last observed on satellite imagery at 0510 UTC moving W at 2.4 km altitude. Ash was not identifiable in satellite imagery due to meteoric clouds, however a hot spot remained visible. At 1755 UTC they reported ongoing intermittent ash emissions last observed on satellite imagery at 0510 UTC moving W at 2.4 km altitude. Ash was not identifiable in satellite imagery due to meteoric clouds, however a hot spot remained visible. At 2355 UTC they reported ongoing intermittent ash emissions observed on satellite imagery at 2350 UTC moving W at 2.4 km altitude. At 0555 UTC on 20 November they reported ongoing intermittent ash emissions were last observed at 2350 UTC on 19 November moving W at 2.4 km altitude. At 1155 UTC they reported frequent ongoing minor discrete ash emissions observed on RGB satellite imagery moving W at 2.4 km altitude. At 1755 UTC they reported intermittent minor discrete ash emissions were last observed at 1610 UTC in RGB satellite imagery moving W at 2.4 km altitude. At 2355 UTC they reported intermittent minor discrete ash emissions observed on visible satellite imagery at 2330 UTC moving SW at 2.4 km altitude. At 0555 UTC on 21 November they reported intermittent minor discrete ash emissions observed on visible satellite imagery at 0340 UTC moving SW at 2.4 km altitude. At 1155 UTC they reported intermittent minor discrete ash emissions observed on RGB satellite imagery moving W at 2.4 km altitude. The last eruption occurred at 0940 UTC. At 1755 UTC they reported intermittent minor discrete ash emissions observed on RGB satellite imagery moving SW at 2.4 km altitude. The last eruption occurred at 1710 UTC. At 2355 UTC they reported intermittent minor discrete ash emissions discernible on satellite imagery moving W at 2.4 km altitude and dissipating quickly. At 0555 UTC on 22 November they reported intermittent minor discrete ash emissions regularly discernible on satellite imagery, last observed at 0420 UTC, moving W at 2.4 km altitude and dissipating quickly. At 1155 UTC they reported intermittent minor discrete ash emissions regularly discernible on satellite imagery moving W at 2.4 km altitude and dissipating quickly. At 1755 UTC they reported intermittent minor discrete ash emissions regularly discernible on satellite imagery moving WSW at 2.4 km altitude and dissipating quickly. At 2355 UTC they reported intermittent minor discrete ash emissions discernible on satellite imagery moving WSW at 2.4 km altitude and dissipating quickly. At 0555 UTC on 23 November they reported intermittent minor discrete ash emissions regularly discernible on satellite imagery moving W at 2.4 km altitude and dissipating quickly. At 1155 UTC they reported intermittent ongoing minor discrete ash emissions last identifiable on satellite imagery at 0900 UTC moving W at 2.4 km altitude and dissipating quickly. At 1730 UTC they reported intermittent ongoing minor discrete ash emissions discernible on RGB satellite imagery moving W at 2.4 km altitude and quickly dissipating. At 2330 UTC they reported intermittent minor discrete ash emissions discernible on visible satellite imagery moving W at 2.4 km altitude and dissipating quickly. At 0530 UTC on 24 November they reported intermittent minor discrete ash emissions discernible on visible satellite imagery moving W at 2.4 km altitude and dissipating quickly. At 1130 UTC they reported intermittent minor discrete ash emissions were last observed on satellite imagery at 0850 UTC moving W at 2.4 km altitude. At 1730 UTC they reported intermittent minor discrete ash emissions were last observed on satellite imagery at 1300 UTC moving WNW at 2.4 km altitude. At 2330 UTC they reported continuous discrete ash emissions were observed on satellite imagery at 2300 UTC moving WNW at 2.4 km altitude. At 0530 UTC on 25 November they reported continuous discrete ash emissions were observed on satellite imagery at 0500 UTC moving NW at 2.4 km altitude. At 1130 UTC they reported frequent discrete ash emissions were observed on RGB satellite imagery moving NW at 2.4 km altitude. At 1730 UTC they reported frequent discrete ash emissions were observed on RGB satellite imagery moving NW at 2.4 km altitude. At 2330 UTC they reported frequent discrete ash emissions were observed on satellite imagery moving NW at 2.4 km altitude. At 0530 UTC on 26 November they reported frequent discrete ash emissions were observed on satellite imagery moving NW at 2.4 km altitude. At 1130 UTC they reported ash observed in RGB satellite imagery at 1100 UTC moving NW at 2.4 km altitude. At 1730 UTC they reported ash observed in RGB satellite imagery at 1700 UTC moving SW at 2.4 km altitude. At 2330 UTC they reported ash observed in satellite imagery at 2310 UTC moving SW at 2.4 km altitude. At 0530 UTC on 27 November they reported ash observed in satellite imagery at 0510 UTC moving SW at 2.4 km altitude. At 1130 UTC they reported continuous discrete eruptions observed in RGB satellite imagery at 1110 UTC moving SW at 2.4 km altitude. At 1730 UTC they reported intermittent eruptions last observed in satellite imagery at 1200 UTC moving W at 2.4 km altitude. Ash was not identifiable on satellite imagery due to meteoric clouds. A hotspot remained evident. At 2330 UTC they reported intermittent eruptions last observed in satellite imagery at 1200 UTC moving W at 2.4 km altitude. Ash was not identifiable on satellite imagery due to meteoric clouds. A hotspot remained evident. At 0530 UTC on 28 November they reported intermittent eruptions last observed in satellite imagery at 1200 UTC on 27 November moving W at 2.4 km altitude. Ash was not identifiable on satellite imagery due to meteoric clouds. Minor emissions were still expected. At 1130 UTC they reported intermittent discrete last observed in satellite imagery at 1200 UTC on 27 November moving NW at 2.4 km altitude. Ash was not identifiable on satellite imagery due to meteoric clouds. A hotspot remained evident. Minor emissions were still expected. At 1730 UTC they reported that ash was last observed in satellite imagery moving SW at 2.4 km altitude at 1200 UTC on 27 November. Ash was not identifiable on satellite imagery due to meteoric clouds. A hotspot remained evident.
2019 Nov 18    - - - - Thermal Anomaly A MODVOLC thermal alert was issued.
2019 Nov 23 2019 Nov 25 Thermal Anomaly Two MODVOLC thermal alerts were issued.
2019 Nov 29    - - - - Ash Plume Based on HIMAWARI-8 information, at 2315 UTC on 28 November the Darwin VAAC reported regular discrete ash emissions clearly identifiable in satellite imagery moving NW at 3.4 km altitude. At 0445 UTC on 29 November they reported that ash was last observed in satellite imagery moving NW at 3.4 km altitude at 0230 UTC and had dissipated.
2019 Nov 29 2019 Dec 4 Ash Plume Based on HIMAWARI-8 information, at 0900 UTC the Darwin VAAC reported minor intermittent ash eruptions clearly identifiable on satellite imagery moving W at 3.4 km altitude, observed at 0840 UTC. At 1500 UTC they reported minor intermittent ash eruptions partially identifiable on satellite imagery moving SW at 2.4 km altitude, observed at 1450 UTC. At 2100 UTC they reported minor intermittent ash eruptions partially identifiable on RGB satellite imagery moving WSW at 2.4 km altitude, observed at 2040 UTC. At 0300 UTC on 30 November they reported minor intermittent ash eruptions clearly identifiable on satellite imagery moving WSW at 2.4 km altitude, observed at 0240 UTC. At 0900 UTC they reported minor intermittent ash eruptions clearly identifiable on satellite imagery moving W at 2.4 km altitude, observed at 0750 UTC. At 1500 UTC they reported that regular discrete ash emissions were last observed in satellite imagery at 0830 UTC moving W at 2.4 km altitude. Ash was not identifiable on overnight satellite imagery, however discrete emissions were expected to be ongoing. At 2100 UTC they reported that regular discrete ash emissions were last observed in satellite imagery at 0830 UTC moving W at 2.4 km altitude. Ash was not identifiable on overnight satellite imagery, however discrete emissions were expected to be ongoing. At 0300 UTC on 1 December they reported regular discrete ash emissions were discernible on satellite imagery moving NW at 2.4 km altitude. At 0810 UTC they reported regular discrete ash emissions were discernible on visible satellite imagery moving NW at 2.4 km altitude. At 1410 UTC they reported regular minor ash emissions were expected to be ongoing moving NW at 2.4 km altitude. At 1910 UTC they reported regular minor ash emissions last observed at 0930 UTC were expected to be ongoing moving NW at 2.4 km altitude. At 0150 UTC on 2 December they reported regular discrete ash emissions were discernible on visible and RGB satellite imagery moving NW at 2.4 km altitude. At 0730 UTC they reported regular minor discrete ash emissions were last discernible on visible and RGB satellite imagery at 0420 UTC moving NW at 2.4 km altitude. At 1330 UTC they reported minor discrete ash emissions were discernible on RGB satellite imagery moving W at 2.4 km altitude. At 1930 UTC they reported regular minor discrete ash emissions were last discernible on satellite imagery at 1300 UTC moving W at 2.4 km altitude and expected to be ongoing. At 0130 UTC on 3 December they reported regular minor discrete ash emissions were discernible on visible and RGB satellite imagery moving W at 2.4 km altitude. At 0730 UTC they reported regular minor discrete ash emissions were last discernible on satellite imagery at 0400 UTC moving NW at 2.4 km altitude and expected to be ongoing. At 1330 UTC they reported regular minor discrete ash emissions were last discernible on satellite imagery at 0910 UTC moving W at 2.4 km altitude and expected to be ongoing. At 1930 UTC they reported regular minor discrete ash emissions were last observed on satellite imagery at 0910 UTC moving W at 2.4 km altitude and expected to be ongoing. At 0130 UTC on 4 December they reported regular minor discrete ash emissions were last observed on satellite imagery at 0910 UTC on 3 December moving W at 2.4 km altitude and expected to be ongoing. Ash was not identified in satellite imagery due to meteoric clouds. At 0658 UTC they reported regular minor discrete ash emissions were last observed on satellite imagery at 0910 UTC on 3 December moving W at 2.4 km altitude and expected to be ongoing. Ash was not identified in satellite imagery due to meteoric clouds. At 1258 UTC they reported regular minor discrete ash emissions were last observed on satellite imagery at 2330 UTC on 3 December moving W at 2.4 km altitude and expected to be ongoing. Ash was not identified in satellite imagery due to meteoric clouds. At 1858 UTC they reported regular minor discrete ash emissions were last observed on satellite imagery at 2330 UTC on 3 December moving W at 2.4 km altitude and expected to be ongoing. Ash was not identified in satellite imagery due to meteoric clouds. At 0027 UTC on 5 December they reported that ash emissions were last observed on satellite imagery at 2330 UTC on 3 December moving W at 2.4 km altitude. Ash had not been seen for the previous 24 hours
2019 Nov 30 2019 Dec 2 Thermal Anomaly Two MODVOLC thermal alerts were issued.
2019 Dec 7 2019 Dec 13 Ash Plume Based on HIMAWARI-8 information, at 2300 UTC on 6 December the Darwin VAAC reported frequent discrete eruptions observed in visible satellite imagery with ash moving W at 2.4 km altitude. At 0400 UTC on 7 December they reported frequent discrete eruptions observed in visible satellite imagery with ash moving W at 2.4 km altitude. At 1000 UTC they reported frequent discrete eruptions last observed in visible satellite imagery at 0450 UTC with ash moving W at 2.4 km altitude. Ash was not identified in satellite imagery due to meteoric clouds. Minor discrete eruptions of ash were expected to be ongoing. At 1600 UTC they reported frequent discrete eruptions last observed in visible satellite imagery at 0450 UTC with ash moving W at 2.4 km altitude. Ash was not identified in satellite imagery due to meteoric clouds. Minor discrete eruptions of ash were expected to be ongoing. At 2200 UTC they reported frequent discrete eruptions last observed in visible satellite imagery at 0450 UTC with ash moving W at 2.4 km altitude. Ash was not identified in satellite imagery due to meteoric clouds. Minor discrete eruptions of ash were expected to be ongoing. At 0400 UTC on 8 December they reported frequent discrete eruptions of ash were clearly discernible in satellite imagery moving NW at 2.4 km altitude. Minor discrete eruptions of ash were expected to be ongoing. At 1000 UTC they reported discrete ash emissions clearly discernible in satellite imagery moving NW at 2.4 km altitude. Minor discrete eruptions of ash were expected to be ongoing. At 1600 UTC they reported ash was not identified in satellite imagery due to darkness. Minor discrete eruptions of ash were expected to be ongoing. At 2200 UTC they reported discrete eruptions of ash were last observed in RGB satellite imagery at 2120 UTC with ash moving W at 2.4 km altitude. At 0400 UTC on 9 December they reported minor discrete ash emissions were last discernible in RGB satellite imagery at 0300 UTC with ash moving WNW at 2.4 km altitude. At 1000 UTC they reported discrete ash emissions discernible in satellite imagery moving NW at 2.4 km altitude. At 1600 UTC they reported discrete ash emissions discernible in satellite imagery moving NW at 2.4 km altitude. A hotspot was visible over the summit. Minor emissions continued. At 2200 UTC they reported regular discrete ash emissions discernible in RGB satellite imagery at 2140 UTC moving WNW at 2.4 km altitude. At 0400 UTC on 10 December they reported that a weak ash signal moving WNW at 2.4 km altitude was last observed at 0230 UTC on RGB satellite imagery. At 1000 UTC they reported that a weak ash signal moving WNW at 2.4 km altitude was last observed at 0900 UTC on visible satellite imagery. At 1600 UTC they reported that ash was not discernible on satellite imagery overnight and was last observed at 0900 UTC on visible satellite imagery moving WNW at 2.4 km altitude. Regular discrete eruptions of ash were assumed to be continuing. At 2200 UTC they reported that ash was not discernible on satellite imagery due to darkness and was last observed at 0900 UTC on visible satellite imagery moving WNW at 2.4 km altitude. Regular discrete eruptions of ash moving W at 2.4 km altitude were assumed to be continuing. At 0400 UTC on 11 December they reported minor intermittent discrete ash emissions observed in satellite imagery at 0330 UTC moving W at 2.4 km altitude and rapidly dissipating. At 1000 UTC they reported minor intermittent discrete ash emissions observed in satellite imagery at 0830 UTC moving NW at 2.4 km altitude and rapidly dissipating. At 1600 UTC they reported minor intermittent discrete ash emissions observed in RGB satellite imagery moving W at 2.4 km altitude and rapidly dissipating. At 2200 UTC they reported that minor intermittent discrete ash emissions were not discernible on satellite imagery overnight and were last observed in satellite imagery at 1540 UTC moving W at 2.4 km altitude. At 0400 UTC on 12 December they reported minor intermittent discrete ash emissions observed in visible satellite imagery at 0330 UTC moving W at 2.4 km altitude. At 1000 UTC they reported minor intermittent discrete ash emissions observed in visible satellite imagery at 0940 UTC moving NW at 2.4 km altitude. At 1600 UTC they reported that minor intermittent discrete ash emissions were not discernible on satellite imagery due to meteoric clouds and were last observed in satellite imagery at 0850 UTC moving W at 2.4 km altitude. At 2200 UTC they reported that minor intermittent discrete ash emissions were not discernible on satellite imagery due to meteoric clouds and were last observed in satellite imagery at 0850 UTC moving W at 2.4 km altitude. At 0400 UTC on 13 December they reported that minor intermittent discrete ash emissions were not discernible on satellite imagery due to meteoric clouds and were last observed in satellite imagery at 0150 UTC moving W at 2.4 km altitude. At 1000 UTC they reported that minor intermittent discrete ash emissions were not discernible on satellite imagery due to meteoric clouds and were last observed in satellite imagery at 0150 UTC moving W at 2.4 km altitude. At 1600 UTC they reported that minor intermittent discrete ash emissions were not discernible on satellite imagery due to meteoric clouds and were last observed in satellite imagery at 0150 UTC moving W at 2.4 km altitude. At 2202 UTC they reported that minor intermittent discrete ash emissions were not discernible on satellite imagery due to meteoric clouds and were last observed in satellite imagery at 0150 UTC moving W at 2.4 km altitude. At 0340 UTC on 14 December they reported that ash had not been discerned in satellite imagery for the previous 24 hours.
2019 Dec 17 2019 Dec 18 Ash Plume Based on HIMAWARI-8 information, at 2338 UTC on 16 December the Darwin VAAC reported that discrete ash emissions moving W at 2.4 km altitude were observed in Visible and RGB satellite imagery at 2310 UTC. At 0537 UTC on 17 December they reported that discrete ash emissions moving W at 2.4 km altitude were observed in Visible and RGB satellite imagery at 0350 UTC. At 1125 UTC they reported that ash was not observed in satellite imagery due to meteoric clouds. Ash was last observed in satellite imagery moving W at 2.4 km altitude at 0900 UTC. Minor intermittent eruptions were expected. At 1720 UTC they reported that minor intermittent eruptions were observed in RBG imagery moving W at 2.4 km altitude. At 2320 UTC they reported that minor intermittent eruptions were observed in satellite imagery moving W at 2.4 km altitude and rapidly dissipating. At 0520 UTC on 18 December they reported that minor intermittent eruptions of ash were observed in satellite imagery moving W at 2.4 km altitude and quickly dissipating. At 1120 UTC they reported that minor intermittent emissions of ash were observed in satellite imagery moving W at 2.4 km altitude and quickly dissipating. At 1720 UTC they reported that minor intermittent emissions of ash were observed in satellite imagery moving W at 2.4 km altitude and quickly dissipating. At 2320 UTC they reported that minor intermittent emissions of ash were last observed in satellite imagery at 2250 UTC on 17 December moving W at 2.4 km altitude and quickly dissipating. Ash was not identifiable in satellite imagery due to meteoric clouds and had not been identifiable for the previous 24 hours.
2019 Dec 18    - - - - Thermal Anomaly Two MODVOLC thermal alerts were issued.
2019 Dec 25    - - - - Ash Plume Based on HIMAWARI-8 information, at 2255 UTC on 24 December the Darwin VAAC reported discrete ash emissions observed on visible satellite imagery moving WSW at 2.4 km altitude. At 0455 UTC on 25 December they reported minor intermittent ash emissions observed on visible satellite imagery moving WSW at 2.4 km altitude. At 1055 UTC they reported that ash was not identifiable in satellite imagery due to meteoric clouds however ash emissions were still expected. At 1655 UTC they reported that ash was not identifiable in satellite imagery due to meteoric clouds however ash emissions were still expected. At 2255 UTC they reported that ash emissions were no longer identifiable in satellite imagery and the volcano was clear of meteoric clouds.
2019 Dec 25    - - - - Thermal Anomaly A MODVOLC thermal alert was issued.
2019 Dec 27    - - - - Ash Plume Based on HIMAWARI-8 information, at 0040 UTC the Darwin VAAC reported discrete ash emissions observed on satellite imagery moving SW at 3.0 km altitude and dissipating rapidly. At 0637 UTC they reported that ash was not identifiable in satellite imagery due to meteoric clouds. At 1237 UTC they reported that ash was not identifiable in satellite imagery due to meteoric clouds. At 1837 UTC they reported that ash was not identifiable in satellite imagery due to meteoric clouds. At 1941 UTC they reported that ash was not identifiable in satellite imagery due to meteoric clouds. At 0024 UTC on 28 December they reported that ash could no longer be identified in satellite imagery.

2014 May 30 - 2015 Nov 5 Confirmed Eruption (Explosive / Effusive) VEI: 4

Episode 1 | Eruption (Explosive / Effusive) Summit crater and east flank
2014 May 30 - 2014 Dec 27 Evidence from Observations: Reported

List of 31 Events for Episode 1 at Summit crater and east flank

Start Date End Date Event Type Event Remarks
2014 May 30    - - - - Seismicity (volcanic) Seismicity increased, with tremor starting at 0500 and becoming continuous at 1348.
2014 May 30    - - - - Explosion CVGHM reported an eruption at 1555 that generated an ash plume that rose more than 3 km above the summit and drifted W, causing ashfall over the sea.
2014 May 30    - - - - Ash Plume CVGHM reported an eruption at 1555 that generated an ash plume that rose more than 3 km above the summit and drifted W, causing ashfall over the sea. Based on satellite images, pilot observations, and the Indonesian Meteorological Office, the Darwin VAAC reported that the ash plume rose to an altitude of 15.2 km and drifted 440 km E and 750 km SE. Pilots in the area reported seeing the cloud rising to 19.8 km, spreading over a 40 km area.
2014 May 30    - - - - Pyroclastic flow Photographs of the eruption showed several pyroclastic flows coming down the volcano summit to the S and E.
2014 May 30    - - - - Ashfall An eruption at 1555 generated an ash plume that rose 3 km and drifted W, causing ashfall over the sea.
2014 May 30    - - - - Evacuations Civil authorities evacuated 135 people to the mainland.
2014 May 30    - - - - VEI (Explosivity Index) VEI 4
2014 May 31    - - - - Explosion BNPB reported that two larger explosions occurred at 1330 and 2242.
2014 May 31    - - - - Ash Plume According to the VAAC, ash plumes from the explosions rose to altitudes of 13.7-15.2 km and drifted 280 km NW and other various directions. Later in the day the ash plumes became detached.
2014 May 31    - - - - Ashfall Ashfall affected many areas in the Bima Regency on the mainland, including Wera.
2014 May 31    - - - - Evacuations Ashfall prompted the evacuation of 7,328 people from four villages within a radius of 8 km from Sangeang Api.
2014 May 31    - - - - VEI (Explosivity Index) VEI 3
2014 Jun 1 2014 Jun 3 Ash Plume The VAAC noted that ash plumes rose to altitudes of 3-4.3 km and drifted up to 45 km W and SW.
2014 Jun 1 2014 Jun 17 Ash Plume During clear conditions, white-and-gray plumes (100-1,500 m above the summit) were visible.
2014 Jun 1 2014 Jun 17 Incandescence During clear conditions, incandescence was visible at the summit.
2014 Jun 4 2014 Jun 7 Ash Plume Based on analyses of satellite imagery and wind data, the Darwin VAAC reported that ash plumes rose to an altitude of 3 km and drifted 45-110 km W and NW.
2014 Jun 7 2014 Dec 27 Lava flow Multiple nearly-daily MODVOLC thermal alerts on the E flank for several months suggested an active lava flow.
2014 Jun 7 2014 Jun 20 Thermal Anomaly Multiple near-daily MODVOLC thermal alerts were issued.
2014 Jun 14    - - - - Ash Plume Based on analyses of satellite imagery and wind data, the Darwin VAAC reported that an ash plume rose to an altitude of 2.1 km and drifted 55 km NW.
2014 Jun 25 2014 Jul 9 Thermal Anomaly Multiple near-daily MODVOLC thermal alerts were issued.
2014 Jul 13 2014 Aug 2 Thermal Anomaly Multiple near-daily MODVOLC thermal alerts were issued.
2014 Aug 5 2014 Aug 16 Thermal Anomaly Multiple near-daily MODVOLC thermal alerts were issued.
2014 Aug 19 2014 Oct 12 Thermal Anomaly Multiple near-daily MODVOLC thermal alerts were issued.
2014 Oct 15 2014 Oct 28 Thermal Anomaly Multiple near-daily MODVOLC thermal alerts were issued.
2014 Oct 31 2014 Nov 6 Thermal Anomaly Eleven MODVOLC thermal alerts were issued.
2014 Nov 9 2014 Nov 13 Thermal Anomaly Six MODVOLC thermal alerts were issued.
2014 Nov 16 2014 Nov 20 Thermal Anomaly Six MODVOLC thermal alerts were issued.
2014 Nov 23    - - - - Thermal Anomaly A MODVOLC thermal alert was issued.
2014 Dec 2    - - - - Thermal Anomaly A MODVOLC thermal alert was issued.
2014 Dec 13 2014 Dec 15 Thermal Anomaly Eight MODVOLC thermal alerts were issued.
2014 Dec 27    - - - - Thermal Anomaly A MODVOLC thermal alert was issued.
Episode 2 | Eruption (Explosive / Effusive) Summit crater and east flank
2015 Mar 17 - 2015 Nov 5 Evidence from Observations: Satellite (infrared)

List of 26 Events for Episode 2 at Summit crater and east flank

Start Date End Date Event Type Event Remarks
2015 Mar 17    - - - - Thermal Anomaly Two MODVOLC thermal alerts were issued.
2015 Mar 24 2015 Mar 26 Thermal Anomaly Three MODVOLC thermal alerts were issued.
2015 Apr 29    - - - - Thermal Anomaly Two MODVOLC thermal alerts were issued.
2015 May 6 2015 May 8 Thermal Anomaly Four MODVOLC thermal alerts were issued.
2015 May 27 2015 May 31 Thermal Anomaly Six MODVOLC thermal alerts were issued.
2015 Jun 14 2015 Jun 16 Thermal Anomaly Three MODVOLC thermal alerts were issued.
2015 Jun 19 2015 Jun 25 Thermal Anomaly Five MODVOLC thermal alerts were issued.
2015 Jun 30    - - - - Thermal Anomaly One MODVOLC thermal alert was issued.
2015 Jul 7    - - - - Ash Plume Based on analyses of satellite imagery and wind data, the Darwin VAAC reported that an ash plume rose to an altitude of 2.7 km and drifted over 35 km E.
2015 Jul 7    - - - - Thermal Anomaly Three MODVOLC thermal alerts were issued.
2015 Jul 7    - - - - VEI (Explosivity Index) VEI 1
2015 Jul 8    - - - - Ash Plume Based on analyses of satellite imagery and wind data, the Darwin VAAC reported that an ash plume rose to an altitude of 2.7 km and drifted over 35 km SE.
2015 Jul 16    - - - - Thermal Anomaly Three MODVOLC thermal alerts were issued.
2015 Jul 23    - - - - Thermal Anomaly One MODVOLC thermal alert was issued.
2015 Aug 22 2015 Aug 28 Thermal Anomaly Nine MODVOLC thermal alerts were issued.
2015 Aug 31 2015 Sep 4 Thermal Anomaly Four MODVOLC thermal alerts were issued.
2015 Sep 9    - - - - Thermal Anomaly One MODVOLC thermal alert was issued.
2015 Sep 20 2015 Sep 22 Thermal Anomaly Two MODVOLC thermal alerts were issued.
2015 Sep 25 2015 Sep 27 Thermal Anomaly Three MODVOLC thermal alerts were issued.
2015 Oct 1
(on or after)
2015 Nov 1
(on or before)
Ash Plume White-to-gray plumes rose as high as 350 m.
2015 Oct 1
(on or after)
2015 Nov 1
(on or before)
Lava dome PVMBG reported that crater incandescence possibly indicated lava-dome growth or lava-flow advancement.
2015 Oct 1
(on or after)
2015 Nov 1
(on or before)
Incandescence PVMBG reported that crater incandescence possibly indicated lava-dome growth or lava-flow advancement.
2015 Oct 4    - - - - Thermal Anomaly Two MODVOLC thermal alerts were issued.
2015 Oct 11 2015 Oct 13 Thermal Anomaly Three MODVOLC thermal alerts were issued.
2015 Oct 23
(on or after)
   - - - - Audible Sounds PVMBG reported that beginning on 23 October, occasional weak thumping noises were reported.
2015 Nov 5    - - - - Thermal Anomaly A MODVOLC thermal alert was issued.

[ 2009 May 1 - 2009 Jun 3 ] Uncertain Eruption

Episode 1 | Eruption (Explosive / Effusive)
2009 May 1 - 2009 Jun 3 Evidence from Unknown

List of 1 Events for Episode 1

Start Date End Date Event Type Event Remarks
   - - - -    - - - - Earthquakes (undefined)

1997 Jul 2 ± 182 days - 1999 Jul 2 ± 182 days Confirmed Eruption (Explosive / Effusive) VEI: 2 (?)

Episode 1 | Eruption (Explosive / Effusive)
1997 Jul 2 ± 182 days - 1999 Jul 2 ± 182 days Evidence from Observations: Reported

List of 4 Events for Episode 1

Start Date End Date Event Type Event Remarks
   - - - -    - - - - Explosion
   - - - -    - - - - Lava flow
   - - - -    - - - - Lava dome
1997    - - - - VEI (Explosivity Index)

1985 Jul 30 - 1988 Feb 16 ± 15 days Confirmed Eruption (Explosive / Effusive) VEI: 3

Episode 1 | Eruption (Explosive / Effusive) Doro Api
1985 Jul 30 - 1988 Feb 16 ± 15 days Evidence from Observations: Reported

List of 10 Events for Episode 1 at Doro Api

Start Date End Date Event Type Event Remarks
   - - - -    - - - - Explosion moderate
   - - - -    - - - - Pyroclastic flow moderate
   - - - -    - - - - Lava flow moderate
   - - - -    - - - - Ash
   - - - -    - - - - Blocks
   - - - -    - - - - Earthquakes (undefined) Before.
   - - - -    - - - - Lahar or Mudflow
   - - - -    - - - - Evacuations
1985 Jul 30    - - - - VEI (Explosivity Index)
1987 Jan    - - - - VEI (Explosivity Index)

1966 Feb 28 - 1966 Nov 16 ± 15 days Confirmed Eruption (Explosive / Effusive) VEI: 2

Episode 1 | Eruption (Explosive / Effusive)
1966 Feb 28 - 1966 Nov 16 ± 15 days Evidence from Observations: Reported

List of 2 Events for Episode 1

Start Date End Date Event Type Event Remarks
   - - - -    - - - - Explosion
1966 Feb 28    - - - - VEI (Explosivity Index)

1964 Jan 29 - 1965 Dec 1 ± 30 days Confirmed Eruption (Explosive / Effusive) VEI: 2

Episode 1 | Eruption (Explosive / Effusive) Doro Api
1964 Jan 29 - 1965 Dec 1 ± 30 days Evidence from Observations: Reported

List of 10 Events for Episode 1 at Doro Api

Start Date End Date Event Type Event Remarks
   - - - -    - - - - Explosion
   - - - -    - - - - Lava flow
   - - - -    - - - - Lava dome
   - - - -    - - - - Cinder Cone
   - - - -    - - - - Ash
   - - - -    - - - - Lapilli
   - - - -    - - - - Bombs
   - - - -    - - - - Earthquakes (undefined) Before.
   - - - -    - - - - Evacuations
1964 Jan 29    - - - - VEI (Explosivity Index)

1958 Jul 2 ± 182 days Confirmed Eruption (Explosive / Effusive) VEI: 1 (?)

Episode 1 | Eruption (Explosive / Effusive)
1958 Jul 2 ± 182 days - Unknown Evidence from Observations: Reported

List of 5 Events for Episode 1

Start Date End Date Event Type Event Remarks
   - - - -    - - - - Explosion Uncertain
   - - - -    - - - - Ash
   - - - -    - - - - Incandescence Event was "Glow"
   - - - -    - - - - Audible Sounds
1958    - - - - VEI (Explosivity Index)

1957 Jul 2 ± 182 days Confirmed Eruption (Explosive / Effusive) VEI: 1

Episode 1 | Eruption (Explosive / Effusive)
1957 Jul 2 ± 182 days - Unknown Evidence from Observations: Reported

List of 3 Events for Episode 1

Start Date End Date Event Type Event Remarks
   - - - -    - - - - Phreatic activity weak or small
   - - - -    - - - - Audible Sounds weak or small
1957    - - - - VEI (Explosivity Index)

1956 Dec 16 ± 15 days Confirmed Eruption (Explosive / Effusive) VEI: 1

Episode 1 | Eruption (Explosive / Effusive)
1956 Dec 16 ± 15 days - Unknown Evidence from Observations: Reported

List of 3 Events for Episode 1

Start Date End Date Event Type Event Remarks
   - - - -    - - - - Phreatic activity weak or small
   - - - -    - - - - Audible Sounds weak or small
1956 Dec    - - - - VEI (Explosivity Index)

1955 Jul 2 ± 182 days Confirmed Eruption (Explosive / Effusive) VEI: 1

Episode 1 | Eruption (Explosive / Effusive)
1955 Jul 2 ± 182 days - Unknown Evidence from Observations: Reported

List of 3 Events for Episode 1

Start Date End Date Event Type Event Remarks
   - - - -    - - - - Phreatic activity weak or small
   - - - -    - - - - Audible Sounds weak or small
1955    - - - - VEI (Explosivity Index)

1954 Nov 4 Confirmed Eruption (Explosive / Effusive) VEI: 2

Episode 1 | Eruption (Explosive / Effusive)
1954 Nov 4 - Unknown Evidence from Observations: Reported

List of 2 Events for Episode 1

Start Date End Date Event Type Event Remarks
   - - - -    - - - - Explosion
1954 Nov 4    - - - - VEI (Explosivity Index)

1954 Apr 26 Confirmed Eruption (Explosive / Effusive) VEI: 2

Episode 1 | Eruption (Explosive / Effusive)
1954 Apr 26 - Unknown Evidence from Observations: Reported

List of 2 Events for Episode 1

Start Date End Date Event Type Event Remarks
   - - - -    - - - - Explosion
1954 Apr 26    - - - - VEI (Explosivity Index)

1953 Mar 19 - 1953 May 15 (on or after) Confirmed Eruption (Explosive / Effusive) VEI: 3

Episode 1 | Eruption (Explosive / Effusive) Doro Api
1953 Mar 19 - 1953 May 15 (on or after) Evidence from Observations: Reported

List of 10 Events for Episode 1 at Doro Api

Start Date End Date Event Type Event Remarks
   - - - -    - - - - Seismicity (volcanic)
   - - - -    - - - - Explosion
   - - - -    - - - - Lava flow
   - - - -    - - - - Ash
   - - - -    - - - - Lapilli
   - - - -    - - - - Bombs
   - - - -    - - - - Audible Sounds
   - - - -    - - - - Lahar or Mudflow
   - - - -    - - - - Evacuations
1953 Mar 19    - - - - VEI (Explosivity Index)

1927 Confirmed Eruption (Explosive / Effusive) VEI: 2

Episode 1 | Eruption (Explosive / Effusive)
1927 - Unknown Evidence from Observations: Reported

List of 2 Events for Episode 1

Start Date End Date Event Type Event Remarks
   - - - -    - - - - Explosion
1927    - - - - VEI (Explosivity Index)

1912 Apr Confirmed Eruption (Explosive / Effusive) VEI: 2

Episode 1 | Eruption (Explosive / Effusive)
1912 Apr - Unknown Evidence from Observations: Reported

List of 2 Events for Episode 1

Start Date End Date Event Type Event Remarks
   - - - -    - - - - Explosion
1912 Apr    - - - - VEI (Explosivity Index)

1911 Feb 13 - 1911 Mar 2 Confirmed Eruption (Explosive / Effusive) VEI: 2

Episode 1 | Eruption (Explosive / Effusive) Doro Api
1911 Feb 13 - 1911 Mar 2 Evidence from Observations: Reported

List of 5 Events for Episode 1 at Doro Api

Start Date End Date Event Type Event Remarks
   - - - -    - - - - Explosion
   - - - -    - - - - Lava flow
   - - - -    - - - - Ash
   - - - -    - - - - Earthquakes (undefined) Before.
1911 Feb 13    - - - - VEI (Explosivity Index)

1860 Sep 11 - 1860 Oct Confirmed Eruption (Explosive / Effusive) VEI: 2

Episode 1 | Eruption (Explosive / Effusive)
1860 Sep 11 - 1860 Oct Evidence from Observations: Reported

List of 2 Events for Episode 1

Start Date End Date Event Type Event Remarks
   - - - -    - - - - Explosion
1860 Sep 11    - - - - VEI (Explosivity Index)

1821 Mar 23 Confirmed Eruption (Explosive / Effusive) VEI: 2

Episode 1 | Eruption (Explosive / Effusive)
1821 Mar 23 - Unknown Evidence from Observations: Reported

List of 2 Events for Episode 1

Start Date End Date Event Type Event Remarks
   - - - -    - - - - Explosion
1821 Mar 23    - - - - VEI (Explosivity Index)

1715 Confirmed Eruption (Explosive / Effusive) VEI: 2

Episode 1 | Eruption (Explosive / Effusive)
1715 - Unknown Evidence from Observations: Reported

List of 2 Events for Episode 1

Start Date End Date Event Type Event Remarks
   - - - -    - - - - Explosion
1715    - - - - VEI (Explosivity Index)

[ 1512 ] Uncertain Eruption

Episode 1 | Eruption (Explosive / Effusive)
1512 - Unknown Evidence from Observations: Reported

List of 2 Events for Episode 1

Start Date End Date Event Type Event Remarks
   - - - -    - - - - Explosion
1512    - - - - VEI (Explosivity Index)

This compilation of synonyms and subsidiary features may not be comprehensive. Features are organized into four major categories: Cones, Craters, Domes, and Thermal Features. Synonyms of features appear indented below the primary name. In some cases additional feature type, elevation, or location details are provided.

Photo Gallery

Thumbnail Photo (see caption)Cumulus clouds drift from the summit of the 13-km-wide island of Sangeang Api off the NE coast of Sumbawa. Sangeang Api volcano contains two large cones, Doro Api and Doro Montoi. Intermittent eruptions have been recorded since 1512.

Copyrighted photo by Katia and Maurice Krafft, 1971.
Thumbnail Photo (see caption)Sangeang Api is a small volcanic island off the NE coast of Sumbawa Island. Two large cones, Doro Api in the center and Doro Mantai on the right, were constructed within and on the south rim of a largely obscured caldera. Intermittent eruptions have been recorded since 1512 and it has been frequently active in the 20th century.

Photo by Tom Casadevall, 1985 (U.S. Geological Survey).
Thumbnail Photo (see caption)An ash plume rises above the Doro Api peak of Sangeang Api volcano on 25 August 1985. The eruption, which began on 30 July and lasted until February 1988, included explosive activity, pyroclastic flows, and a lava flow that traveled 4-5 km down the W flank.

Photo by Tom Casadevall, 1985 (U.S. Geological Survey).
Thumbnail Photo (see caption)A lava flow descends the W flank of Doro Api at Sangeang Api volcano on 4 December 1985. The eruption began on 30 July and pyroclastic flows forced the evacuation of the island's 1,242 inhabitants. The lava flow eventually traveled 4-5 km before stopping in June 1986. Explosive activity continued until February 1988.

Photo by Tom Casadevall, 1985 (U.S. Geological Survey).
Thumbnail Photo (see caption)Islanders prepare to evacuate on 25 August 1985 as Sangeang Api volcano erupts in the background. The eruption began on 30 July and produced pyroclastic flows that eventually forced the evacuation of the island's entire 1,242 inhabitants.

Photo by Tom Casadevall, 1985 (U.S. Geological Survey).
Thumbnail Photo (see caption)An eruption of Doro Api at Sangeang Api volcano is observed from the village of Doro Mewanga on 18 September 1964. The eruption began on 29 January 1964 and lasted until the end of 1965. During the eruption strong explosions took place from the summit crater and a lava flow traveled down to 750 m elevation.

Photo courtesy of Volcanological Survey of Indonesia, 1964.
Thumbnail Photo (see caption)A plume rises above Doro Api, one of the two large post-caldera cones of Sangeang Api, in 1985. Doro Mantai appears at the right in this view from Sori Buntu on the S flank. An eruption that included both explosive activity and the effusion of lava flows down the W flank began in July 1985 and lasted until February 1988.

Photo by Samud W., 1990 (Volcanological Survey of Indonesia).
Smithsonian Sample Collections Database

There are no samples for Sangeang Api in the Smithsonian's NMNH Department of Mineral Sciences Rock and Ore collection.

External Sites