Manam is a 10-km-wide island that consists of two active summit craters: the Main summit crater and the South summit crater and is located 13 km off the northern coast of mainland Papua New Guinea. Frequent mild-to-moderate eruptions have been recorded since 1616. The current eruption period began during June 2014 and has more recently been characterized by intermittent ash plumes and thermal activity (BGVN 47:11). This report updates activity that occurred from November 2022 through May 2023 based on information from the Darwin Volcanic Ash Advisory Center (VAAC) and various satellite data.

Ash plumes were reported during November and December 2022 by the Darwin VAAC. On 7 November an ash plume rose to 2.1 km altitude and drifted NE based on satellite images and weather models. On 14 November an ash plume rose to 2.1 km altitude and drifted W based on RVO webcam images. On 20 November ash plumes rose to 1.8 km altitude and drifted NW. On 26 December an ash plume rose to 3 km altitude and drifted S and SSE.

Intermittent sulfur dioxide plumes were detected using the TROPOMI instrument on the Sentinel-5P satellite, some of which exceeded at least two Dobson Units (DU) and drifted in different directions (figure 93). Occasional low-to-moderate power thermal anomalies were recorded by the MIROVA (Middle InfraRed Observation of Volcanic Activity) system; less than five anomalies were recorded each month during November 2022 through May 2023 (figure 94). Two thermal hotspots were detected by the MODVOLC thermal alerts system on 10 December 2022. On clear weather days, thermal activity was also captured in infrared satellite imagery in both the Main and South summit craters, accompanied by gas-and-steam emissions (figure 95).

Figure 93. Distinct sulfur dioxide plumes were captured, rising from Manam based on data from the TROPOMI instrument on the Sentinel-5P satellite on 16 November 2022 (top left), 6 December 2022 (top right), 14 January 2023 (bottom left), and 23 March 2023 (bottom right). Plumes generally drifted in different directions. Courtesy of the NASA Global Sulfur Dioxide Monitoring Page.

Figure 94. Occasional low-to-moderate power thermal anomalies were detected at Manam during November 2022 through May 2023, as shown in this MIROVA graph (Log Radiative Power). Only three anomalies were detected during late November, one in early December, two during January 2023, one in late March, four during April, and one during late May. Courtesy of MIROVA.

Figure 95. Infrared (bands B12, B11, B4) satellite images show a consistent thermal anomaly (bright yellow-orange) in both the Main (the northern crater) and South summit craters on 10 November 2022 (top left), 15 December 2022 (top right), 3 February 2023 (bottom left), and 24 April 2023 (bottom right). Gas-and-steam emissions occasionally accompanied the thermal activity. Courtesy of Copernicus Browser.

Geologic Background. The 10-km-wide island of Manam, lying 13 km off the northern coast of mainland Papua New Guinea, is one of the country's most active volcanoes. Four large radial valleys extend from the unvegetated summit of the conical basaltic-andesitic stratovolcano to its lower flanks. These valleys channel lava flows and pyroclastic avalanches that have sometimes reached the coast. Five small satellitic centers are located near the island's shoreline on the northern, southern, and western sides. Two summit craters are present; both are active, although most observed eruptions have originated from the southern crater, concentrating eruptive products during much of the past century into the SE valley. Frequent eruptions, typically of mild-to-moderate scale, have been recorded since 1616. Occasional larger eruptions have produced pyroclastic flows and lava flows that reached flat-lying coastal areas and entered the sea, sometimes impacting populated areas.

Information Contacts: Rabaul Volcano Observatory (RVO), Geohazards Management Division, Department of Mineral Policy and Geohazards Management (DMPGM), PO Box 3386, Kokopo, East New Britain Province, Papua New Guinea; 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/); NASA Global Sulfur Dioxide Monitoring Page, Atmospheric Chemistry and Dynamics Laboratory, NASA Goddard Space Flight Center (NASA/GSFC), 8800 Greenbelt Road, Goddard, Maryland, USA (URL: https://so2.gsfc.nasa.gov/); Copernicus Browser, Copernicus Data Space Ecosystem, European Space Agency (URL: https://dataspace.copernicus.eu/browser/).

Krakatau is located in the Sunda Strait between Java and Sumatra, Indonesia. Caldera collapse during the catastrophic 1883 eruption destroyed Danan and Perbuwatan cones and left only a remnant of Rakata. The post-collapse cone of Anak Krakatau (Child of Krakatau) was constructed within the 1883 caldera at a point between the former Danan and Perbuwatan cones; it has been the site of frequent eruptions since 1927. The current eruption period began in May 2021 and has recently consisted of explosions, ash plumes, and thermal activity (BGVN 47:11). This report covers activity during November 2022 through April 2023 based on information provided by the Indonesian Center for Volcanology and Geological Hazard Mitigation, referred to as Pusat Vulkanologi dan Mitigasi Bencana Geologi (PVMBG), MAGMA Indonesia, the Darwin Volcanic Ash Advisory Center (VAAC), and several sources of satellite data.

Activity was relatively low during November and December 2022. Daily white gas-and-steam plumes rose 25-100 m above the summit and drifted in different directions. Gray ash plumes rose 200 m above the summit and drifted NE at 1047 and at 2343 on 11 November. On 14 November at 0933 ash plumes rose 300 m above the summit and drifted E. An ash plume was reported at 0935 on 15 December that rose 100 m above the summit and drifted NE. An eruptive event at 1031 later that day generated an ash plume that rose 700 m above the summit and drifted NE. A gray ash plume at 1910 rose 100 m above the summit and drifted E. Incandescent material was ejected above the vent based on an image taken at 1936.

During January 2023 daily white gas-and-steam plumes rose 25-300 m above the summit and drifted in multiple directions. Gray-to-brown ash plumes were reported at 1638 on 3 January, at 1410 and 1509 on 4 January, and at 0013 on 5 January that rose 100-750 m above the summit and drifted NE and E; the gray-to-black ash plume at 1509 on 4 January rose as high as 3 km above the summit and drifted E. Gray ash plumes were recorded at 1754, 2241, and 2325 on 11 January and at 0046 on 12 January and rose 200-300 m above the summit and drifted NE. Toward the end of January, PVMBG reported that activity had intensified; Strombolian activity was visible in webcam images taken at 0041, 0043, and 0450 on 23 January. Multiple gray ash plumes throughout the day rose 200-500 m above the summit and drifted E and SE (figure 135). Webcam images showed progressively intensifying Strombolian activity at 1919, 1958, and 2113 on 24 January; a gray ash plume at 1957 rose 300 m above the summit and drifted E (figure 135). Eruptive events at 0231 and 2256 on 25 January and at 0003 on 26 January ejected incandescent material from the vent, based on webcam images. Gray ash plumes observed during 26-27 January rose 300-500 m above the summit and drifted NE, E, and SE.

Figure 135. Webcam images of a strong, gray ash plume (left) and Strombolian activity (right) captured at Krakatau at 0802 on 23 January 2023 (left) and at 2116 on 24 January 2023 (right). Courtesy of PVMBG and MAGMA Indonesia.

Low levels of activity were reported during February and March. Daily white gas-and-steam plumes rose 25-300 m above the summit and drifted in different directions. The Darwin VAAC reported that continuous ash emissions rose to 1.5-1.8 km altitude and drifted W and NW during 1240-1300 on 10 March, based on satellite images, weather models, and PVMBG webcams. White-and-gray ash plumes rose 500 m and 300 m above the summit and drifted SW at 1446 and 1846 on 18 March, respectively. An eruptive event was recorded at 2143, though it was not visible due to darkness. Multiple ash plumes were reported during 27-29 March that rose as high as 2.5 km above the summit and drifted NE, W, and SW (figure 136). Webcam images captured incandescent ejecta above the vent at 0415 and around the summit area at 2003 on 28 March and at 0047 above the vent on 29 March.

Figure 136. Webcam image of a strong ash plume rising above Krakatau at 1522 on 28 March 2023. Courtesy of PVMBG and MAGMA Indonesia.

Daily white gas-and-steam plumes rose 25-300 m above the summit and drifted in multiple directions during April and May. White-and-gray and black plumes rose 50-300 m above the summit on 2 and 9 April. On 11 May at 1241 a gray ash plume rose 1-3 km above the summit and drifted SW. On 12 May at 0920 a gray ash plume rose 2.5 km above the summit and drifted SW and at 2320 an ash plume rose 1.5 km above the summit and drifted SW. An accompanying webcam image showed incandescent ejecta. On 13 May at 0710 a gray ash plume rose 2 km above the summit and drifted SW (figure 137).

Figure 137. Webcam image of an ash plume rising 2 km above the summit of Krakatau at 0715 on 13 May 2023. Courtesy of PVMBG and MAGMA Indonesia.

The MIROVA (Middle InfraRed Observation of Volcanic Activity) graph of MODIS thermal anomaly data showed intermittent low-to-moderate power thermal anomalies during November 2022 through April 2023 (figure 138). Some of this thermal activity was also visible in infrared satellite imagery at the crater, accompanied by gas-and-steam and ash plumes that drifted in different directions (figure 139).

Figure 138. Intermittent low-to-moderate power thermal anomalies were detected at Krakatau during November 2022 through April 2023, based on this MIROVA graph (Log Radiative Power). Courtesy of MIROVA.

Figure 139. A thermal anomaly (bright yellow-orange) was visible at Krakatau in infrared (bands B12, B11, B4) satellite images on clear weather days during November 2022 through May 2023. Occasional gas-and-steam and ash plumes accompanied the thermal activity, which drifted in different directions. Images were captured on 25 November 2022 (top left), 15 December 2022 (top right), 27 January 2023 (bottom left), and 12 May 2023 (bottom right). Courtesy of Copernicus Browser.

Geologic Background. The renowned Krakatau (frequently mis-named as Krakatoa) volcano lies in the Sunda Strait between Java and Sumatra. Collapse of an older edifice, perhaps in 416 or 535 CE, formed a 7-km-wide caldera. Remnants of that volcano are preserved in Verlaten and Lang Islands; subsequently the Rakata, Danan, and Perbuwatan cones were formed, coalescing to create the pre-1883 Krakatau Island. Caldera collapse during the catastrophic 1883 eruption destroyed Danan and Perbuwatan, and left only a remnant of Rakata. This eruption caused more than 36,000 fatalities, most as a result of tsunamis that swept the adjacent coastlines of Sumatra and Java. Pyroclastic surges traveled 40 km across the Sunda Strait and reached the Sumatra coast. After a quiescence of less than a half century, the post-collapse cone of Anak Krakatau (Child of Krakatau) was constructed within the 1883 caldera at a point between the former Danan and Perbuwatan cones. Anak Krakatau has been the site of frequent eruptions since 1927.

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.esdm.go.id/v1); 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/); Copernicus Browser, Copernicus Data Space Ecosystem, European Space Agency (URL: https://dataspace.copernicus.eu/browser/).

Stromboli, located in Italy, has exhibited nearly constant lava fountains for the past 2,000 years; recorded eruptions date back to 350 BCE. Eruptive activity occurs at the summit from multiple vents, which include a north crater area (N area) and a central-southern crater (CS area) on a terrace known as the ‘terrazza craterica’ at the head of the Sciara del Fuoco, a large scarp that runs from the summit down the NW side of the volcano-island. Activity typically consists of Strombolian explosions, incandescent ejecta, lava flows, and pyroclastic flows. Thermal and visual monitoring cameras are located on the nearby Pizzo Sopra La Fossa, above the terrazza craterica, and at multiple flank locations. The current eruption period has been ongoing since 1934 and recent activity has consisted of frequent Strombolian explosions and lava flows (BGVN 48:02). This report updates activity during January through April 2023 primarily characterized by Strombolian explosions and lava flows based on reports from Italy's Istituto Nazionale di Geofisica e Vulcanologia (INGV) and various satellite data.

Frequent explosive activity continued throughout the reporting period, generally in the low-to-medium range, based on the number of hourly explosions in the summit crater (figure 253, table 16). Intermittent thermal activity was recorded by the MIROVA (Middle InfraRed Observation of Volcanic Activity) analysis of MODIS satellite data (figure 254). According to data collected by the MODVOLC thermal algorithm, a total of 9 thermal alerts were detected: one on 2 January 2023, one on 1 February, five on 24 March, and two on 26 March. The stronger pulses of thermal activity likely reflected lava flow events. Infrared satellite imagery captured relatively strong thermal hotspots at the two active summit craters on clear weather days, showing an especially strong event on 8 March (figure 255).

Figure 253. Explosive activity persisted at Stromboli during January through April 2023, with low to medium numbers of daily explosions at the summit crater. The average number of daily explosions (y-axis) during January through April (x-axis) are broken out by area and as a total, with red for the N area, blue for the CS area, and black for the combined total. The data are smoothed as daily (thin lines) and weekly (thick lines) averages. The black squares along the top represent days with no observations due to poor visibility (Visib. Scarsa). The right axis indicates the qualitative activity levels from low (basso) to highest (altissimo) with the green highlighted band indicating the most common level. Courtesy of INGV (Report 17/2023, Stromboli, Bollettino Settimanale, 18/04/2023 - 24/04/2023).

Table 16. Summary of type, frequency, and intensity of explosive activity at Stromboli by month during January-April 2023; information from webcam observations. Courtesy of INGV weekly reports.

Figure 254. Intermittent thermal activity at Stromboli was detected during January through April 2023 and varied in strength, as shown in this MIROVA graph (Log Radiative Power). A pulse of activity was captured during late March. Courtesy of MIROVA.

Figure 255. Infrared (bands B12, B11, B4) satellite images showing persistent thermal anomalies at both summit crater on 1 February 2023 (top left), 23 March 2023 (top right), 8 March 2023 (bottom left), and 27 April 2023. A particularly strong thermal anomaly was visible on 8 March. Courtesy of Copernicus Browser.

Activity during January-February 2023. Strombolian explosions were reported in the N crater area, as well as lava effusion. Explosive activity in the N crater area ejected coarse material (bombs and lapilli). Intense spattering was observed in both the N1 and N2 craters. In the CS crater area, explosions generally ejected fine material (ash), sometimes to heights greater than 250 m. The intensity of the explosions was characterized as low-to-medium in the N crater and medium-to-high in the CS crater. After intense spattering activity from the N crater area, a lava overflow began at 2136 on 2 January that flowed part way down the Sciara del Fuoco, possibly moving down the drainage that formed in October, out of view from webcams. The flow remained active for a couple of hours before stopping and beginning to cool. A second lava flow was reported at 0224 on 4 January that similarly remained active for a few hours before stopping and cooling. Intense spattering was observed on 11 and 13 January from the N1 crater. After intense spattering activity at the N2 crater at 1052 on 17 January another lava flow started to flow into the upper part of the Sciara del Fuoco (figure 256), dividing into two: one that traveled in the direction of the drainage formed in October, and the other one moving parallel to the point of emission. By the afternoon, the rate of the flow began to decrease, and at 1900 it started to cool. A lava flow was reported at 1519 on 24 January following intense spattering in the N2 area, which began to flow into the upper part of the Sciara del Fuoco. By the morning of 25 January, the lava flow had begun to cool. During 27 January the frequency of eruption in the CS crater area increased to 6-7 events/hour compared to the typical 1-7 events/hour; the following two days showed a decrease in frequency to less than 1 event/hour. Starting at 1007 on 30 January a high-energy explosive sequence was produced by vents in the CS crater area. The sequence began with an initial energetic pulse that lasted 45 seconds, ejecting predominantly coarse products 300 m above the crater that fell in an ESE direction. Subsequent and less intense explosions ejected material 100 m above the crater. The total duration of this event lasted approximately two minutes. During 31 January through 6, 13, and 24 February spattering activity was particularly intense for short periods in the N2 crater.

Figure 256. Webcam images of the lava flow development at Stromboli during 17 January 2023 taken by the SCT infrared camera. The lava flow appears light yellow-green in the infrared images. Courtesy of INGV (Report 04/2023, Stromboli, Bollettino Settimanale, 16/01/2023 - 22/01/2023).

An explosive sequence was reported on 16 February that was characterized by a major explosion in the CS crater area (figure 257). The sequence began at 1817 near the S2 crater that ejected material radially. A few seconds later, lava fountains were observed in the central part of the crater. Three explosions of medium intensity (material was ejected less than 150 m high) were recorded at the S2 crater. The first part of this sequence lasted approximately one minute, according to INGV, and material rose 300 m above the crater and then was deposited along the Sciara del Fuoco. The second phase began at 1818 at the S1 crater; it lasted seven seconds and material was ejected 150 m above the crater. Another event 20 seconds later lasted 12 seconds, also ejecting material 150 m above the crater. The sequence ended with at least three explosions of mostly fine material from the S1 crater. The total duration of this sequence was about two minutes.

Figure 257. Webcam images of the explosive sequence at Stromboli on 16 February 2023 taken by the SCT and SCV infrared and visible cameras. The lava appears light yellow-green in the infrared images. Courtesy of INGV (Report 08/2023, Stromboli, Bollettino Settimanale, 13/02/2023 - 19/02/2023).

Short, intense spattering activity was noted above the N1 crater on 27 and 28 February. A lava overflow was first reported at 0657 from the N2 crater on 27 February that flowed into the October 2022 drainage. By 1900 the flow had stopped. A second lava overflow also in the N crater area occurred at 2149, which overlapped the first flow and then stopped by 0150 on 28 February. Material detached from both the lava overflows rolled down the Sciara del Fuoco, some of which was visible in webcam images.

Activity during March-April 2023. Strombolian activity continued with spattering activity and lava overflows in the N crater area during March. Explosive activity at the N crater area varied from low (less than 80 m high) to medium (less than 150 m high) and ejected coarse material, such as bombs and lapilli. Spattering was observed above the N1 crater, while explosive activity at the CS crater area varied from medium to high (greater than 150 m high) and ejected coarse material. Intense spattering activity was observed for short periods on 6 March above the N1 crater. At approximately 0610 a lava overflow was reported around the N2 crater on 8 March, which then flowed into the October 2022 drainage. By 1700 the flow started to cool. A second overflow began at 1712 on 9 March and overlapped the previous flow. It had stopped by 2100. Material from both flows was deposited along the Sciara del Fuoco, though much of the activity was not visible in webcam images. On 11 March a lava overflow was observed at 0215 that overlapped the two previous flows in the October 2022 drainage. By late afternoon on 12 March, it had stopped.

During a field excursion on 16 March, scientists noted that a vent in the central crater area was degassing. Another vent showed occasional Strombolian activity that emitted ash and lapilli. During 1200-1430 low-to-medium intense activity was reported; the N1 crater emitted ash emissions and the N2 crater emitted both ash and coarse material. Some explosions also occurred in the CS crater area that ejected coarse material. The C crater in the CS crater area occasionally showed gas jetting and low intensity explosions on 17 and 22 March; no activity was observed at the S1 crater. Intense, longer periods of spattering were reported in the N1 crater on 19, 24, and 25 March. Around 2242 on 23 March a lava overflow began from the N1 crater that, after about an hour, began moving down the October 2022 drainage and flow along the Sciara del Fuoco (figure 258). Between 0200 and 0400 on 26 March the flow rate increased, which generated avalanches of material from collapses at the advancing flow front. By early afternoon, the flow began to cool. On 25 March at 1548 an explosive sequence began from one of the vents at S2 in the CS crater area (figure 258). Fine ash mixed with coarse material was ejected 300 m above the crater rim and drifted SSE. Some modest explosions around Vent C were detected at 1549 on 25 March, which included an explosion at 1551 that ejected coarse material. The entire explosive sequence lasted approximately three minutes.

Figure 258. Webcam images of the lava overflow in the N1 crater area of Stromboli on 23 March 2023 taken by the SCT infrared camera. The lava appears light yellow-green in the infrared images. The start of the explosive sequence was also captured on 25 March 2023 accompanied by an eruption plume (e) captured by the SCT and SPT infrared webcams. Courtesy of INGV (Report 13/2023, Stromboli, Bollettino Settimanale, 20/03/2023 - 26/03/2023).

During April explosions persisted in both the N and CS crater areas. Fine material was ejected less than 80 m above the N crater rim until 6 April, followed by ejection of coarser material. Fine material was also ejected less than 80 m above the CS crater rim. The C and S2 crater did not show significant eruptive activity. On 7 April an explosive sequence was detected in the CS crater area at 1203 (figure 259). The first explosion lasted approximately 18 seconds and ejected material 400 m above the crater rim, depositing pyroclastic material in the upper part of the Sciara del Fuoco. At 1204 a second, less intense explosion lasted approximately four seconds and deposited pyroclastic products outside the crater area and near Pizzo Sopra La Fossa. A third explosion at 1205 was mainly composed of ash that rose about 150 m above the crater and lasted roughly 20 seconds. A fourth explosion occurred at 1205 about 28 seconds after the third explosion and ejected a mixture of coarse and fine material about 200 m above the crater; the explosion lasted roughly seven seconds. Overall, the entire explosive sequence lasted about two minutes and 20 seconds. After the explosive sequence on 7 April, explosions in both the N and CS crater areas ejected material as high as 150 m above the crater.

Figure 259. Webcam images of the explosive sequence at Stromboli during 1203-1205 (local time) on 7 April 2023 taken by the SCT infrared camera. Strong eruption plumes are visible, accompanied by deposits on the nearby flanks. Courtesy of INGV (Report 15/2023, Stromboli, Bollettino Settimanale, 03/04/2023 - 09/04/2023).

On 21 April research scientists from INGV made field observations in the summit area of Stromboli, and some lapilli samples were collected. In the N crater area near the N1 crater, a small cone was observed with at least two active vents, one of which was characterized by Strombolian explosions. The other vent produced explosions that ejected ash and chunks of cooled lava. At the N2 crater at least one vent was active and frequently emitted ash. In the CS crater area, a small cone contained 2-3 degassing vents and a smaller, possible fissure area also showed signs of degassing close to the Pizzo Sopra La Fossa. In the S part of the crater, three vents were active: a small hornito was characterized by modest and rare explosions, a vent that intermittently produced weak Strombolian explosions, and a vent at the end of the terrace that produced frequent ash emissions. Near the S1 crater there was a hornito that generally emitted weak gas-and-steam emissions, sometimes associated with “gas rings”. On 22 April another field inspection was carried out that reported two large sliding surfaces on the Sciara del Fuoco that showed where blocks frequently descended toward the sea. A thermal anomaly was detected at 0150 on 29 April.

Geologic Background. Spectacular incandescent nighttime explosions at Stromboli have long attracted visitors to the "Lighthouse of the Mediterranean" in the NE Aeolian Islands. This volcano has lent its name to the frequent mild explosive activity that has characterized its eruptions throughout much of historical time. The small island is the emergent summit of a volcano that grew in two main eruptive cycles, the last of which formed the western portion of the island. The Neostromboli eruptive period took place between about 13,000 and 5,000 years ago. The active summit vents are located at the head of the Sciara del Fuoco, a prominent scarp that formed about 5,000 years ago due to a series of slope failures which extends to below sea level. The modern volcano has been constructed within this scarp, which funnels pyroclastic ejecta and lava flows to the NW. Essentially continuous mild Strombolian explosions, sometimes accompanied by lava flows, have been recorded for more than a millennium.

Information Contacts: Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione di Catania, Piazza Roma 2, 95123 Catania, Italy, (URL: http://www.ct.ingv.it/en/); 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/); Copernicus Browser, Copernicus Data Space Ecosystem, European Space Agency (URL: https://dataspace.copernicus.eu/browser/).

Nishinoshima is a small island located about 1,000 km S of Tokyo in the Ogasawara Arc in Japan. The island is the summit of a massive submarine volcano that has prominent peaks to the S, W, and NE. Eruptions date back to 1973; the most recent eruption period began in October 2022 and was characterized by ash plumes and fumarolic activity (BGVN 47:12). This report describes ash plumes and fumarolic activity during November 2022 through April 2023 based on monthly reports from the Japan Meteorological Agency (JMA) monthly reports and satellite data.

The most recent eruptive activity prior to the reporting internal occurred on 12 October 2022, when an ash plume rose 3.5 km above the crater rim. An aerial observation conducted by the Japan Coast Guard (JCG) on 25 November reported that white fumaroles rose approximately 200 m above the central crater of a pyroclastic cone (figure 119), and multiple plumes were observed on the ESE flank of the cone. Discolored water ranging from reddish-brown to brown and yellowish-green were visible around the perimeter of the island (figure 119). No significant activity was reported in December.

Figure 119. Aerial photo of gas-and-steam plumes rising 200 m above Nishinoshima on 25 November 2022. Reddish brown to brown and yellowish-green discolored water was visible around the perimeter of the island. Courtesy of JCG via JMA (monthly reports of activity at Nishinoshima, November 2022).

During an overflight conducted by JCG on 25 January 2023 intermittent activity and small, blackish-gray plumes rose 900 m above the central part of the crater were observed (figure 120). The fumarolic zone of the E flank and base of the cone had expanded and emissions had intensified. Dark brown discolored water was visible around the perimeter of the island.

Figure 120. Aerial photo of a black-gray ash plume rising approximately 900 m above the crater rim of Nishinoshima on 25 January 2023. White fumaroles were visible on the E slope of the pyroclastic cone. Dense brown to brown discolored water was observed surrounding the island. Photo has been color corrected. Courtesy of JCG via JMA (monthly reports of activity at Nishinoshima, January, 2023).

No significant activity was reported during February through March. Ash plumes at 1050 and 1420 on 11 April rose 1.9 km above the crater rim and drifted NW and N. These were the first ash plumes observed since 12 October 2022. On 14 April JCG carried out an overflight and reported that no further eruptive activity was visible, although white gas-and-steam plumes were visible from the central crater and rose 900 m high (figure 121). Brownish and yellow-green discolored water surrounded the island.

Figure 121. Aerial photo of white gas-and-steam plumes rising 900 m above Nishinoshima on 14 April 2023. Brown and yellow-green discolored water is visible around the perimeter of the island. Photo has been color corrected. Courtesy of JCG via JMA (monthly reports of activity at Nishinoshima, April, 2023).

Intermittent low-to-moderate power thermal anomalies were recorded in the MIROVA graph (Middle InfraRed Observation of Volcanic Activity) during November 2022 through April 2023 (figure 123). A cluster of six to eight anomalies were detected during November while a smaller number were detected during the following months: two to three during December, one during mid-January 2023, one during February, five during March, and two during April. Thermal activity was also reflected in infrared satellite data at the summit crater, accompanied by occasional gas-and-steam plumes (figure 124).

Figure 123. Intermittent low-to-moderate thermal anomalies were detected at Nishinoshima during November 2022 through April 2023, according to this MIROVA graph (Log Radiative Power). A cluster of anomalies occurred throughout November, while fewer anomalies were detected during the following months. Courtesy of MIROVA.

Figure 124. Infrared (bands B12, B11, B4) satellite images show a small thermal anomaly at the summit crater of Nishinoshima on 9 January 2023 (left) and 8 February 2023 (right). Gas-and-steam plumes accompanied this activity and extended S and SE, respectively. Courtesy of Copernicus Browser.

Geologic Background. The small island of Nishinoshima was enlarged when several new islands coalesced during an eruption in 1973-74. Multiple eruptions that began in 2013 completely covered the previous exposed surface and continued to enlarge the island. The island is the summit of a massive submarine volcano that has prominent peaks to the S, W, and NE. The summit of the southern cone rises to within 214 m of the ocean surface 9 km SSE.

Information Contacts: Japan Meteorological Agency (JMA), 1-3-4 Otemachi, Chiyoda-ku, Tokyo 100-8122, Japan (URL: http://www.jma.go.jp/jma/indexe.html); 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/); Copernicus Browser, Copernicus Data Space Ecosystem, European Space Agency (URL: https://dataspace.copernicus.eu/browser/).

Karangetang (also known as Api Siau), at the northern end of the island of Siau, Indonesia, contains five summit craters along a N-S line. More than 40 eruptions have been recorded since 1675; recent eruptions have included frequent explosive activity, sometimes accompanied by pyroclastic flows and lahars. Lava dome growth has occurred in the summit craters and collapses of lava flow fronts have produced pyroclastic flows. The two active summit craters are Kawah Dua (the N crater) and Kawah Utama (the S crater, also referred to as the “Main Crater”). The most recent eruption began in late November 2018 and has more recently consisted of weak thermal activity and gas-and-steam emissions (BGVN 48:01). This report updates activity characterized by lava flows, incandescent avalanches, and ash plumes during January through June 2023 using reports from Pusat Vulkanologi dan Mitigasi Bencana Geologi (PVMBG, also known as CVGHM, or the Center of Volcanology and Geological Hazard Mitigation), MAGMA Indonesia, the Darwin VAAC (Volcano Ash Advisory Center), and satellite data.

Activity during January was relatively low and mainly consisted of white gas-and-steam emissions that rose 25-150 m above Main Crater (S crater) and drifted in different directions. Incandescence was visible from the lava dome in Kawah Dua (the N crater). Weather conditions often prevented clear views of the summit. On 18 January the number of seismic signals that indicated avalanches of material began to increase. In addition, there were a total of 71 earthquakes detected during the month.

Activity continued to increase during the first week of February. Material from Main Crater traveled as far as 800 m down the Batuawang (S) and Batang (W) drainages and as far as 1 km W down the Beha (W) drainage on 4 February. On 6 February 43 earthquake events were recorded, and on 7 February, 62 events were recorded. White gas-and-steam emissions rose 25-250 m above both summit craters throughout the month. PVMBG reported an eruption began during the evening of 8 February around 1700. Photos showed incandescent material at Main Crater. Incandescent material had also descended the flank in at least two unconfirmed directions as far as 2 km from Main Crater, accompanied by ash plumes (figure 60). As a result, PVMBG increased the Volcano Alert Level (VAL) to 3 (the second highest level on a 1-4 scale).

Figure 60. Photos of the eruption at Karangetang on 8 February 2023 that consisted of incandescent material descending the flanks (top left), ash plumes (top right and bottom left), and summit crater incandescence (bottom right). Courtesy of IDN Times.

Occasional nighttime webcam images showed three main incandescent lava flows of differing lengths traveling down the S, SW, and W flanks (figure 61). Incandescent rocks were visible on the upper flanks, possibly from ejected or collapsed material from the crater, and incandescence was the most intense at the summit. Based on analyses of satellite imagery and weather models, the Darwin VAAC reported that daily ash plumes during 16-20 February rose to 2.1-3 km altitude and drifted NNE, E, and SE. BNPB reported on 16 February that as many as 77 people were evacuated and relocated to the East Siau Museum. A webcam image taken at 2156 on 17 February possibly showed incandescent material descending the SE flank. Ash plumes rose to 2.1 km altitude and drifted SE during 22-23 February, according to the Darwin VAAC.

Figure 61. Webcam image of summit incandescence and lava flows descending the S, SW, and W flanks of Karangetang on 13 February 2023. Courtesy of MAGMA Indonesia.

Incandescent avalanches of material and summit incandescence at Main Crater continued during March. White gas-and-steam emissions during March generally rose 25-150 m above the summit crater; on 31 March gas-and-steam emissions rose 200-400 m high. An ash plume rose to 2.4 km altitude and drifted S at 1710 on 9 March and a large thermal anomaly was visible in images taken at 0550 and 0930 on 10 March. Incandescent material was visible at the summit and on the flanks based on webcam images taken at 0007 and 2345 on 16 March, at 1828 on 17 March, at 1940 on 18 March, at 2311 on 19 March, and at 2351 on 20 March. Incandescence was most intense on 18 and 20 March and webcam images showed possible Strombolian explosions (figure 62). An ash plume rose to 2.4 km altitude and drifted SW on 18 March, accompanied by a thermal anomaly.

Figure 62. Webcam image of intense summit incandescence and incandescent avalanches descending the flanks of Karangetang on 18 March 2023. Photo has been color corrected. Courtesy of MAGMA Indonesia.

Summit crater incandescence at Main Crater and on the flanks persisted during April. Incandescent material at the S crater and on the flanks was reported at 0016 on 1 April. The lava flows had stopped by 1 April according to PVMBG, although incandescence was still visible up to 10 m high. Seismic signals indicating effusion decreased and by 6 April they were no longer detected. Incandescence was visible from both summit craters. On 26 April the VAL was lowered to 2 (the second lowest level on a 1-4 scale). White gas-and-steam emissions rose 25-200 m above the summit crater.

During May white gas-and-steam emissions generally rose 50-250 m above the summit, though it was often cloudy, which prevented clear views; on 21 May gas-and-steam emissions rose 50-400 m high. Nighttime N summit crater incandescence rose 10-25 m above the lava dome, and less intense incandescence was noted above Main Crater, which reached about 10 m above the dome. Sounds of falling rocks at Main Crater were heard on 15 May and the seismic network recorded 32 rockfall events in the crater on 17 May. Avalanches traveled as far as 1.5 km down the SW and S flanks, accompanied by rumbling sounds on 18 May. Incandescent material descending the flanks was captured in a webcam image at 2025 on 19 May (figure 63) and on 29 May; summit crater incandescence was observed in webcam images at 2332 on 26 May and at 2304 on 29 May. On 19 May the VAL was again raised to 3.

Figure 63. Webcam image showing incandescent material descending the flanks of Karangetang on 19 May 2023. Courtesy of MAGMA Indonesia.

Occasional Main Crater incandescence was reported during June, as well as incandescent material on the flanks. White gas-and-steam emissions rose 10-200 m above the summit crater. Ash plumes rose to 2.1 km altitude and drifted SE and E during 2-4 June, according to the Darwin VAAC. Material on the flanks of Main Crater were observed at 2225 on 7 June, at 2051 on 9 June, at 0007 on 17 June, and at 0440 on 18 June. Webcam images taken on 21, 25, and 27 June showed incandescence at Main Crater and from material on the flanks.

MIROVA (Middle InfraRed Observation of Volcanic Activity) analysis of MODIS satellite data showed strong thermal activity during mid-February through March and mid-May through June, which represented incandescent avalanches and lava flows (figure 64). During April through mid-May the power of the anomalies decreased but frequent anomalies were still detected. Brief gaps in activity occurred during late March through early April and during mid-June. Infrared satellite images showed strong lava flows mainly affecting the SW and S flanks, accompanied by gas-and-steam emissions (figure 65). According to data recorded by the MODVOLC thermal algorithm, there were a total of 79 thermal hotspots detected: 28 during February, 24 during March, one during April, five during May, and 21 during June.

Figure 64. Strong thermal activity was detected during mid-February 2023 through March and mid-May through June at Karangetang during January through June 2023, as recorded by this MIROVA graph (Log Radiative Power). During April through mid-May the power of the anomalies decreased, but the frequency at which they occurred was still relatively high. A brief gap in activity was shown during mid-June. Courtesy of MIROVA.

Figure 65. Incandescent avalanches of material and summit crater incandescence was visible in infrared satellite images (bands 12, 11, 8A) at both the N and S summit crater of Karangetang on 17 February 2023 (top left), 13 April 2023 (top right), 28 May 2023 (bottom left), and 7 June 2023 (bottom right), as shown in these infrared (bands 12, 11, 8A) satellite images. The incandescent avalanches mainly affected the SW and S flanks. Sometimes gas-and-steam plumes accompanied the thermal activity. Courtesy of Copernicus Browser.

Geologic Background. Karangetang (Api Siau) volcano lies at the northern end of the island of Siau, about 125 km NNE of the NE-most point of Sulawesi. The stratovolcano contains five summit craters along a N-S line. It is one of Indonesia's most active volcanoes, with more than 40 eruptions recorded since 1675 and many additional small eruptions that were not documented (Neumann van Padang, 1951). Twentieth-century eruptions have included frequent explosive activity sometimes accompanied by pyroclastic flows and lahars. Lava dome growth has occurred in the summit craters; collapse of lava flow fronts have produced pyroclastic flows.

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.esdm.go.id/v1); Badan Nasional Penanggulangan Bencana (BNPB), National Disaster Management Agency, Graha BNPB - Jl. Scout Kav.38, East Jakarta 13120, Indonesia (URL: http://www.bnpb.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/); Copernicus Browser, Copernicus Data Space Ecosystem, European Space Agency (URL: https://dataspace.copernicus.eu/browser/); IDN Times, Jl. Jend. Gatot Subroto Kav. 27 3rd Floor Kuningan, Jakarta, Indonesia 12950, Status of Karangetang Volcano in Sitaro Islands Increases (URL: https://sulsel.idntimes.com/news/indonesia/savi/status-gunung-api-karangetang-di-kepulauan-sitaro-meningkat?page=all).

Ahyi seamount is a large, conical submarine volcano that rises to within 75 m of the ocean surface about 18 km SE of the island of Farallon de Pajaros in the Northern Marianas. The remote location of the seamount has made eruptions difficult to document, but seismic stations installed in the region confirmed an eruption in the vicinity in 2001. No new activity was detected until April-May 2014 when an eruption was detected by NOAA (National Oceanic and Atmospheric Administration) divers, hydroacoustic sensors, and seismic stations (BGVN 42:04). New activity was first detected on 15 November by hydroacoustic sensors that were consistent with submarine volcanic activity. This report covers activity during November 2022 through June 2023 based on daily and weekly reports from the US Geological Survey.

Starting in mid-October, hydroacoustic sensors at Wake Island (2.2 km E) recorded signals consistent with submarine volcanic activity, according to a report from the USGS issued on 15 November 2022. A combined analysis of the hydroacoustic signals and seismic stations located at Guam and Chichijima Island, Japan, suggested that the source of this activity was at or near the Ahyi seamount. After a re-analysis of a satellite image of the area that was captured on 6 November, USGS confirmed that there was no evidence of discoloration at the ocean surface. Few hydroacoustic and seismic signals continued through November, including on 18 November, which USGS suggested signified a decline or pause in unrest. A VONA (Volcano Observatory Notice for Aviation) reported that a discolored water plume was persistently visible in satellite data starting on 18 November (figure 6). Though clouds often obscured clear views of the volcano, another discolored water plume was captured in a satellite image on 26 November. The Aviation Color Code (ACC) was raised to Yellow (the second lowest level on a four-color scale) and the Volcano Alert Level (VAL) was raised to Advisory (the second lowest level on a four-level scale) on 29 November.

Figure 6. A clear, true color satellite image showed a yellow-green discolored water plume extending NW from the Ahyi seamount (white arrow) on 21 November 2022. Courtesy of Copernicus Browser.

During December, occasional detections were recorded on the Wake Island hydrophone sensors and discolored water over the seamount remained visible. During 2-7, 10-12, and 16-31 December possible explosion signals were detected. A small area of discolored water was observed in high-resolution Sentinel-2 satellite images during 1-6 December (figure 7). High-resolution satellite images recorded discolored water plumes on 13 December that originated from the summit region; no observations indicated that activity breached the ocean surface. A possible underwater plume was visible in satellite images on 18 December, and during 19-20 December a definite but diffuse underwater plume located SSE from the main vent was reported. An underwater plume was visible in a satellite image taken on 26 December (figure 7).

Figure 7. Clear, true color satellite images showed yellow-green discolored water plumes extending NE and W from Ahyi (white arrows) on 1 (left) and 26 (right) December 2022, respectively. Courtesy of Copernicus Browser.

Hydrophone sensors continued to detect signals consistent with possible explosions during 1-8 January 2023. USGS reported that the number of detections decreased during 4-5 January. The hydrophone sensors experienced a data outage that started at 0118 on 8 January and continued through 10 January, though according to USGS, possible explosions were recorded prior to the data outage and likely continued during the outage. A discolored water plume originating from the summit region was detected in a partly cloudy satellite image on 8 January. On 11-12 and 15-17 January possible explosion signals were recorded again. One small signal was detected during 22-23 January and several signals were recorded on 25 and 31 January. During 27-31 January a plume of discolored water was observed above the seamount in satellite imagery (figure 8).

Figure 8. True color satellite images showed intermittent yellow-green discolored water plumes of various sizes extending N on 5 January 2023 (top left), SE on 30 January 2023 (top right), W on 4 February 2023 (bottom left), and SW on 1 March 2023 (bottom right) from Ahyi (white arrows). Courtesy of Copernicus Browser.

Low levels of activity continued during February and March, based on data from pressure sensors on Wake Island. During 1 and 4-6 February activity was reported, and a submarine plume was observed on 4 February (figure 8). Possible explosion signals were detected during 7-8, 10, 13-14, and 24 February. During 1-2 and 3-5 March a plume of discolored water was observed in satellite imagery (figure 8). Almost continuous hydroacoustic signals were detected in remote pressure sensor data on Wake Island 2,270 km E from the volcano during 7-13 March. During 12-13 March water discoloration around the seamount was observed in satellite imagery, despite cloudy weather. By 14 March discolored water extended about 35 km, but no direction was noted. USGS reported that the continuous hydroacoustic signals detected during 13-14 March stopped abruptly on 14 March and no new detections were observed. Three 30 second hydroacoustic detections were reported during 17-19 March, but no activity was visible due to cloudy weather. A data outage was reported during 21-22 March, making pressure sensor data unavailable; a discolored water plume was, however, visible in satellite data. A possible underwater explosion signal was detected by pressure sensors at Wake Island on 26, 29, and 31 March, though the cause and origin of these events were unclear.

Similar low activity continued during April, May, and June. Several signals were detected during 1-3 April in pressure sensors at Wake Island. USGS suggested that these may be related to underwater explosions or earthquakes at the volcano, but no underwater plumes were visible in clear satellite images. The pressure sensors had data outages during 12-13 April and no data were recorded; no underwater plumes were visible in satellite images, although cloudy weather obscured most clear views. Eruptive activity was reported starting at 2210 on 21 May. On 22 May a discolored water plume that extended 4 km was visible in satellite images, though no direction was recorded. During 23-24 May some signals were detected by the underwater pressure sensors. Possible hydroacoustic signals were detected during 2-3 and 6-8 June. Multiple hydroacoustic signals were detected during 9-11 and 16-17 June, although no activity was visible in satellite images. One hydroacoustic signal was detected during 23-24 June, but there was some uncertainty about its association with volcanic activity. A single possible hydroacoustic signal was detected during 30 June to 1 July.

Geologic Background. Ahyi seamount is a large conical submarine volcano that rises to within 75 m of the ocean surface ~18 km SE of the island of Farallon de Pajaros in the northern Marianas. Water discoloration has been observed there, and in 1979 the crew of a fishing boat felt shocks over the summit area, followed by upwelling of sulfur-bearing water. On 24-25 April 2001 an explosive eruption was detected seismically by a station on Rangiroa Atoll, Tuamotu Archipelago. The event was well constrained (+/- 15 km) at a location near the southern base of Ahyi. An eruption in April-May 2014 was detected by NOAA divers, hydroacoustic sensors, and seismic stations.

Information Contacts: US Geological Survey, Volcano Hazards Program (USGS-VHP), 12201 Sunrise Valley Drive, Reston, VA, USA, https://volcanoes.usgs.gov/index.html; Copernicus Browser, Copernicus Data Space Ecosystem, European Space Agency (URL: https://dataspace.copernicus.eu/browser/).

Kadovar is a 2-km-wide island that is the emergent summit of a Bismarck Sea stratovolcano. It lies off the coast of New Guinea, about 25 km N of the mouth of the Sepik River. Prior to an eruption that began in 2018, a lava dome formed the high point of the volcano, filling an arcuate landslide scarp open to the S. Submarine debris-avalanche deposits occur to the S of the island. The current eruption began in January 2018 and has comprised lava effusion from vents at the summit and at the E coast; more recent activity has consisted of ash plumes, weak thermal activity, and gas-and-steam plumes (BGVN 48:02). This report covers activity during February through May 2023 using information from the Darwin Volcanic Ash Advisory Center (VAAC) and satellite data.

Activity during the reporting period was relatively low and mainly consisted of white gas-and-steam plumes that were visible in natural color satellite images on clear weather days (figure 67). According to a Darwin VAAC report, at 2040 on 6 May an ash plume rose to 4.6 km altitude and drifted W; by 2300 the plume had dissipated. MODIS satellite instruments using the MODVOLC thermal algorithm detected a single thermal hotspot on the SE side of the island on 7 May. Weak thermal activity was also detected in a satellite image on the E side of the island on 14 May, accompanied by a white gas-and-steam plume that drifted SE (figure 68).

Figure 67. True color satellite images showing a white gas-and-steam plume rising from Kadovar on 28 February 2023 (left) and 30 March 2023 (right) and drifting SE and S, respectively. Courtesy of Copernicus Browser.

Figure 68. Infrared (bands B12, B11, B4) image showing weak thermal activity on the E side of the island, accompanied by a gas-and-steam plume that drifted SE from Kadovar on 14 May 2023. Courtesy of Copernicus Browser.

Geologic Background. The 2-km-wide island of Kadovar is the emergent summit of a Bismarck Sea stratovolcano of Holocene age. It is part of the Schouten Islands, and lies off the coast of New Guinea, about 25 km N of the mouth of the Sepik River. Prior to an eruption that began in 2018, a lava dome formed the high point of the andesitic volcano, filling an arcuate landslide scarp open to the south; submarine debris-avalanche deposits occur in that direction. Thick lava flows with columnar jointing forms low cliffs along the coast. The youthful island lacks fringing or offshore reefs. A period of heightened thermal phenomena took place in 1976. An eruption began in January 2018 that included lava effusion from vents at the summit and at the E coast.

Information Contacts: 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/); Copernicus Browser, Copernicus Data Space Ecosystem, European Space Agency (URL: https://dataspace.copernicus.eu/browser/).

San Miguel in El Salvador is a broad, deep crater complex that has been frequently modified by eruptions recorded since the early 16th century and consists of the summit known locally as Chaparrastique. Flank eruptions have produced lava flows that extended to the N, NE, and SE during the 17-19th centuries. The most recent activity has consisted of minor ash eruptions from the summit crater. The current eruption period began in November 2022 and has been characterized by frequent phreatic explosions, gas-and-ash emissions, and sulfur dioxide plumes (BGVN 47:12). This report describes small gas-and-ash explosions during December 2022 through May 2023 based on special reports from the Ministero de Medio Ambiente y Recursos Naturales (MARN).

Activity has been relatively low since the last recorded explosions on 29 November 2022. Seismicity recorded by the San Miguel Volcano Station (VSM) located on the N flank at 1.7 km elevation had decreased by 7 December. Sulfur dioxide gas measurements taken with DOAS (Differential Optical Absorption Spectroscopy) mobile equipment were below typical previously recorded values: 300 tons per day (t/d). During December, small explosions were recorded by the seismic network and manifested as gas-and-steam emissions.

Gas-and-ash explosions in the crater occurred during January 2023, which were recorded by the seismic network. Sulfur dioxide values remained low, between 300-400 t/d through 10 March. At 0817 on 14 January a gas-and-ash emission was visible in webcam images, rising just above the crater rim. Some mornings during February, small gas-and-steam plumes were visible in the crater. On 7 March at 2252 MARN noted an increase in degassing from the central crater; gas emissions were constantly observed through the early morning hours on 8 March. During the early morning of 8 March through the afternoon on 9 March, 12 emissions were registered, some accompanied by ash. The last gas-and-ash emission was recorded at 1210 on 9 March; very fine ashfall was reported in El Tránsito (10 km S), La Morita (6 km W), and La Piedrita (3 km W). The smell of sulfur was reported in Piedra Azul (5 km SW). On 16 March MARN reported that gas-and-steam emissions decreased.

Low degassing and very low seismicity were reported during April; no explosions have been detected between 9 March and 27 May. The sulfur dioxide emissions remained between 350-400 t/d; during 13-20 April sulfur dioxide values fluctuated between 30-300 t/d. Activity remained low through most of May; on 23 May seismicity increased. An explosion was detected at 1647 on 27 May generated a gas-and-ash plume that rose 700 m high (figure 32); a decrease in seismicity and gas emissions followed. The DOAS station installed on the W flank recorded sulfur dioxide values that reached 400 t/d on 27 May; subsequent measurements showed a decrease to 268 t/d on 28 May and 100 t/d on 29 May.

Figure 32. Webcam image of a gas-and-ash plume rising 700 m above San Miguel at 1652 on 27 May 2023. Courtesy of MARN.

Geologic Background. The symmetrical cone of San Miguel, one of the most active volcanoes in El Salvador, rises from near sea level to form one of the country's most prominent landmarks. A broad, deep, crater complex that has been frequently modified by eruptions recorded since the early 16th century caps the truncated unvegetated summit, also known locally as Chaparrastique. Flanks eruptions of the basaltic-andesitic volcano have produced many lava flows, including several during the 17th-19th centuries that extended to the N, NE, and SE. The SE-flank flows are the largest and form broad, sparsely vegetated lava fields crossed by highways and a railroad skirting the base of the volcano. Flank vent locations have migrated higher on the edifice during historical time, and the most recent activity has consisted of minor ash eruptions from the summit crater.

Information Contacts: Ministero de Medio Ambiente y Recursos Naturales (MARN), Km. 5½ Carretera a Nueva San Salvador, Avenida las Mercedes, San Salvador, El Salvador (URL: http://www.snet.gob.sv/ver/vulcanologia).

Semisopochnoi is located in the western Aleutians, is 20-km-wide at sea level, and contains an 8-km-wide caldera. The three-peaked Mount Young (formerly Cerberus) was constructed within the caldera during the Holocene. Each of these peaks contains a summit crater; the lava flows on the N flank appear younger than those on the S side. The current eruption period began in early February 2021 and has more recently consisted of intermittent explosions and ash emissions (BGVN 47:12). This report updates activity during December 2022 through May 2023 using daily, weekly, and special reports from the Alaska Volcano Observatory (AVO). AVO monitors the volcano using local seismic and infrasound sensors, satellite data, web cameras, and remote infrasound and lightning networks.

Activity during most of December 2022 was relatively quiet; according to AVO no eruptive or explosive activity was observed since 7 November 2022. Intermittent tremor and occasional small earthquakes were observed in geophysical data. Continuous gas-and-steam emissions were observed from the N crater of Mount Young in webcam images on clear weather days (figure 25). On 24 December, there was a slight increase in earthquake activity and several small possible explosion signals were detected in infrasound data. Eruptive activity resumed on 27 December at the N crater of Mount Young; AVO issued a Volcano Activity Notice (VAN) that reported minor ash deposits on the flanks of Mount Young that extended as far as 1 km from the vent, according to webcam images taken during 27-28 December (figure 26). No ash plumes were observed in webcam or satellite imagery, but a persistent gas-and-steam plume that might have contained some ash rose to 1.5 km altitude. As a result, AVO raised the Aviation Color Code (ACC) to Orange (the second highest level on a four-color scale) and the Volcano Alert Level (VAL) to Watch (the second highest level on a four-level scale). Possible explosions were detected during 21 December 2022 through 1 January 2023 and seismic tremor was recorded during 30-31 December.

Figure 25. Webcam image of a gas-and-steam plume rising above Semisopochnoi from Mount Young on 21 December 2022. Courtesy of AVO.

Figure 26. Webcam image showing fresh ash deposits (black color) at the summit and on the flanks of Mount Young at Semisopochnoi, extending up to 1 km from the N crater. Image was taken on 27 December 2022. Image has been color corrected. Courtesy of AVO.

During January 2023 eruptive activity continued at the active N crater of Mount Young. Minor ash deposits were observed on the flanks, extending about 2 km SSW, based on webcam images from 1 and 3 January. A possible explosion occurred during 1-2 January based on elevated seismicity recorded on local seismometers and an infrasound signal recorded minutes later by an array at Adak. Though no ash plumes were observed in webcam or satellite imagery, a persistent gas-and-steam plume rose to 1.5 km altitude that might have carried minor traces of ash. Ash deposits were accompanied by periods of elevated seismicity and infrasound signals from the local geophysical network, which AVO reported were likely due to weak explosive activity. Low-level explosive activity was also detected during 2-3 January, with minor gas-and-steam emissions and a new ash deposit that was visible in webcam images. Low-level explosive activity was detected in geophysical data during 4-5 January, with elevated seismicity and infrasound signals observed on local stations. Volcanic tremor was detected during 7-9 January and very weak explosive activity was detected in seismic and infrasound data on 9 January. Weak seismic and infrasound signals were recorded on 17 January, which indicated minor explosive activity, but no ash emissions were observed in clear webcam images; a gas-and-steam plume continued to rise to 1.5 km altitude. During 29-30 January, ash deposits near the summit were observed on fresh snow, according to webcam images.

The active N cone at Mount Young continued to produce a gas-and-steam plume during February, but no ash emissions or explosive events were detected. Seismicity remained elevated with faint tremor during early February. Gas-and-steam emissions from the N crater were observed in clear webcam images on 11-13 and 16 February; no explosive activity was detected in seismic, infrasound, or satellite data. Seismicity has also decreased, with no significant seismic tremor observed since 25 January. Therefore, the ACC was lowered to Yellow (the second lowest level on a four-color scale) and the VAL was lowered to Advisory (the second lowest level on a four-color scale) on 22 February.

Gas-and-steam emissions persisted during March from the N cone of Mount Young, based on clear webcam images. A few brief episodes of weak tremor were detected in seismic data, although seismicity decreased over the month. A gas-and-steam plume detected in satellite data extended 150 km on 18 March. Low-level ash emissions from the N cone at Mount Young were observed in several webcam images during 18-19 March, in addition to small explosions and volcanic tremor. The ACC was raised to Orange and the VAL increased to Watch on 19 March. A small explosion was detected in seismic and infrasound data on 21 March.

Low-level unrest continued during April, although cloudy weather often obscured views of the summit; periods of seismic tremor and local earthquakes were recorded. During 3-4 April a gas-and-steam plume was visible traveling more than 200 km overnight; no ash was evident in the plume, according to AVO. A gas-and-steam plume was observed during 4-6 April that extended 400 km but did not seem to contain ash. Small explosions were detected in seismic and infrasound data on 5 April. Occasional clear webcam images showed continuing gas-and-steam emissions rose from Mount Young, but no ash deposits were observed on the snow. On 19 April small explosions and tremor were detected in seismic and infrasound data. A period of seismic tremor was detected during 22-25 April, with possible weak explosions on 25 April. Ash deposits were visible near the crater rim, but it was unclear if these deposits were recent or due to older deposits.

Occasional small earthquakes were recorded during May, but there were no signs of explosive activity seen in geophysical data. Gas-and-steam emissions continued from the N crater of Mount Young, based on webcam images, and seismicity remained slightly elevated. A new, light ash deposit was visible during the morning of 5 May on fresh snow on the NW flank of Mount Young. During 10 May periods of volcanic tremor were observed. The ACC was lowered to Yellow and the VAL to Advisory on 17 May due to no additional evidence of activity.

Geologic Background. Semisopochnoi, the largest subaerial volcano of the western Aleutians, is 20 km wide at sea level and contains an 8-km-wide caldera. It formed as a result of collapse of a low-angle, dominantly basaltic volcano following the eruption of a large volume of dacitic pumice. The high point of the island is Anvil Peak, a double-peaked late-Pleistocene cone that forms much of the island's northern part. The three-peaked Mount Cerberus (renamed Mount Young in 2023) was constructed within the caldera during the Holocene. Each of the peaks contains a summit crater; lava flows on the N flank appear younger than those on the south side. Other post-caldera volcanoes include the symmetrical Sugarloaf Peak SSE of the caldera and Lakeshore Cone, a small cinder cone at the edge of Fenner Lake in the NE part of the caldera. Most documented eruptions have originated from Young, although Coats (1950) considered that both Sugarloaf and Lakeshore Cone could have been recently active.

Information Contacts: Alaska Volcano Observatory (AVO), a cooperative program of a) U.S. Geological Survey, 4200 University Drive, Anchorage, AK 99508-4667 USA (URL: https://avo.alaska.edu/), b) Geophysical Institute, University of Alaska, PO Box 757320, Fairbanks, AK 99775-7320, USA, and c) Alaska Division of Geological & Geophysical Surveys, 794 University Ave., Suite 200, Fairbanks, AK 99709, USA (URL: http://dggs.alaska.gov/).

Ebeko, located on the N end of Paramushir Island in the Kuril Islands, consists of three summit craters along a SSW-NNE line at the northern end of a complex of five volcanic cones. Eruptions date back to the late 18th century and have been characterized as small-to-moderate explosions from the summit crater, accompanied by intense fumarolic activity. The current eruption period began in June 2022 and has recently consisted of frequent explosions, ash plumes, and thermal activity (BGVN 47:10). This report covers similar activity during October 2022 through May 2023, based on information from the Kamchatka Volcanic Eruptions Response Team (KVERT) and satellite data.

Activity during October consisted of explosive activity, ash plumes, and occasional thermal anomalies. Visual data by volcanologists from Severo-Kurilsk showed explosions producing ash clouds up to 2.1-3 km altitude which drifted E, N, NE, and SE during 1-8, 10, 16, and 18 October. KVERT issued several Volcano Observatory Notices for Aviation (VONA) on 7, 13-15, and 27 October 2022, stating that explosions generated ash plumes that rose to 2.3-4 km altitude and drifted 5 km E, NE, and SE. Ashfall was reported in Severo-Kurilsk (Paramushir Island, about 7 km E) on 7 and 13 October. Satellite data showed a thermal anomaly over the volcano on 15-16 October. Visual data showed ash plumes rising to 2.5-3.6 km altitude on 22, 25-29, and 31 October and moving NE due to constant explosions.

Similar activity continued during November, with explosions, ash plumes, and ashfall occurring. KVERT issued VONAs on 1-2, 4, 6-7, 9, 13, and 16 November that reported explosions and resulting ash plumes that rose to 1.7-3.6 km altitude and drifted 3-5 km SE, ESE, E, and NE. On 1 November ash plumes extended as far as 110 km SE. On 5, 8, 12, and 24-25 November explosions and ash plumes rose to 2-3.1 km altitude and drifted N and E. Ashfall was observed in Severo-Kurilsk on 7 and 16 November. A thermal anomaly was visible during 1-4, 16, and 20 November. Explosions during 26 November rose as high as 2.7 km altitude and drifted NE (figure 45).

Figure 45. Photo of an ash plume rising to 2.7 km altitude above Ebeko on 26 November 2022. Photo has been color corrected. Photo by L. Kotenko, IVS FEB RAS.

Explosions and ash plumes continued to occur in December. During 1-2 and 4 December volcanologists from Severo-Kurilsk observed explosions that sent ash to 1.9-2.5 km altitude and drifted NE and SE (figure 46). VONAs were issued on 5, 9, and 16 December reporting that explosions generated ash plumes rising to 1.9 km, 2.6 km, and 2.4 km altitude and drifted 5 km SE, E, and NE, respectively. A thermal anomaly was visible in satellite imagery on 16 December. On 18 and 27-28 December explosions produced ash plumes that rose to 2.5 km altitude and drifted NE and SE. On 31 December an ash plume rose to 2 km altitude and drifted NE.

Figure 46. Photo of an explosive event at Ebeko at 1109 on 2 December 2022. Photo has been color corrected. Photo by S. Lakomov, IVS FEB RAS.

Explosions continued during January 2023, based on visual observations by volcanologists from Severo-Kurilsk. During 1-7 January explosions generated ash plumes that rose to 4 km altitude and drifted NE, E, W, and SE. According to VONAs issued by KVERT on 2, 4, 10, and 23 January, explosions produced ash plumes that rose to 2-4 km altitude and drifted 5 km N, NE, E, and ENE; the ash plume that rose to 4 km altitude occurred on 10 January (figure 47). Satellite data showed a thermal anomaly during 3-4, 10, 13, 16, 21, 22, and 31 January. KVERT reported that an ash cloud on 4 January moved 12 km NE. On 6 and 9-11 January explosions sent ash plumes to 4.5 km altitude and drifted W and ESE. On 13 January an ash plume rose to 3 km altitude and drifted SE. During 20-24 January ash plumes from explosions rose to 3.7 km altitude and drifted SE, N, and NE. On 21 January the ash plume drifted as far as 40 km NE. During 28-29 and 31 January and 1 February ash plumes rose to 4 km altitude and drifted NE.

Figure 47. Photo of a strong ash plume rising to 4 km altitude from an explosive event on 10 January 2023 (local time). Photo by L. Kotenko, IVS FEB RAS.

During February, explosions, ash plumes, and ashfall were reported. During 1, 4-5 and 7-8 February explosions generated ash plumes that rose to 4.5 km altitude and drifted E and NE; ashfall was observed on 5 and 8 February. On 6 February an explosion produced an ash plume that rose to 3 km altitude and drifted 7 km E, causing ashfall in Severo-Kurilsk. A thermal anomaly was visible in satellite data on 8, 9, 13, and 21 February. Explosions on 9 and 12-13 February produced ash plumes that rose to 4 km altitude and drifted E and NE; the ash cloud on 12 February extended as far as 45 km E. On 22 February explosions sent ash to 3 km altitude that drifted E. During 24 and 26-27 February ash plumes rose to 4 km altitude and drifted E. On 28 February an explosion sent ash to 2.5-3 km altitude and drifted 5 km E; ashfall was observed in Severo-Kurilsk.

Activity continued during March; visual observations showed that explosions generated ash plumes that rose to 3.6 km altitude on 3, 5-7, and 9-12 March and drifted E, NE, and NW. Thermal anomalies were visible on 10, 13, and 29-30 March in satellite imagery. On 18, 21-23, 26, and 29-30 March explosions produced ash plumes that rose to 2.8 km altitude and drifted NE and E; the ash plumes during 22-23 March extended up to 76 km E. A VONA issued on 21 March reported an explosion that produced an ash plume that rose to 2.8 km altitude and drifted 5 km E. Another VONA issued on 23 March reported that satellite data showed an ash plume rising to 3 km altitude and drifted 14 km E.

Explosions during April continued to generate ash plumes. On 1 and 4 April an ash plume rose to 2.8-3.5 km altitude and drifted SE and NE. A thermal anomaly was visible in satellite imagery during 1-6 April. Satellite data showed ash plumes and clouds rising to 2-3 km altitude and drifting up to 12 km SW and E on 3 and 6 April (figure 48). KVERT issued VONAs on 3, 5, 14, 16 April describing explosions that produced ash plumes rising to 3 km, 3.5 km, 3.5 km, and 3 km altitude and drifting 5 km S, 5 km NE and SE, 72 km NNE, and 5 km NE, respectively. According to satellite data, the resulting ash cloud from the explosion on 14 April was 25 x 7 km in size and drifted 72-104 km NNE during 14-15 April. According to visual data by volcanologists from Severo-Kurilsk explosions sent ash up to 3.5 km altitude that drifted NE and E during 15-16, 22, 25-26, and 29 April.

Figure 48. Photo of an ash cloud rising to 3.5 km altitude at Ebeko on 6 April 2023. The cloud extended up to 12 km SW and E. Photo has been color corrected. Photo by L. Kotenko, IVS FEB RAS.

The explosive eruption continued during May. Explosions during 3-4, 6-7, and 9-10 May generated ash plumes that rose to 4 km altitude and drifted SW and E. Satellite data showed a thermal anomaly on 3, 9, 13-14, and 24 May. During 12-16, 23-25, and 27-28 May ash plumes rose to 3.5 km altitude and drifted in different directions due to explosions. Two VONA notices were issued on 16 and 25 May, describing explosions that generated ash plumes rising to 3 km and 3.5 km altitude, respectively and extending 5 km E. The ash cloud on 25 May drifted 75 km SE.

Thermal activity in the summit crater, occasionally accompanied by ash plumes and ash deposits on the SE and E flanks due to frequent explosions, were visible in infrared and true color satellite images (figure 49).

Figure 49. Infrared (bands B12, B11, B4) and true color satellite images of Ebeko showing occasional small thermal anomalies at the summit crater on 4 October 2022 (top left), 30 April 2023 (bottom left), and 27 May 2023 (bottom right). On 1 November (top right) ash deposits (light-to-dark gray) were visible on the SE flank. An ash plume drifted NE on 30 April, and ash deposits were also visible to the E on both 30 April and 27 May. Courtesy of Copernicus Browser.

Geologic Background. The flat-topped summit of the central cone of Ebeko volcano, one of the most active in the Kuril Islands, occupies the northern end of Paramushir Island. Three summit craters located along a SSW-NNE line form Ebeko volcano proper, at the northern end of a complex of five volcanic cones. Blocky lava flows extend west from Ebeko and SE from the neighboring Nezametnyi cone. The eastern part of the southern crater contains strong solfataras and a large boiling spring. The central crater is filled by a lake about 20 m deep whose shores are lined with steaming solfataras; the northern crater lies across a narrow, low barrier from the central crater and contains a small, cold crescentic lake. Historical activity, recorded since the late-18th century, has been restricted to small-to-moderate explosive eruptions from the summit craters. Intense fumarolic activity occurs in the summit craters, on the outer flanks of the cone, and in lateral explosion craters.

Information Contacts: Kamchatka Volcanic Eruptions Response Team (KVERT), Far Eastern Branch, Russian Academy of Sciences, 9 Piip Blvd., Petropavlovsk-Kamchatsky, 683006, Russia (URL: http://www.kscnet.ru/ivs/kvert/); 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/); Copernicus Browser, Copernicus Data Space Ecosystem, European Space Agency (URL: https://dataspace.copernicus.eu/browser/).

Home Reef is a submarine volcano located in the central Tonga islands between Lateiki (Metis Shoal) and Late Island. The first recorded eruption occurred in the mid-19th century, when an ephemeral island formed. An eruption in 1984 produced a 12-km-high eruption plume, a large volume of floating pumice, and an ephemeral island 500 x 1,500 m wide, with cliffs 30-50 m high that enclosed a water-filled crater. Another island-forming eruption in 2006 produced widespread pumice rafts that drifted as far as Australia; by 2008 the island had eroded below sea level. The previous eruption occurred during October 2022 and was characterized by a new island-forming eruption, lava effusion, ash plumes, discolored water, and gas-and-steam plumes (BGVN 47:11). This report covers discolored water plumes during November 2022 through April 2023 using satellite data.

Discolored plumes continued during the reporting period and were observed in true color satellite images on clear weather days. Satellite images show light green-yellow discolored water extending W on 8 and 28 November 2022 (figure 31), and SW on 18 November. Light green-yellow plumes extended W on 3 December, S on 13 December, SW on 18 December, and W and S on 23 December (figure 31). On 12 January 2023 discolored green-yellow plumes extended to the NE, E, SE, and N. The plume moved SE on 17 January and NW on 22 January. Faint discolored water in February was visible moving NE on 1 February. A discolored plume extended NW on 8 and 28 March and NW on 13 March (figure 31). During April, clear weather showed green-blue discolored plumes moving S on 2 April, W on 7 April, and NE and S on 12 April. A strong green-yellow discolored plume extended E and NE on 22 April for several kilometers (figure 31).

Figure 31. Visual (true color) satellite images showing continued green-yellow discolored plumes at Home Reef (black circle) that extended W on 28 November 2022 (top left), W and S on 23 December 2022 (top right), NW on 13 March 2023 (bottom left), and E and NE on 22 April 2023 (bottom right). Courtesy of Copernicus Browser.

Geologic Background. Home Reef, a submarine volcano midway between Metis Shoal and Late Island in the central Tonga islands, was first reported active in the mid-19th century, when an ephemeral island formed. An eruption in 1984 produced a 12-km-high eruption plume, large amounts of floating pumice, and an ephemeral 500 x 1,500 m island, with cliffs 30-50 m high that enclosed a water-filled crater. In 2006 an island-forming eruption produced widespread dacitic pumice rafts that drifted as far as Australia. Another island was built during a September-October 2022 eruption.

Information Contacts: Copernicus Browser, Copernicus Data Space Ecosystem, European Space Agency (URL: https://dataspace.copernicus.eu/browser/).

Ambae, also known as Aoba, is a large basaltic shield volcano in Vanuatu. A broad pyroclastic cone containing three crater lakes (Manaro Ngoru, Voui, and Manaro Lakua) is located at the summit within the youngest of at least two nested calderas. Periodic phreatic and pyroclastic explosions have been reported since the 16th century. A large eruption more than 400 years ago resulted in a volcanic cone within the summit crater that is now filled by Lake Voui; the similarly sized Lake Manaro fills the western third of the caldera. The previous eruption ended in August 2022 that was characterized by gas-and-steam and ash emissions and explosions of wet tephra (BGVN 47:10). This report covers a new eruption during February through May 2023 that consisted of a new lava flow, ash plumes, and sulfur dioxide emissions, using information from the Vanuatu Meteorology and Geo-Hazards Department (VMGD) and satellite data.

During the reporting period, the Alert Level remained at a 2 (on a scale of 0-5), which has been in place since December 2021. Activity during October 2022 through March 2023 remained relatively low and mostly consisted of gas-and-steam emissions in Lake Voui. VMGD reported that at 1300 on 15 November a satellite image captured a strong amount of sulfur dioxide rising above the volcano (figure 99), and that seismicity slightly increased. The southern and northern part of the island reported a strong sulfur dioxide smell and heard explosions. On 20 February 2023 a gas-and-ash plume rose 1.3 km above the summit and drifted SSW, according to a webcam image (figure 100). Gas-and-steam and possibly ash emissions continued on 23 February and volcanic earthquakes were recorded by the seismic network.

Figure 99. Satellite image of the strong sulfur dioxide plume above Ambae taken on 15 November 2022. The Dobson Units (DU) exceeded 12. Courtesy of VMGD.

Figure 100. Webcam image of a gas-and-ash plume rising above Ambae at 1745 on 20 February 2023. The plume drifted SSW. Courtesy of VMGD.

During April, volcanic earthquakes and gas-and-steam and ash emissions were reported from the cone in Lake Voui. VMGD reported that activity increased during 5-7 April; high gas-and-steam and ash plumes were visible, accompanied by nighttime incandescence. According to a Wellington VAAC report, a low-level ash plume rose as high as 2.5 km above the summit and drifted W and SW on 5 April, based on satellite imagery. Reports in Saratamata stated that a dark ash plume drifted to the WSW, but no loud explosion was heard. Webcam images from 2100 showed incandescence above the crater and reflected in the clouds. According to an aerial survey, field observations, and satellite data, water was no longer present in the lake. A lava flow was reported effusing from the vent and traveling N into the dry Lake Voui, which lasted three days. The next morning at 0745 on 6 April a gas-and-steam and ash plume rose 5.4 km above the summit and drifted ESE, based on information from VMGD (figure 101). The Wellington VAAC also reported that light ashfall was observed on the island. Intermittent gas-and-steam and ash emissions were visible on 7 April, some of which rose to an estimated 3 km above the summit and drifted E. Webcam images during 0107-0730 on 7 April showed continuing ash emissions. A gas-and-steam and ash plume rose 695 m above the summit crater at 0730 on 19 April and drifted ESE, based on a webcam image (figure 102).

Figure 101. Webcam image showing a gas-and-ash plume rising 5.4 km above the summit of Ambae at 0745 on 6 April 2023. Courtesy of VMGD.

Figure 102. Webcam image showing a gas-and-ash plume rising 695 m above the summit of Ambae at 0730 on 19 April 2023. Courtesy of VMGD.

According to visual and infrared satellite data, water was visible in Lake Voui as late as 24 March 2023 (figure 103). The vent in the caldera showed a gas-and-steam plume drifted SE. On 3 April thermal activity was first detected, accompanied by a gas-and-ash plume that drifted W (figure 103). The lava flow moved N within the dry lake and was shown cooling by 8 April. By 23 April much of the water in the lake had returned. Occasional sulfur dioxide plumes were detected by the TROPOMI instrument on the Sentinel-5P satellite that exceeded 2 Dobson Units (DU) and drifted in different directions (figure 104).

Figure 103. Satellite images showing both visual (true color) and infrared (bands B12, B11, B4) views on 24 March 2023 (top left), 3 April 2023 (top left), 8 April 2023 (bottom left), and 23 April 2023 (bottom right). In the image on 24 March, water filled Lake Voui around the small northern lake. A gas-and-steam plume drifted SE. Thermal activity (bright yellow-orange) was first detected in infrared data on 3 April 2023, accompanied by a gas-and-ash plume that drifted W. The lava flow slowly filled the northern part of the then-dry lake and remained hot on 8 April. By 23 April, the water in Lake Voui had returned. Courtesy of Copernicus Browser.

Figure 104. Images showing sulfur dioxide plumes rising from Ambae on 26 December 2022 (top left), 25 February 2023 (top right), 23 March 2023 (bottom left), and 5 April 2023 (bottom right), as detected by the TROPOMI instrument on the Sentinel-5P satellite. These plumes exceeded at least 2 Dobson Units (DU) and drifted in different directions. Courtesy of the NASA Global Sulfur Dioxide Monitoring Page.

Geologic Background. The island of Ambae, also known as Aoba, is a massive 2,500 km3 basaltic shield that is the most voluminous volcano of the New Hebrides archipelago. A pronounced NE-SW-trending rift zone with numerous scoria cones gives the 16 x 38 km island an elongated form. A broad pyroclastic cone containing three crater lakes (Manaro Ngoru, Voui, and Manaro Lakua) is located at the summit within the youngest of at least two nested calderas, the largest of which is 6 km in diameter. That large central edifice is also called Manaro Voui or Lombenben volcano. Post-caldera explosive eruptions formed the summit craters about 360 years ago. A tuff cone was constructed within Lake Voui (or Vui) about 60 years later. The latest known flank eruption, about 300 years ago, destroyed the population of the Nduindui area near the western coast.

Information Contacts: Geo-Hazards Division, Vanuatu Meteorology and Geo-Hazards Department (VMGD), Ministry of Climate Change Adaptation, Meteorology, Geo-Hazards, Energy, Environment and Disaster Management, Private Mail Bag 9054, Lini Highway, Port Vila, Vanuatu (URL: http://www.vmgd.gov.vu/, https://www.facebook.com/VanuatuGeohazardsObservatory/); Wellington Volcanic Ash Advisory Centre (VAAC), Meteorological Service of New Zealand Ltd (MetService), PO Box 722, Wellington, New Zealand (URL: http://www.metservice.com/vaac/, http://www.ssd.noaa.gov/VAAC/OTH/NZ/messages.html); 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/); Global Sulfur Dioxide Monitoring Page, Atmospheric Chemistry and Dynamics Laboratory, NASA Goddard Space Flight Center (NASA/GSFC), 8800 Greenbelt Road, Goddard, Maryland, USA (URL: https://so2.gsfc.nasa.gov/); Copernicus Browser, Copernicus Data Space Ecosystem, European Space Agency (URL: https://dataspace.copernicus.eu/browser/).

Sakurajima rises from Kagoshima Bay, which fills the Aira Caldera near the southern tip of Japan's Kyushu Island. Frequent explosive and occasional effusive activity has been ongoing for centuries. The Minamidake summit cone has been the location of persistent activity since 1955; the Showa crater on its E flank has been the most active site since 2006. Tens of explosions and ash-bearing emissions have been occurring monthly for the last several years and were continuous through October 2015. After a three-month break, activity resumed in February 2016 and lasted through August 2016. No further activity was reported through December 2016. The Japan Meteorological Agency (JMA) provided regular reports on activity, and the Tokyo VAAC (Volcanic Ash Advisory Center) issued hundreds of reports about ash plumes during 2015-2016.

The number of explosive events at the Showa crater of Sakurajima increased from January-May 2015. During the period, ash emissions commonly rose 3,000 m above the crater rim, and a few exceeded 4,000 m; tephra was often ejected 1.3 km and as far as 1.8 km from the crater. Incandescence was observed every week; multiple MODVOLC thermal alerts were reported monthly from January-June 2015. The Tokyo VAAC issued 845 reports between 1 January and 14 October 2015. The number of monthly explosions decreased sharply during June-August. Tiltmeter and strainmeter data indicated continuing inflation through mid-August when the inflation rate increased significantly for a brief period. This was followed by deflation for the remainder of 2015. Pyroclastic flows were reported in March, April, and June. Minor emissions occurred at Minamidake crater in May, June, and August. Activity increased at both craters during September, with the first substantial explosion at Minamidake in almost a year. An emission from Showa on 2 November 2015 was noted in a JMA weekly report, but its composition was not described; the last confirmed ash emission of the year was on 14 October 2015.

After three months of quiet, a substantial explosion at Showa in early February 2016 marked the beginning of a new eruptive episode that continued through the end of July, after which explosive activity ceased at Showa for the remainder of the year (figure 49). Minor emissions were reported at Minamidake through August 2016. Pyroclastic flows occurred in April and June from explosions at the Showa crater. Inflation was measured again beginning in April 2016 and continued through December 2016.

Figure 49. Explosions from the Showa crater at Sakurajima, January 2013-December 2016. Data do not include activity at Minamidake crater, or passive (non-explosive) ash or steam emissions from Showa. After many years of multiple monthly explosions, activity decreased in September 2015. A smaller burst of activity occurred from February to July 2016. Data compiled from JMA reports.

Activity during January-May 2015. JMA reported 61 explosions from the Showa crater during January 2015, twice the number recorded in December 2014 (figure 50). Explosions on 4 and 30 January sent ejecta as far as 1.8 km from the crater. The maximum plume height reported by JMA was 4,000 m above the crater rim on 23 January. Lapilli up to 2 cm in diameter from recent explosions were found in Kurokami (3.5 km E) and Arimura (3 km S) during JMA field visits on 16 and 30 January.

Figure 50. An ash emission at Sakurajima on 20 January 2015 was captured by a webcam in Kagoshima (10 km W). Courtesy of Volcano Discovery.

The number of explosions increased to 88 during February 2015, with events on 21 and 22 February sending tephra 1.8 km from the crater. Plumes rose as much as 3,500 m above the rim during the month. During a field survey on 4 March scientists observed ash deposits with fragments up to 2 cm in diameter, in an area 3 km S of Showa Crater. JMA reported that the largest number of explosions they have recorded in a month, 178, occurred at the crater in March. Numerous plumes rose 3,300 m above the crater. A small pyroclastic flow on 17 March traveled 600 m SE.

Seismicity below the island increased briefly between 31 March and 2 April 2015. An explosion on 17 April sent tephra 1.8 km from the crater rim. Two pyroclastic flows were reported on 18 and 28 April 2015; Showa crater had 112 explosions throughout the month. The pyroclastic flow on 28 April travelled 500 m down the SE flank. The highest ash plume rose 4,000 m on 24 April. JMA calculated that about 1.2 million tons of ash fell during April, the largest monthly amount recorded since 2006.

Several of the 169 explosions at the Showa crater during May 2015 produced ejecta that was deposited up to 1.8 km from the crater. Many explosions had plume heights exceeding 3,000 m. A small emission, rising 200 m, was observed from the Minamidaki crater on 12 May and was the first in several months. JMA scientists observed 2-cm-diameter tephra in the vicinity of Kurojin-cho, Kagoshima-shi on 14 May, likely from an explosion the previous day; significant ashfall covered the ground as well. The highest ash plume of the month rose 4,300 m above the Showa crater on 21 May 2015 (figures 51 and 52).

Figure 51. An ash plume rose 4,300 m above Sakurajima on 21 May 2015, shown in this webcam image from Kagoshima. Courtesy of Volcano Discovery.

Figure 52. A dense plume of ash drifted S and E from Sakurajima on 21 May 2015. This natural-color satellite image was taken by the Operational Land Imager on Landsat 8. Courtesy of NASA Earth Observatory.

Activity during June-December 2015. Five of the 64 explosions recorded during June produced ejecta that landed up to 1.3 km from the Showa Crater (figure 53). A 3,300-m-high ash plume on 1 June was the highest for the month. After three explosions on 4 June, a small pyroclastic flow traveled 400 m down the E flank. A second small event on 22 June at Minamidake produced a gray plume that rose 200 m.

Figure 53. Ash rose from Showa Crater at Sakurajima on 9 June 2015. Image taken by a drone managed by Naoto Yoshitome and Krishima Aerial Photography. Courtesy of Naoto Yoshitome, Twitter.

Activity decreased significantly beginning in July 2015, with 14 explosions reported from the Showa Crater, and declined further during August with only 5 explosions. A small explosion from the Minamidake crater on 16 July sent emissions likely containing ash (described as "non-white") to 200 m. A rapid increase in seismicity directly beneath Minamidake began on 15 August and lasted about 48 hours; along with tiltmeter and strainmeter observations of rapid inflation (figure 54), this led JMA to briefly raise the Alert Level from 3 (Do not approach the volcano) to 4 (Prepare to evacuate) an a scale of 1-5. They lowered it back to 3 on 1 September 2015. Only small explosions with tephra ejected up to 800 m were recorded during the rest of the August. Minor emissions occurred at Minamidake Crater on 30 August.

Figure 54. An interference image of Sakurajima using PALSAR-2 high-resolution mode (3 m resolution) data comparing displacement between 4 January and 16 August 2015. The data showed a displacement toward the satellite (inflation) of about 16 cm maximum (within the white square), on the E side of the Minamidake summit crater. The synthetic aperture radar (PALSAR - 2) equipped with Daichi 2 (Land Observing Satellite No. 2 "Daichi 2" (ALOS- 2)) can measure the displacement of the ground surface (how much the ground moved) by taking the difference between two sets of observation data. Such an analysis method is called interference SAR analysis (or interferometry, InSAR). The color changes represent the differences in the two observations, a pattern of green to red to blue indicates movement of the surface towards the satellite (inflation); a pattern of green to blue to red indicates movement away from the satellite (deflation). Courtesy of JAXA (http://www.eorc.jaxa.jp/ALOS-2/img_up/jpal2_sakurajima_20150816-17.htm).

Incandescence at the Showa Crater was observed several times during September 2015; 46 explosive events were reported. The first significant explosions at the Minamidake summit crater since 7 November 2014 occurred on 13 and 28 September. The 28 September plume rose to 2,700 m above the crater rim. Tiltmeter data indicated no additional inflation since the rapid ground deformation of 15-16 August. The last explosive event of 2015 reported by JMA at the Showa crater was on 17 September and at the Minamidaki crater on 29 September.

The Tokyo VAAC reported an ash emission on 14 October 2015 that rose to 1.8 km and drifted SW. This was the last VAAC report until 5 February 2016. No explosions were recorded at the Showa crater in October, but minor ash emissions were reported on 14, 15, 21, 22, and 30 October. No activity was observed at Minamidake. Data from continuous GNSS (Global Navigation Satellite System) observations suggested that deflation began after the 15 August rapid inflation event.

A minor emission was reported by JMA from the Showa crater on 2 November 2015, the last emission reported for the year. After not having explosive activity since late September, JMA lowered the Alert Level to 2 (Do not approach the crater) on 25 November, reducing the exclusion area to 1 km around the two craters. Only steam plumes rising 50-200 m above the Showa crater and 50-600 m above the Minamidake crater were observed during December 2015.

Aerial observation on 2 December 2015 revealed 100-m-high steam plumes around the floor of the Showa crater. Thermal observations showed high heat flow around the edges and at the center of the crater floor, unchanged since the previous observation in August 2015; 200-m-high steam plumes around the Minamidake crater prevented observation of the crater floor.

Activity during 2016. No explosive activity was observed at Showa or Minamidake craters from October 2015 to 5 February 2016. JMA raised the Alert Level back to 3 after a substantial explosion on 5 February sent incandescent tephra up to 1.8 km from the Showa crater; lightning was observed in the ash cloud (figure 55). The Tokyo VAAC reported that an ash plume visible in satellite imagery was at 3 km altitude drifting SE. Multiple explosions continued from the Showa crater for the rest of February with ash plumes rising to 2.2 km above the crater, and tephra was frequently ejected 1.3 km from the crater. Four MODVOLC thermal alerts in February were the only alerts for 2016. At the Minamidake summit crater, minor emissions occurred on 8, 9, and 20 February with plumes rising 800 m above the crater rim.

Figure 55. Incandescent tephra explodes from Showa crater at Sakurajima on 5 February 2016 after three months of inactivity. Photo by Kyoto News/AP. Courtesy of the Washington Post.

Eight explosions at the Showa crater were reported by JMA, and six at the Minamidake summit crater during March 2016. Ash plumes at Minamidake on 4, 8, and 11 March rose 1,600-1,900 m above the crater rim; on 25 and 26 March they rose 2,000 m. Minor emissions were also noted on 14 and 15 March. Three explosions from the Showa Crater on 26 March sent ash plumes 2,700 m high (figure 56); tephra as large as 8 mm in diameter was found in areas 4 km E.

Figure 56. Multiple explosions on 26 March 2016 at Sakurajima sent tephra as large as 8 mm in diameter as far as 4 km from Minamidake crater. Image taken from a drone managed by Naoto Yoshidome. Courtesy of Naoto Yoshidome, Twitter.

Activity increased during April 2016 with 51 emission events that included 15 explosions at Showa, and JMA reported inflation again after several months of stability. Reports of falling tephra, 2 cm in diameter, came from a town 3 km S after explosions were witnessed during 1-3 April. On 1 April, an explosion at Minamidake summit crater produced an ash plume which rose 800 m above its crater rim; another on 3 April rose 1,700 m. Minor emissions also occurred at Minamidake on 5, 6, and 9 April. Explosions on 6 and 8 April at Showa sent ash plumes 3,500-3,700 m high and tephra 1.3 km. During the 8 April explosion at Showa, a small pyroclastic flow traveled 400 m down the E flank, the first since June 2015. A 2,200-m-high ash plume rose from Showa crater on 17 April. Minor emissions that rose 800 m were detected at Minamidake on 20 and 28 April. Two explosions occurred on 27 April at Showa, followed by additional explosions on 28, 29, and 30 April; the events generated ash plumes that rose 3,000 m. Pyroclastic flows were generated during the events of 28 and 30 April; they each flowed about 500 m, SE and E, respectively.

A large explosion at the Showa crater on 1 May sent an ash plume to 4,100 m above the crater rim (figure 57). It was the first time since 21 May 2015 that a plume rose higher than 4,000 m. At the Minamidake summit crater, ash emissions on 1 and 13 May rose 3,500 and 3,700 m, respectively, the first plumes at Minamidake over 3,000 m since October 2009. An explosion on 8 May at Showa sent an ash plume over 3,300 m above the crater rim, and tephra reached 1,300 m from the crater. Numerous ash emissions continued throughout the month, some with plumes rising to 3,500 m. The Tokyo VAAC issued 26 reports between 13 and 22 May. Activity diminished toward the end of the month, but minor inflation continued.

Figure 57. An explosive eruption at Sakurajima's Showa Crater on 1 May 2016 sent an ash plume 4,100 m above the crater that drifted SE. It was the highest plume in the last year. Taken with the "Cattle Root" webcam, courtesy of JMA (May 2016 Monthly Sakurajima report).

Multiple ash emissions in early June 2016 produced plumes as high as 2,000 m above the Showa crater rim. An explosion on 3 June produced a pyroclastic flow that traveled 400 m SE, and tephra that was ejected 800 m from the crater. An emission at the Minamidake crater on 3 June rose 1,500m high. No further explosive activity was reported for June; only a minor emission from the Showa crater on 29 June. During the month, the Tokyo VAAC issued only six reports (during 2-3 June).

Two explosive events were recorded at Showa crater in July 2016. An explosion occurred on 2 July that produced a 1,200-m-high ash plume and sent large blocks 800 m from the crater. A substantial explosion on 26 July at Showa sent blocks 800 m from the crater, and produced an ash plume that rose 5,000 m. A minor amount of ashfall on the W and SW flanks of Sakurajima was observed, and ashfall was confirmed in a wide area from Kagoshima City (10 km W) to Hioki City (25 km NW). The Tokyo VAAC reported an ash plume drifting SW at 6.1 km altitude that day.

Minor emissions were observed at the Minamidake crater intermittently throughout August 2016, but no emissions or explosions were reported from Showa. The Tokyo VAAC reported a low-level ash plume on 22 August at 1.2 km altitude drifting 50 km SW (figure 58). This was the last VAAC report for 2016. Although there were no emissions or explosive activity reported from either crater during September-December 2016, inflation of the volcano continued, and thus the Alert Level remained at 3.

Figure 58. An ash emission rose from Sakurajima's Minamidake crater on the morning of 22 August 2016. This was the last reported ash emission of 2016. Taken from the Tarumizu City MBC (Minaminihon Broadcasting Co., Ltd.) webcam no. 14, located about 14 km E. Courtesy of Minaminihon Broadcasting Co., Ltd. (http://www.mbc.co.jp/web-cam/).

Geologic Background. The Aira caldera in the northern half of Kagoshima Bay contains the post-caldera Sakurajima volcano, one of Japan's most active. Eruption of the voluminous Ito pyroclastic flow accompanied formation of the 17 x 23 km caldera about 22,000 years ago. The smaller Wakamiko caldera was formed during the early Holocene in the NE corner of the caldera, along with several post-caldera cones. The construction of Sakurajima began about 13,000 years ago on the southern rim and built an island that was joined to the Osumi Peninsula during the major explosive and effusive eruption of 1914. Activity at the Kitadake summit cone ended about 4,850 years ago, after which eruptions took place at Minamidake. Frequent eruptions since the 8th century have deposited ash on the city of Kagoshima, located across Kagoshima Bay only 8 km from the summit. The largest recorded eruption took place during 1471-76.

Information Contacts: Japan Meteorological Agency (JMA), Otemachi, 1-3-4, Chiyoda-ku Tokyo 100-8122, Japan (URL: http://www.jma.go.jp/jma/indexe.html); Tokyo Volcanic Ash Advisory Center (VAAC), 1-3-4 Otemachi, Chiyoda-ku, Tokyo, Japan (URL: http://ds.data.jma.go.jp/svd/vaac/data/); 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/); NASA Earth Observatory, EOS Project Science Office, NASA Goddard Space Flight Center, Goddard, Maryland, USA (URL: http://earthobservatory.nasa.gov/); Japan Aerospace Exploration Agency (JAXA) (URL: http://global.jaxa.jp/); Associated Press (URL: http://www.ap.org/); Tom Pfeiffer, Volcano Discovery (URL: http://www.volcanodiscovery.com/ ); Naoto Yoshidome, Twitter (URL: https://twitter.com); Minaminihon Broadcasting Co., Ltd (MBC). (http://www.mbc.co.jp/web-cam/).

Ambae (formerly called Aoba) is a large basaltic shield volcano in the New Hebrides arc that has generated periodic phreatic and pyroclastic explosions originating in the summit crater lakes Manaro Lakua and Voui during the last 25 years; the central edifice with the active summit craters is also commonly referred to as Lombenben, Manaro Voui, or simply the Manaro volcano. From late November 2005 to mid-February 2006 explosions from Lake Voui resulted in the formation of a pyroclastic cone in the lake. By late November 2006 the side of the cone was breached, and its central crater filled with lake water (figure 30, BGVN 31:12). The Vanuatu Meteorology and Geo-Hazards Department (VMGD) reported intermittent increases in degassing activity between 2006 and August 2017, and minor ash emissions during June-July 2011 and August 2016. An explosive eruption from a new pyroclastic cone in the lake began in mid-September 2017 and lasted through mid-November. This report summarizes activity between 2010 and the new eruption in September 2017 and provides details for the eruption through December 2017, with information provided primarily by the Vanuatu Geohazards Observatory of VMGD, the Wellington Volcanic Ash Advisory Center (VAAC), and satellite data from several sources.

Local ashfall around the pyroclastic cone in Lake Voui during June-July 2011 and August 2016 were the only eruptive events between February 2006 and September 2017, although intermittent SO₂ emissions were noted throughout the period. Renewed explosive activity was reported beginning on 6 September 2017. Lava was first observed on 22 September emerging from a vent at the summit of the pyroclastic cone. Ash plumes and fountaining lava persisted for a few weeks as the pyroclastic cone increased in size. Activity became more intermittent by mid-October, but explosions still produced ash plumes; the highest was reported at 9.1 km altitude. Pulses of thermal activity suggesting lava flows continued through early November. The last ash emission of the year was reported on 23 November 2017, after which only steam and gas were noted.

Activity during 2010-August 2017. After several years of quiet since early 2006, substantial gas plumes were observed beginning in December 2009 and the Volcanic Alert Level was raised to 1 (on a 0-5 scale). Plumes of gas emissions were observed during 6-11 April 2010, and steam emissions were photographed during 3-4 June 2010 (figure 32).

Figure 32. Steam plumes rose from the crater of the pyroclastic cone in Lake Voui at Ambae on 4 June 2010. Courtesy of Vanuatu Meteorology and Geo-Hazards Department (VMGD) (Vanuatu Volcanic Activity Bulletin No. 1-Ambae activity, Monday, July 11th, 2011).

Sulfur dioxide emissions were often elevated, and plumes were identified multiple times with satellite instruments during 2011 (figure 33). Local ashfall around the crater of the pyroclastic cone in Lake Voui was reported after explosions and seismicity on 4 June 2011; additional explosions occurred on 10 July 2011. Compared to January 2010, the cone was significantly eroded when photographed on 12 July 2011.

Figure 33. SO2 plumes from Ambae and Ambrym volcanoes during 2011. SO2 plumes drifted W from both Ambae (N) and Ambrym (S) on 19 April 2011 (left). The SO2 plume from Ambae is small but also distinct from the much larger plume from Ambrym on 30 October 2011 (right). It is often difficult to distinguish between the two sources of the SO2. Courtesy of NASA Goddard Space Flight Center.

While no ash emissions or explosions were reported during 2012 from Ambae, SO₂ plumes were recorded by satellite instruments every month except June and August (figure 34). Villagers in Ambanga reported a "phase of minor activity" beginning in December 2012. Increased SO₂ plumes were recorded in satellite data during December as well (figure 35). Nearby Ambrym often produces large SO₂ plumes which obscure SO₂ emissions from Ambae.

Figure 34. SO2 plumes were recorded every month of 2012 except June and August. Plumes emerging from Ambae are often difficult to distinguish from larger plumes released from Ambrym, located 100 km S. Data from the OMI instrument on the Aura satellite on both 9 January and 5 April (top images) showed SO2 emissions from three volcanos in the New Hebrides arc; from N to S, Gaua, Ambae, and Ambrym. Plumes from both Ambae and Ambrym drifted SE on 21 September (lower left), and smaller plumes drifted W from both Ambrym and Ambae on 3 November (lower right). Courtesy of NASA Goddard Space Flight Center.

Figure 35. Increased gas emissions from Ambae were reported by nearby residents in Ambanga during December 2012. More frequent SO2 emissions were also recorded by the OMI satellite instrument including on 1 (top left), 12 (top right), 17 (bottom left), and 21 (bottom right) December 2012. Courtesy of NASA, Goddard Space Flight Center.

Site observations during 30 January-2 February 2013 confirmed continuing degassing at Lake Voui, and remnants of the old pyroclastic cone still visible in the lake. The Aura satellite instrument detected SO₂ emissions a number of times throughout 2013-2016 (figure 36), and VMGD noted continuing unrest multiple times during 2015.

Figure 36. Selected SO2 emissions during 2013-2016 at Ambae. SO2 emissions drifted W from both Ambae (N) and Ambrym (S) on 13 February 2013 (top left). A rare image of an SO2 plume from Ambae with no plume from Ambrym was recorded on 5 May 2014 (top right). SO2 emissions were also distinct from each volcano on 10 November 2015 (bottom left) and 28 December 2016 (bottom right). Courtesy of NASA Goddard Space Flight Center.

VMGD reported that during 18-19 August 2016 a steam plume was accompanied by a small ash emission in the caldera area. The Vanuatu Volcanic Alert Level (VVAL) was raised from 1 to 2 on 21 August 2016 and remained there for just over a year. Changing conditions were first reported by VMGD on 30 August 2017.

Activity during September-December 2017. The Alert Level was raised to 3 on 6 September 2017, indicating that a minor eruption was occurring. A week later VMGD reminded residents of the 3 km danger zone around the lake and added a 1 km exclusion zone within that area (figure 37). Explosive activity began building a new pyroclastic cone in Lake Voui, and ash plumes generated local ashfall on the island.

Figure 37. "Safety Map" showing hazard zones in the summit area of Ambae, consisting of a Danger Zone A (red oval line) around the summit caldera and a 1-km-radius Exclusion Zone around Manaro Voui. Courtesy of VMGD (Vanuatu Volcano Alert Bulletin No 10-Ambae Activity, Friday September 15th 2017).

On 22 September 2017, lava was observed at the surface by VMGD staff, there was a MODVOLC thermal alert, and a volcanic ash advisory was issued by the Wellington VAAC. The VAAC report estimated the ash plume observed in satellite data to be at an altitude of 3 km drifting E. On 23 September the VMGD stated that activity had continued to increase, prompting them to raise the VVAL to 4, indicating that a moderate eruption was taking place. They warned that ejecta and gas would affect an area within 6.5 km of Lake Voui, and many communities were at risk from various types of volcanic activity (figure 38). A dense plume of dark ash was photographed on 23 September by airplane travelers going to Ambae (figure 39).

Figure 38. Volcanic hazard map for Ambae. On 23 September 2017, VMGD raised the alert level to 4 and warned that ejecta and gas would likely affect an area within 6.5 km of Lake Voui (pink zone). Villages located in the gray and orange areas of the map could see ashfall and other hazards such as lahars and pyroclastic flows. The lighter area outlined with a dashed border indicates where villages would be more susceptible to ashfall and acid rain based on the general wind direction. Courtesy of VMGD (Vanuatu Volcano Alert Bulletin No. 11 - Ambae Activity, Saturday, September 23rd, 2017).

Figure 39. Ash emission photographed on 23 September 2017 from an airplane going to Ambae. Courtesy of Batik Bong Shem, Facebook.

Eruptive activity increased over the next few days. Larger explosions generated ash plumes that caused local ashfall. A photo taken on 24 September showed incandescent ejections and an ash plume rising from the pyroclastic cone (figure 40). The Wellington VAAC reported intermittent emissions that day at 2.4 km altitude drifting N, and again on 26 September at 2.1 km altitude drifting W. The New Zealand Defense Force conducted an overflight on 25 September 2017 and witnessed incandescence at the summit and lava flowing into the lake (figures 41, 42, and 43).

Figure 40. An eruption from the pyroclastic cone in Lake Voui at Ambae on 24 September 2017. Courtesy of Yumi Toktok Stret News, Facebook.

Figure 41. The New Zealand Defence Force (NZDF) aerial survey on 25 September 2017 showed large columns of gas, ash, and volcanic rocks emerging from Lake Voui on Ambae. Courtesy of NZDF.

Figure 42. Lava flows into Lake Voui at Ambae, causing steam plumes. Incandescence is visible at the cone's summit through the clouds. The photo was likely taken on 25 or 26 September 2017. Posted by Geoff Reid NZ on Facebook on 2 October 2017.

Figure 43. Incandescent lava from the crater of the Lake Voui cone was photographed at Ambae on 25 September 2017. Image courtesy of Reuters, reported by BBC.

A 27 September a news article from ABC.net stated that about 8,000 residents had been evacuated from the northern and southern parts of the island to eastern and western areas. An overflight by the New Zealand Defence Force showed ongoing activity. Multiple MODVOLC thermal alerts were issued nearly every day from 22 September through 7 October.

Photographs and thermal infrared images taken by VMGD during observation flights on 30 September and 1 October 2017 showed explosions of tephra, and lava flowing from small vents into the lake (figures 44-48). The number of vents on the cone varied from 2 to 4 during the observation flights.

Figure 44. Aerial view of the pyroclastic cone that formed in Lake Voui during September in the Ambae summit caldera. The active lava-producing vents are near the center of the island. The blue steaming zone is a lava flow. The white steaming to the right is lava entering the lake. Photo taken on 30 September 2017. Courtesy of VMGB, posted on Facebook 2 October 2017.

Figure 45. The pyroclastic cone in Lake Voui at the summit of Ambae had active steam, ash, and gas emissions, in addition to lava flowing into the lake, on 1 October 2017. Courtesy of VMGD.

Figure 46. Aerial view of the cone that formed in Lake Voui during September 2017 in the summit caldera of Ambae. The Manaro Lakua lake can be seen in the background. The active vents are near the center of the island. The white steaming zone at the far end of the island was caused by lava flows entering the lake. Photo taken on 1 October 2017. Courtesy of VMGB, posted on Facebook 2 October 2017.

Figure 47. Infrared aerial view of the volcanic cone that has formed in Lake Voui during September 2017 near the summit of Ambae Island. The active lava producing vents are the hottest areas near the center of the island (inwhite). The white streak in the foreground is a lava flow. The red areas in the foreground are areas where lava recently entered the lake. The caldera rim at the summit of Ambae is visible in the background. Photo taken on 1 October 2017. Courtesy of VMGB, posted on Facebook, 2 October 2017.

Figure 48. Closeup view of a lava flow from the cone entering into Lake Voui at Ambae on 1 October 2017. Courtesy of VMGB, posted on Facebook 2 October 2017.

On 6 October 2017, the VMGD noted that there was no evidence of the eruption escalating; the Alert Level was lowered to 3 and residents and tourists were reminded to stay outside of the Red Zone, defined as a 3 km radius around the active cone. The Wellington VAAC reported ash emissions on 9 October visible in satellite imagery spreading N of the island as high as 3.7 km altitude. They reported low-level (2.4-4.6 km) ash plumes daily through 15 October. A short-lived eruption on 13 October produced an ash plume clearly visible in satellite imagery that rose to 9.1 km altitude.

Webcam observations and seismic analysis reported on 13 October by VMGD indicated ongoing minor explosive activity and ash emission from vents on the cone in Lake Voui over the previous several days (figure 49). Lava had apparently ceased flowing to the lake. The local population from Ambae and neighboring islands could still hear some of the explosions, see volcanic ash and gas plumes, and see incandescence at night. Multiple MODVOLC thermal alerts were issued on 15 and 16 October, and again during 19-23 October. Wellington VAAC reports during 22-23 October indicated intermittent low-level ash plumes at 2.4-3.7 km altitude moving E.

Figure 49. An ash plume rises over Ambae island on 12 October 2017 in this photo taken from Santo - Pekoa Airport 65 km W on Espiritu Santo Island. Photo by Steve Clegg, courtesy of VMGD (posted on their Facebook page).

A new surge of activity created multiple MODVOLC thermal alerts between 27 October and 1 November 2017. The Wellington VAAC reported an ash plume on 29 October at 6.1 km altitude drifting SE. The activity ceased, and the plume dissipated by the end of the day. VMGD reported on 31 October that seismic activity was ongoing, and explosions could be seen in webcam photos; incandescence and explosions were also heard and seen from neighboring islands at night.

Webcam photos from 5 and 6 November showed that ash emissions and incandescent explosions continued (figures 50 and 51). The Wellington VAAC reported an ash emission rising to 4.3 km altitude and drifting W on 5 November. By the next day the altitude of the ash plume had dropped to 2.1 km. This was followed late on 6 November by an ash emission reported at 3.9 km altitude extending 25 km W and SW of the volcano, which continued through the next day. Another emission on 8 November drifted W at 3 km altitude for several hours before dissipating. Fourteen MODVOLC thermal alerts were issued on 5 November, and two more the next day. A final alert on 9 November was the last for 2017.

Figure 50. Webcam images of Ambae indicate that ash emissions and incandescent explosions were continuing on 5 November 2017. Image taken from the Saratamata webcam located 22 km NE on the NE tip of Ambae Island. Courtesy of VMGD, posted on Facebook 5 November 2017.

Figure 51. Steam and ash emissions were visible from the Saratamata webcam (22 km NE) in the early morning of 6 November 2017. Courtesy of VMGD, posted on Facebook 5 November 2017 (UTC).

VGO reported on 8 November 2017 that the eruption had been continuing, and photos taken during the first week of the month confirmed that the pyroclastic cone in Lake Voui continued to grow in height and size, with frequent explosions and ash plumes. The Wellington VAAC reported a ground observation of an ongoing minor eruption on 21 November that produced an ash plume that rose to 1.8 km altitude. By the following day, the plume appeared to be mostly steam. A new eruption the next day (23 November) produced a plume estimated at 3.7 km altitude moving W. An ash emission later that day was estimated at 3 km altitude drifting N based on satellite imagery. It had dissipated by the following day, and there were no further VAAC reports issued during 2017.

By 7 December 2017, activity had decreased significantly, and emissions consisted of only steam and gas plumes; VMGD lowered the Alert Level from 3 to 2, and reduced the restricted area to within 2 km of the active vent in Lake Voui, noting that the eruption had ceased. The MIROVA plot of Log Radiative Power at Ambae (Aoba) correlates well with visual and thermal observations of activity between 23 September and early November 2017 (figure 52). Significant quantities of SO₂ were released at Ambae during October-December 2017 (figure 53). SO₂ emissions continued into December after the ash emissions ceased.

Figure 52. The MIROVA plot of Log Radiative Power at Ambae (Aoba) for the year ending on 29 December 2017 correlates well with visual and thermal observations of activity between 23 September and early November 2017. Courtesy of MIROVA.

Figure 53. Significant quantities of SO2 were released from Ambae during October-December 2017. Variable wind directions seem to create complex patterns of SO2 plumes. Emissions on 23 and 28 October (top), 8, 13, and 17 November (middle row and bottom left) all show plumes that appear to be mostly sourced from Ambae, but some component of source from Ambrym is also likely. By 31 December 2017 (bottom right) SO2 emissions at Ambae were still significant even though no ash emissions had been reported for over a month. Courtesy of NASA Goddard Space Flight Center.

Geologic Background. The island of Ambae, also known as Aoba, is a massive 2,500 km3 basaltic shield that is the most voluminous volcano of the New Hebrides archipelago. A pronounced NE-SW-trending rift zone with numerous scoria cones gives the 16 x 38 km island an elongated form. A broad pyroclastic cone containing three crater lakes (Manaro Ngoru, Voui, and Manaro Lakua) is located at the summit within the youngest of at least two nested calderas, the largest of which is 6 km in diameter. That large central edifice is also called Manaro Voui or Lombenben volcano. Post-caldera explosive eruptions formed the summit craters about 360 years ago. A tuff cone was constructed within Lake Voui (or Vui) about 60 years later. The latest known flank eruption, about 300 years ago, destroyed the population of the Nduindui area near the western coast.

Information Contacts: Geo-Hazards Division, Vanuatu Meteorology and Geo-Hazards Department, Ministry of Climate Change Adaptation, Meteorology, Geo-Hazards, Energy, Environment and Disaster Management, Private Mail Bag 9054, Lini Highway, Port Vila, Vanuatu (URL: http://www.vmgd.gov.vu/, https://www.facebook.com/VanuatuGeohazardsObservatory/); 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/); Wellington Volcanic Ash Advisory Centre (VAAC), Meteorological Service of New Zealand Ltd (MetService), PO Box 722, Wellington, New Zealand (URL: http://www.metservice.com/vaac/, http://www.ssd.noaa.gov/VAAC/OTH/NZ/messages.html); NASA Goddard Space Flight Center (NASA/GSFC), Global Sulfur Dioxide Monitoring Page, Atmospheric Chemistry and Dynamics Laboratory, 8800 Greenbelt Road, Goddard, Maryland, USA (URL: https://so2.gsfc.nasa.gov/); New Zealand Defence Force (URL: http://www.nzdf.mil.nz/); BBC News (URL: http://www.bbc.com/news); ABC News (http://abcnews.go.com/); Batik Bong Shem, Facebook (URL: https://www.facebook.com/batick.shem); Yumi Toktok Stret News, Facebook URL: https://www.facebook.com/ytsnews.today/); Geoff Reid NZ, Facebook (URL: https://www.facebook.com/GeoffReidNZ/).

Occasional weak eruptions and low-level ash emissions are typical of activity at Ambrym. The most recent ash emission was on 3 April 2017 (BGVN 42:05). The current report summarizes activity from late April through December 2017.

On 30 August 2017, the Vanuatu Meteorology and Geo-Hazards Department (VMGD) reported that "drastic changes" at Ambrym prompted an increase in the Alert Level from 2 to 3 (on a scale of 0-5). Areas deemed hazardous were near and around the active vents (Benbow, Maben-Mbwelesu, Niri-Mbwelesu and Mbwelesu), and in downwind areas prone to ashfall. According to a news report (Radio New Zealand), a representative of VMGD indicated that the Alert Level change was based on increased seismicity detected since the beginning of August, but which became more notable on 25 August.

According to VMGD, aerial observations on 24 and 30 September, and 1 and 6 October, combined with analysis of seismic data, confirmed that minor eruptive activity within the caldera was characterized by hot volcanic gas and steam emissions. Areas deemed hazardous were within a 2-km radius from Benbow Crater and a 3-km radius from Marum Crater.

A news report (The Vanuatu Independent) quoted an official from VMGD as stating that on 8 November 2017 at 0500, the Niri-Mbwelesu eruptive vent emitted a minor ash plume. On 7 December 2017, VGO lowered the Alert Level to 2, noting that activity had stabilized by the end of November and was characterized by gas-and-steam emissions. Seismicity had also declined. The report reminded the public to stay outside of the Permanent Danger Zone, defined as a 1-km radius from Benbow Crater and a 2.7-km radius from Marum Crater.

During the reporting period, thermal anomalies based on MODIS satellite instruments and analyzed using the MODVOLC algorithm, continued to be numerous every month, possibly reflecting lava lakes in Benbow and Marum craters. The MIROVA (Middle InfraRed Observation of Volcanic Activity) system also detected numerous hotspots every month within 5 km of the volcano.

Geologic Background. Ambrym, a large basaltic volcano with a 12-km-wide caldera, is one of the most active volcanoes of the New Hebrides Arc. A thick, almost exclusively pyroclastic sequence, initially dacitic then basaltic, overlies lava flows of a pre-caldera shield volcano. The caldera was formed during a major Plinian eruption with dacitic pyroclastic flows about 1,900 years ago. Post-caldera eruptions, primarily from Marum and Benbow cones, have partially filled the caldera floor and produced lava flows that ponded on the floor or overflowed through gaps in the caldera rim. Post-caldera eruptions have also formed a series of scoria cones and maars along a fissure system oriented ENE-WSW. Eruptions have apparently occurred almost yearly during historical time from cones within the caldera or from flank vents. However, from 1850 to 1950, reporting was mostly limited to extra-caldera eruptions that would have affected local populations.

Information Contacts: Geo-Hazards Division, Vanuatu Meteorology and Geo-Hazards Department, Ministry of Climate Change Adaptation, Meteorology, Geo-Hazards, Energy, Environment and Disaster Management, Private Mail Bag 9054, Lini Highway, Port Vila, Vanuatu (URL: http://www.vmgd.gov.vu/, https://www.facebook.com/VanuatuGeohazardsObservatory/); Radio New Zealand (URL: https://www.radionz.co.nz); The Vanuatu Independent (URL: https://vanuatuindependent.com/); 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/); Middle InfraRed Observation of Volcanic Activity (MIROVA), Mirova (collaborative project between the Universities of Turin and Florence, Italy)(URL: http://www.mirovaweb.it).

Eruptions at Fernandina Island in the Galapagos often occur from vents located around the caldera rim along boundary faults and fissures, and occasionally from side vents on the flank. The last eruption in 2009 generated fountaining basaltic lava along several fissure vents. Lava flowed down the SW flank and entered the sea for a few weeks during April 2009. A new eruption began on 4 September 2017 after eight years of no surface activity, and lasted for about one week. Information about this new eruption was provided by Ecuador's Institudo Geofisica, Escuela Politécnica Nacional (IG-EPN), the Dirección del Parque Nacional Galápagos (DPNG), the Washington Volcanic Ash Advisory Center (VAAC), and several sources of satellite data.

A brief fissure vent eruption began on 4 September 2017 at Fernandina, located at the SW rim of the caldera. Small amounts of ash were noted in the plume that rose 2.5 km, but most of the emission was steam and SO₂. Vegetation fires were ignited on the SW flank, but lava did not reach the ocean. There was no sign of volcanic activity within the summit crater. A significant area with thermal anomalies was seen in infrared satellite data through 7 September.

Eruption of early September 2017. After eight years of little activity, Fernandina (La Cumbre) began a new eruptive phase on 4 September 2017, at approximately 1225 (Galápagos time) (figure 22). Inflation between March 2015 and September 2017 was 17 cm centered on the caldera; 5 cm of that inflation occurred in the last two months before the eruption (figure 23).

Figure 22. Fernandina began a new eruption on 4 September 2017. The initial plume was mostly steam, but contained significant SO2 and possibly minor ash. Photo by DPNG personnel, courtesy of IG-EPN (INFORME ESPECIAL VOLCÁN FERNANDINA N°1 – 2017, Lunes, 04 Septiembre 2017 16:49).

Figure 23. Interferogram image of Fernandina between 19 March 2015 and 4 September 2017 shows about 17 cm of inflation in the caldera. Each concentric band of colors within the caldera represents several centimeters of inflation. Created by Yu Zhou and Mike Stock, courtesy of IG-EPN (INFORME ESPECIAL DEL VOLCÁN FERNANDINA N°2 – 2017, Miércoles, 06 Septiembre 2017 17:16).

Seismic activity began with hybrid-type earthquakes (fractures with fluid movements) followed by Long Period (LP) earthquakes (fluid movements). The seismic network of the Geophysical Institute installed in the Galapagos began to detect activity at the volcano around 0955 on 4 September 2017. The beginning of the eruption was associated with a volcanic tremor that began at 1225. At 1428, an eruptive column was visible in satellite imagery, interpreted at an approximate height of 4,000 m above the crater, drifting WNW (figure 24).

Figure 24. This false-color satellite image of Fernandina on 4 September 2017 showed the eruption column drifting NW estimated at 4,000 m altitude. Source: http://goes.higp.hawaii.edu/cgi-bin/imageview?sitename=galapagos. Courtesy of IG-EPN (INFORME ESPECIAL VOLCÁN FERNANDINA N°1 – 2017, Lunes, 04 Septiembre 2017 16:49).

The Washington VAAC reported that satellite imagery indicated a lava eruption which produced a plume of steam and gas that rose to 2,400 m above sea level and extended about 60 km W of the summit. While initially no ash was reported in the plume, a few hours later a new VAAC report suggested that minor ash was possibly present, although it was most likely primarily SO₂. Satellite data reported by the NASA Goddard Space Flight Center showed SO₂ emissions on 4-6 and 8 September (figure 25).

Figure 25. SO2 emissions from Fernandina were identified with the OMI instrument on the Aura satellite and the OMPS instrument on Japan's Suomi satellite during 4-8 September 2017. Upper left: A small SO2 emission emerges very close in time to the first reported observation of the eruption on 4 September. Upper right: The low-resolution OMPS image clearly shows a large plume drifting W about 24 hours later. Lower left and right: SO2 is present NW of the Galapagos over the eastern Pacific on 6 and 8 September. Courtesy of NASA Goddard Space Flight Center.

Thermal alerts indicative of fresh lava flows from the rim of the summit crater were first reported by MODVOLC on 4 September 2017 (UTC), and abundant through 7 September (figure 26). No thermal anomalies were recorded in MODVOLC data on 8 September. An additional group of alert pixels was recorded on 9 September, but it's not clear if they were caused by fresh lava flows or burning fires; a few more intermittent pixels were recorded through 20 September. The MIROVA system also captured a significant spike in heatflow at Fernandina during the same period (figure 27). Some of the anomalies measured by both systems were likely the result of the fires caused by the lava flows as well as the flows themselves.

Figure 26. Map showing the location of new lava flows at Fernandina during 4-7 September 2017 using MODVOLC thermal alerts. Fires may have caused some of the alert pixels. Courtesy of HIGP MODVOLC Thermal Alerts System.

Figure 27. MIROVA thermal anomalies show a spike in activity at Fernandina during the period of the September 2017 eruption in this graph of log radiative power for the year ending on 16 October 2017. The initial spike that was located more than 5 km from the summit confirms the lava flows were located on the crater rim and flank and not in the summit crater. Some anomalies may also be due to the fires caused by the lava flows. Courtesy of MIROVA.

Incandescence was first observed during the night of 4 September (figure 28). Lava flows apparently originated from a circumferential fissure near the fissure of the 2005 eruption on the SSW rim of the caldera. The lava flowed down the S and SW flanks but did not reach the sea. Active lava flows were observed during the night of 5 September (figure 29). The intensity of the eruption decreased significantly after about 48 hours.

Figure 28. Incandescence at Fernandina on 4 September 2017. Photo by Alex Medina, courtesy of IG-EPN (INFORME ESPECIAL DEL VOLCÁN FERNANDINA N°2 – 2017, Miércoles, 06 Septiembre 2017 17:16).

Figure 29. A lava flow is visible on the SW flank of Fernandina on 5 September 2017. Photo by Alex Medina, courtesy of IG-EPN (INFORME ESPECIAL DEL VOLCÁN FERNANDINA N°2 – 2017, Miércoles, 06 Septiembre 2017 17:16).

A technical team from the Directorate of the Galapagos National Park (DPNG) made an aerial inspection using the seaplane Sea Wolf on 7 September 2017. They observed a radial fissure in the same area where the 2005 eruption occurred, and several lava flows. No recent volcanic activity or any landslides were seen inside the caldera. The lava flows had ceased movement, but there were isolated fires burning patches of vegetation surrounded by older lava flows (figures 30 and 31). The lava had traveled from the summit crater at about 1,200 m down to 500 m elevation. While lava was not observed flowing into the sea, coastal monitoring by the park rangers showed water vapor on the SW coast, so it was possible that lava had reached the ocean through subsurface lava tubes.

Figure 30. Lava flows burn vegetation on Fernandina during the eruption of September 2017. Observers on a 7 September 2017 flyover by DPNG reported that the active flows had ceased, but vegetation was burning at four different sites. Courtesy of Directorate of the Galapagos National Park (DPNG) (11/09/2017– Sobrevuelo al volcán La Cumbre, en Galápagos).

Figure 31. Vegetation on Fernandina burns on 7 September 2017 after lava flows erupted beginning on 4 September 2017. There was no evidence of flowing lava during the overflight. Courtesy of the Galapagos Conservancy.

Geologic Background. Fernandina, the most active of Galápagos volcanoes and the one closest to the Galápagos mantle plume, is a basaltic shield volcano with a deep 5 x 6.5 km summit caldera. The volcano displays the classic "overturned soup bowl" profile of Galápagos shield volcanoes. Its caldera is elongated in a NW-SE direction and formed during several episodes of collapse. Circumferential fissures surround the caldera and were instrumental in growth of the volcano. Reporting has been poor in this uninhabited western end of the archipelago, and even a 1981 eruption was not witnessed at the time. In 1968 the caldera floor dropped 350 m following a major explosive eruption. Subsequent eruptions, mostly from vents located on or near the caldera boundary faults, have produced lava flows inside the caldera as well as those in 1995 that reached the coast from a SW-flank vent. Collapse of a nearly 1 km3 section of the east caldera wall during an eruption in 1988 produced a debris-avalanche deposit that covered much of the caldera floor and absorbed the caldera lake.

Information Contacts: Instituto Geofísico (IG-EPN), Escuela Politécnica Nacional, Casilla 17-01-2759, Quito, Ecuador (URL: http://www.igepn.edu.ec ); Dirección del Parque Nacional Galápagos (DPNG), Isla Santa Cruz, Galápagos, Ecuador (URL: http://www.galapagos.gob.ec/); 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/); NASA Goddard Space Flight Center (NASA/GSFC), Global Sulfur Dioxide Monitoring Page, Atmospheric Chemistry and Dynamics Laboratory, 8800 Greenbelt Road, Goddard, Maryland, USA (URL: http://so2.gsfc.nasa.gov/index.html ); Galapagos Conservancy, (URL:https://www.galapagos.org).

Guatemala's Volcán de Fuego was continuously active throughout 2017, and has been erupting vigorously since 2002; historical observations of eruptions date back to 1531. These eruptions have resulted in major ashfalls, pyroclastic flows, lava flows, and damaging lahars. Reports of activity are provided by the Instituto Nacional de Sismologia, Vulcanología, Meteorología e Hidrologia (INSIVUMEH), and aviation alerts of ash plumes are issued by the Washington Volcanic Ash Advisory Center (VAAC). Satellite data from NASA, NOAA, and other sources provide valuable information about heat flow and gas emissions.

Activity remained high at Fuego throughout July-December 2017. Background levels of activity included frequent explosions (4-6 per hour) with incandescent material rising 150 m above the summit and sending blocks 200 m down the flanks. Block avalanches commonly traveled down the major ravines for hundreds of meters. Ash plumes regularly rose 500-1,000 m above the summit (4.3-4.8 km altitude); ashfall affected communities SW of the summit within 15 km every week. During the multiple short-lived (48-hour or less) eruptive episodes, the hourly explosion rates increased significantly (6-12 per hour), and incandescent material often rose 300 m above the summit; one or more lava flows would also travel more than a kilometer down major ravines. Higher ash plumes (often rising to 5-6 km altitude) during the eruptive episodes sent ash plumes drifting hundreds of kilometers in various directions causing ashfall in cities tens of kilometers away in various directions. Pyroclastic flows often accompanied the eruptive episodes. Seven episodes were reported by INSIVUMEH during July-December 2017 (table 17); they are clearly discernible as periods of higher heat flow in the MIROVA thermal anomaly data (figure 73) as well.

Table 17. Eruptive episodes at Fuego during July-December 2017. Information provided primarily by INSIVUMEH. Some ash plume information is from the Washington VAAC.

Figure 73. MIROVA thermal anomaly data for Fuego for 2017 shows the continuing activity that included intermittent pulses of high-heat-flow from twelve defined eruptive episodes shown by red arrows. Courtesy of MIROVA. Eruptive episodes defined by INSIVUMEH.

Activity during July 2017. Activity increased at Fuego during July 2017, compared with the previous month. INSIVUMEH reported that explosions per hour increased during 6-7 July from 4-7 to 7-10; a lava flow also traveled 1.5 km down Las Lajas ravine. Incandescent material was ejected 100-200 m above the crater rim and caused avalanches of material that traveled down the Ceniza (SSW), Taniluyá (SW), Santa Teresa (SW), and Trinidad (S) drainages (figure 74). Ash plumes during 7-9 July caused ashfall in Santa Sofía (12 km SW), Morelia (9 km SW), Panimaché I and II (8 km SW), El Porvenir (8 km ENE), Sangre de Cristo (8 km WSW), and possibly San Pedro Yepocapa (8 km N).

Figure 74. Incandescent material was ejected over a hundred meters above the summit of Fuego and blocks of material traveled hundreds of meters down the flank on 9 July 2017. Courtesy of INSIVUMEH and OVFGO (Reporte Semanal de Monitoreo: Volcán Fuego (1402-09), Semana del 08 al 14de julio 2017).

The Washington VAAC reported dense ash emissions seen in satellite data on 10 July extending WNW 60 km from the summit at 4.6 km altitude. They noted that ashfall was reported 10 km SW from the summit the following morning. The 6th eruptive episode of the year occurred on 11-12 July 2017. Explosions generated ash plumes that rose as high as 1.3 km above the crater and drifted 35 km W, and shock waves rattled nearby structures. Ash fell in areas to the SW. Two lava flows were fed by lava fountains 150-250 m high; one flow traveled 2.3 km down the Las Lajas drainage and another traveled 1.7 km down the Santa Teresa (SW) drainage. The increased activity levels lasted for about 31 hours, with tens of explosions. Weak-to-moderate explosions continued afterwards, generating ash plumes that rose 850 m and drifted 6 km W.

Multiple explosions continued generating ash plumes and block avalanches during 13-14 July. On 16 July, a 30-m-wide, 2-m-deep, hot lahar descended tributaries of the Pantaleón (W) drainage, carrying blocks more than 2 m in diameter, branches, and tree trunks. The lahars again overtook the road between communities on the SW flank, isolating the village of Sangre de Cristo (8 km WSW) and the Palo Verde estate. The Washington VAAC estimated that the ash plumes released early on 16 July rose to 5.2 km altitude, and drifted SE from the summit. By afternoon they had risen to 5.8 km and were drifting SW, extending about 75 km. Explosions during 17-18 July produced dense ash plumes that drifted 15 km W and NW causing ashfall in Panimache, Morelia, and Santa Sofía. Satellite imagery on 19 July showed an ash plume extending 65 km WNW of the summit in a narrow band at 4.3 km altitude. Similar plumes were reported daily between 19-23 July at 4.3-4.9 km altitude drifting generally W up to about 50 km before dissipating (figure 75).

Figure 75. Ash emissions were reported almost daily from Fuego during July 2017. A small pulse of ash on 20 July was captured on the Panimaché I webcam (10 km SW) in this view looking NE in the early morning. Courtesy of OVFGO-INSIVUMEH (Reporte Semanal de Monitoreo: Volcán Fuego (1402-09), Semana del 15 al 21 de julio 2017).

Activity during August 2017. MODVOLC thermal alerts that were issued on 28 and 30 July confirmed the continuing incandescent summit activity which produced block avalanches down the major drainages. Multiple daily alerts were also issued during 15 days of August. Coordinadora Nacional Para la Reduccion de Desastres (CONRED) reported increased activity on 4 August that included 300-m-high ejections of incandescent material and a lava flow that traveled 600 m down the Ceniza ravine. During 7-8 August two lava fountains rose 150 m high, prompting INSIVUMEH to announce the seventh effusive episode at Fuego in 2017. The fountains fed lava flows, 1.5 km and 700 m long, in the Ceniza and the Santa Teresa ravines (figure 76). Explosions (occurring at a rate of 6-8 per hour) produced ash plumes that drifted 20 km W, causing ashfall in Panimache, Morelia, Santa Sofía, El Porvenir, and Yepocapa. The Washington VAAC also noted increasing ash emissions on 7 August. Weather clouds prevented observations from satellite images on 7 and 8 August, but the VAAC reported a "" strong hotspot in infrared imagery on 8 August. Although the lava flow in the Ceniza drainage remained active, explosive activity decreased to an average of three explosions per hour the following week, with ash emissions rising to 4.4-4.6 km and drifting 10 or more km W and SW, bringing ashfall to communities on the W and SW flank.

Figure 76. A lava flow at Fuego during eruptive episode 7 descends the SE flank on 7 August 2017. Courtesy of OVFGO-INSIVUMEH (Reporte Semanal de Monitoreo:, Volcán Fuego (1402-09), Semana del 5 al 11 de agosto 2017).

Activity intensified again during 19-20 August, when constant explosions generated ash plumes that rose 2.3 km above the crater and drifted more than 50 km W and SW. INSIVUMEH reported that the eighth effusive episode at Fuego in 2017 began on 20 August and lasted for about 48 hours. Two lava fountains, each 300 m high, fed lava flows that traveled 1.4 km SSW down the Ceniza ravine and 1.2 km W down the Seca (Santa Teresa) ravine (figure 77). Incandescent block avalanches occurred throughout the crater. Pyroclastic flows (figure 78) were concentrated in the Santa Teresa ravine, possibly filling the drainage with deposits (similar to activity from 5 May) and increasing the chances for lahars. A bright hotspot was visible in satellite imagery from 19-21 August. Seismicity remained elevated through 21 August. During 21 August, the Washington VAAC reported the ash plume near 5.5 km altitude extending 75 km WNW. A remnant cloud of ash was detected in satellite imagery over 200 km WNW of the summit in extreme SE Mexico late on 21 August.

Figure 77. Incandescent explosions and block avalanches descend the SE flank of Fuego during eruptive episode 8, 19-21 August 2017 in this view from the Panimaché I webcam. Courtesy of OVGFO-INSIVUMEH (Reporte Semanal de Monitoreo: Volcán de Fuego (1402-09), Semana del 19 al 25 de agosto 2017).

Figure 78. A pyroclastic flow descends the Santa Teresa ravine at Fuego during eruptive episode 8 on 21 August 2017 in this view from the Panimaché I webcam. Courtesy of OVGFO-INSIVUMEH (Reporte Semanal de Monitoreo: Volcán de Fuego (1402-09), Semana del 19 al 25 de agosto 2017).

INSIVUMEH reported that on 25 August multiple lahars descended the Pantaleón, Cenizas, El Jute, and Las Lajas drainages on Fuego's W, SSW, and SE flanks. The lahar in the Pantaleón river (fed by the Santa Teresa and El Mineral rivers) was 35 m wide, 2.5-3 m deep, and carried trees and blocks more than 2-3 m in diameter. The Cenizas lahar was about 25 m wide, 3 m deep, and carried blocks up to 2 m in diameter. The lahars in El Jute and Las Lajas drainages were 20 m wide, 1.5 m deep, and carried tree debris and blocks up to 2 m in diameter.

Explosions during 26-29 August generated ash plumes that rose as high as 950 m above the crater and drifted 7-12 km SW, W, and NW. The Washington VAAC reported near continuous emissions of ash on 28 August moving WSW and extending about 100 km at 4.6 km altitude, rising to 5.8 km altitude the following day. Incandescent material was ejected 100-200 m above the crater rim and caused avalanches of material around the crater area. Explosions were audible within a 20-km radius, and shock waves vibrated local structures. Ash fell in areas downwind including Panimache I and II, Morelia, Finca Palo verde, Sangre de Cristo, and El Porvenir. On 29 August, lahars 10 m wide and 1.5 m deep again descended the Santa Teresa and El Mineral drainages, carrying tree debris and blocks up to 2 m in diameter.

Activity during September 2017. Lahars were reported in the Santa Teresa and El Mineral drainages intermittently during September. Ash emissions continued to cause ashfall in communities within 10 km W and SW throughout the month. Continuous ejection of incandescent blocks rose 200-300 m above the crater and sent material 300 m down the flanks. The Washington VAAC reported a continuous plume of ash detected in satellite imagery and in the webcam extending about 95 km WSW on 8 September at 4.6 km altitude. INISVUMEH reported that the increase in activity during 8 September fed a lava flow that traveled 800 m down Barranca Seca.

The ninth eruptive episode of 2017 began late on 12 September and lasted about 35 hours (figure 79). Pyroclastic flows descended the Seca (Santa Teresa) ravine on the W flank, along with a lava flow that traveled 1.3 km during the episode. Ashfall was reported in Morelia, Palo Verde Estate, Sangre de Cristo, El Porvenir, Santa Sofía, and Panimaché I and II. The Washington VAAC reported that an ash plume extended about 65 km N from the summit on 13 September at 4.6 km altitude. After several days of weather clouds obscuring the satellite images, they reported a plume drifting W on 17 September extending 95 km from the summit. A hotspot intermittently appeared during 13-17 September.

Figure 79. Incandescent lava rises 200-300 m above the summit of Fuego, and a lava flow traveled down the Santa Theresa ravine on the W flank during eruptive episode 9 on 12 September 2017. View from Panimaché I webcam. Courtesy of OVFGO-INSIVUMEH (Reporte Semanal de Monitoreo: Volcán de Fuego (1402-09), Semana del 09 al 15 de septiembre 2017.

The Washington VAAC reported weak puffs of ash drifting N and quickly dissipating on 25 September, and another ash plume extending 15 km W on 28 September at 4.6 km. Hotspots were also observed both days in satellite images. INSIVUMEH reported eruptive episode 10 during 27-28 September, lasting about 40 hours. The ash plume generated during the episode drifted in multiple directions simultaneously (figure 80) and resulted in ashfall more than 30 km from the crater, primarily N and NE, in La Soledad (7 km N), Pastores (20 km NNE), San Miguel Dueñas (10 km NE) and Antigua Guatemala (20 km NE). The incandescent material reached 300 meters above the crater and fed two lava flows, the first went 300 m down the Seca Canyon, and the second traveled 500 m down Las Lajas Canyon.

Figure 80. The ash plumes drift in multiple directions (W, NW, SW and S) from the summit of Fuego on 28 September 2017 during eruptive episode 10. Image taken in San Pedro Yepocapa, 8 km NW. Courtesy of INSIVUMEH (Reporte Semanal de Monitoreo: Volcán de Fuego (1402-09), Semana del 23 al 29 de septiembre 2017).

Seven lahars were recorded during September in the main ravines of Fuego, on days 3, 4, 5, 6, 8, 27, and 29, as a result of the unusually large amount of rainfall during the month (1,059 mm) (figure 81). The larger ones at the beginning of the month contained blocks up to 3 m in diameter, and many were warm enough to generate steam with strong odors of SO₂. Several roads were damaged.

Figure 81. High rainfall (1,059 mm) during September 2017 generated large lahars in the Seca, Mineral, Taniluya, Ceniza, Trinidad, Las Lahas, El Jute, and Honda ravines at Fuego, shown in purple. Many dirt roads (shown in red) were damaged. Courtesy of INSIVUMEH (VOLCÁN DE FUEGO, INFORME MENSUAL, Septiembre 2017).

Activity during October 2017. Overall activity was quieter during October 2017. Background levels of activity included incandescent material rising up to 250 m above the summit and falling a similar distance down the flanks, and ash plumes rising to 4.4-5.0 km altitude and drifting more than 25 km W, NW, and E. Eight to twelve explosions per hour were not uncommon, although 4-6 per hour were more typical. A few of the block avalanches traveled 2 km down the flanks. The communities that experienced persistent ashfall were all located 10-20 km SW, and included Morelia, Palo Verde Farm, Sangre de Cristo, El Porvenir, Santa Sofía, and Panimaché I and II. Due to the wind conditions and increased activity during the first week of October, ashfall was also reported farther away in Guatemala City (40 km NE), Antigua Guatemala, Villa Nueva (30 km ENE) and San Miguel Petapa (35 km ENE). INSIVUMEH reported three increases in explosive activity during the month on 2, 3, and 5 October, but they did not develop into eruptive episodes.

Four lahars were reported on 1, 2, and 4 October in the Seca and Mineral drainages. They carried blocks of volcanic rocks and debris as large as 3 m in diameter and were 6-12 m wide and 1-2 m deep. The Washington VAAC reported a series of explosions on 4 October, after which ash emissions were seen in multispectral imagery at 5.2 km altitude drifting SW that reached as far as 75 km. They reported occasional puffs of ash on 15 October extending up to 95 km W of the summit. By 17 October, imagery showed continuous emissions with an ash plume extending 95 km SSW from the summit before dissipating. A possible ash plume was reported by the Washington VAAC on 31 October extending 45 km W from the summit at 4.3 km altitude.

Activity during November 2017. There were numerous periods of intermittent ash emissions during November. Continuous emissions often drifted 65-100 km or more SW or W at altitudes around 4.6-5.2 km during periods of activity. INSIVUMEH reported that during 2-3 November tremor at Fuego increased. Explosions during the first week averaged 5-8 per hour and ash plumes rose as high as 1.3 km above the crater. Incandescent material was ejected 300 m above the crater, causing avalanches that were confined to the crater. The 11th eruptive episode in 2017 began on 5 November and lasted for two days. Lava flowed 1-1.2 km W down the Seca drainage and 800 m SSW down the Ceniza drainage. Avalanches of material from the ends of the lava flows descended the flanks and reached vegetated areas.

Ashfall was reported in areas downwind in the communities 8-12 km SW including Morelia, Santa Sofia, Palo Verde Farm, and Panimaché I and II throughout the month. Shockwaves from explosions often rattled windows and roofs around the volcano. Avalanche blocks were reported in the Cenizas, Trinidad, Taniluyá and Seca canyons. Multiple VAAC reports were issued on 25 days of November, and multiple daily MODVOLC thermal alerts were issued on 20 days of the month. On 10 November the emissions extended about 275 km WSW from the summit. A lahar during the third week descended the Seca and el Mineral drainages.

Activity during December 2017. Explosions averaged 4-8 per hour during most of December sending incandescent material 200-250 m above the crater. INSIVUMEH reported that the 12th eruptive episode at Fuego in 2017 began on 10 December and, based on seismicity, lasted for about 36 hours. Ash plumes from moderate-to-strong explosions rose as high as 1.2 km above the crater rim and drifted 20 km S and SW. Lava flowed as far as 1.5 km W down the Seca (Santa Teresa), SW down the Taniluyá, and SSW down the Ceniza ravines. Ash fell many times in the communities of La Rochela, San Andrés Osuna, Morelia, and Panimaché I and II. On 12 December there was an average of 10 explosions per hour, generating avalanches in the Ceniza and Taniluyá drainages and ashfall in nearby areas. Ashfall was also reported in San Miguel Dueñas, Alotenango, and Ciudad Vieja (13.5 km NE) on 14 December.

Multiple MODVOLC thermal alerts appeared on 20 days during December, and the Washington VAAC issued 91 reports of continuous or intermittent ash plume activity. During eruptive episode 12 on 11 December, they reported an intense hot spot seen at the crater in satellite imagery despite meteoric cloud cover. For most of the second half of December, either continuous or intermittent ash emissions drifted 100-150 km WNW from the summit before dissipating. The Washington VAAC reported an ash emission on 20 December drifting WNW at 5.8 km altitude that extended over 300 km from the summit. A remnant of the plume was observed almost 450 km away late on 20 December before dissipating. Plumes were repeatedly observed over 200 km from the summit during 20-25 December.

Geologic Background. Volcán Fuego, one of Central America's most active volcanoes, is also one of three large stratovolcanoes overlooking Guatemala's former capital, Antigua. The scarp of an older edifice, Meseta, lies between Fuego and Acatenango to the north. Construction of Meseta dates back to about 230,000 years and continued until the late Pleistocene or early Holocene. Collapse of Meseta may have produced the massive Escuintla debris-avalanche deposit, which extends about 50 km onto the Pacific coastal plain. Growth of the modern Fuego volcano followed, continuing the southward migration of volcanism that began at the mostly andesitic Acatenango. Eruptions at Fuego have become more mafic with time, and most historical activity has produced basaltic rocks. Frequent vigorous historical eruptions have been recorded since the onset of the Spanish era in 1524, and have produced major ashfalls, along with occasional pyroclastic flows and lava flows.

Information Contacts: Coordinadora Nacional para la Reducción de Desastres (CONRED), Av. Hincapié 21-72, Zona 13, Guatemala City, Guatemala (URL: http://conred.gob.gt/www/index.php ); Instituto Nacional de Sismologia, Vulcanologia, Meteorologia e Hydrologia (INSIVUMEH), Unit of Volcanology, Geologic Department of Investigation and Services, 7a Av. 14-57, Zona 13, Guatemala City, Guatemala (URL: http://www.insivumeh.gob.gt/ ); 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/).

An eruption at Sheveluch has been ongoing since 1999, and volcanic activity was previously described through August 2017 (BGVN 42:08). Ongoing activity consists of pyroclastic flows, explosions, and lava dome growth with a viscous lava flow in the N. Strong fumarole activity, ash explosions, hot avalanches and incandescence from the dome accompany this process. Explosions and ash flows were reported by Kamchatka Volcanic Eruption Response Team (KVERT) during the August 2017 through January 2018 period.

During this report period the Aviation Color Code (ACC) remained at Orange (the second highest level on a four-color scale), except for 10 January 2018 when it was briefly elevated to Red (highest level) and lowered back to Orange later the same day. Satellite infrared data also showed increased activity on this day. Ash plume altitudes ranged from a low of 5 km to a high of 11 km on 10 January 2018. The farthest lateral extent of the ash plume was reported at 990 km to the NE on 8 November 2017.

On 4 and 8 August 2017 large ash clouds reached altitudes of 6.5 km and approximately 10 km, respectively. Ashfall was reported in Klyuchi Village (50 km SW) on 8 August and drifted about 180 km E, NW, and NE during 12 and 15-16 August. On 7 September ash plumes rose to 8-10 km altitude and drifted NE, SE, and S; another ash plume was photographed on 8 September (figure 47). On 15-22 September ash plumes rose to 9-10 km altitude and drifted about 400 km NW, E, and SE. Explosions on 10 October generated ash plumes to 10 km altitude and drifted about 250 km N (figure 48). Plumes comprised of re-suspended ash drifted about 350 km SE on 12 October and about 230 km SE on 13 October.

Figure 47. Photo of an ash cloud from Sheveluch generated by an explosion on 8 September 2017. Photo by G. Teplitsky; courtesy of the Institute of Volcanology and Seismology FEB RAS, KVERT.

Figure 48. Explosions from Sheveluch sent ash up to 10 km altitude on 10 October 2017. Photo from a webcam, courtesy of the Institute of Volcanology and Seismology FEB RAS, KVERT.

Explosions on 2 and 8 November generated ash plumes that rose to an altitude of 8 km and drifted approximately 990 km NE. Weather prevented observations on the other days from 4-10, 12-17, and 19-24 November. A strong explosive event on 5 December generated ash plumes that rose to altitudes of 10.5 km and 5 km and drifted NE and E, respectively. Explosions on 26 December generated an ash plume that rose to an altitude of 8 km and drifted about 300 km NE.

On 10 January 2018 satellite images captured an ash cloud with a dimension of 192 x 132 km drifting 230 km NE from explosions rising to altitudes of 10-11 km. In response, KVERT raised the ACC to Red. Later that same day, satellite images showed the ash cloud expanded to 350 x 180 km in dimension and had drifted 400 km E; the ACC was lowered back to Orange. The 10 January explosions began at 1035 with resulting ash that drifted about 900 km E during 10-11 January.

Thermal anomalies. As reported by KVERT, satellite imagery continue to detect the existence of a thermal anomaly over Sheveluch. The anomaly was reported on 10-30 days every month from August 2017 through January 2018. Detections of the thermal anomaly were lower in certain months because cloudy conditions obscured satellite imagery. The MIROVA system detected numerous hotspots every month during August 2017-January 2018, most of which were about 5 km or less from the summit with mainly low to a few high power signatures in August, September 2017 and January 2018. Thermal anomalies based on MODIS satellite instruments analyzed using the MODVOLC algorithm were detected in 11-12 August 2017 and 10 January 2018 corresponding to the explosive eruptions on those days.

Geologic Background. The high, isolated massif of Sheveluch volcano (also spelled Shiveluch) rises above the lowlands NNE of the Kliuchevskaya volcano group. The 1,300 km3 andesitic volcano is one of Kamchatka's largest and most active volcanic structures, with at least 60 large eruptions during the Holocene. The summit of roughly 65,000-year-old Stary Shiveluch is truncated by a broad 9-km-wide late-Pleistocene caldera breached to the south. Many lava domes occur on its outer flanks. The Molodoy Shiveluch lava dome complex was constructed during the Holocene within the large open caldera; Holocene lava dome extrusion also took place on the flanks of Stary Shiveluch. Widespread tephra layers from these eruptions have provided valuable time markers for dating volcanic events in Kamchatka. Frequent collapses of dome complexes, most recently in 1964, have produced debris avalanches whose deposits cover much of the floor of the breached caldera.

Information Contacts: Kamchatka Volcanic Eruptions Response Team (KVERT), Far East Division, Russian Academy of Sciences, 9 Piip Blvd., Petropavlovsk-Kamchatsky, 683006, Russia (URL: http://www.kscnet.ru/ivs/kvert/); Institute of Volcanology and Seismology, Far Eastern Branch, Russian Academy of Sciences (IVS FEB RAS), 9 Piip Blvd., Petropavlovsk-Kamchatsky 683006, Russia (URL: http://www.kscnet.ru/ivs/eng/); 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/).

Confirmed historical eruptions at Italy's Stromboli volcano go back 2,000 years as this island volcano in the Tyrrhenian Sea has been a natural beacon for eons with its near-constant fountains of lava. Eruptive activity at the summit consistently occurs from multiple vents at both a north crater area (N Area) and a southern crater group (S or CS Area) on the Terrazza Craterica at the head of the Sciara del Fuoco, a large scarp that runs from the summit down the NW side of the island (figures 102 and 103). Thermal and visual cameras placed on the nearby Pizzo Sopra La Fossa monitor activity at the Terrazza Craterica. Eruptive activity continued at low to moderate levels during 2015 and 2016, with intermittent periods of frequent explosions from both crater areas that sent ash, lapilli, and bombs across the Terrazza Craterica and onto the head of the Sciara del Fuoco (BGVN 42:07).

Figure 102. A view of Stromboli looking SW with the Sciara del Fuoco on the NW flank on the right. Image taken during 10-12 June 2017. Copyrighted photo by Martin Rietze, used with permission.

Figure 103. A view to the NW of the Terrazza Craterica from the summit of Stromboli shows the CS Area (left) and N Area (right) vents during 10-12 June 2017. Copyrighted photo by Martin Rietze, used with permission.

This report covers activity from January-October 2017. Activity similar to 2016 continued through March 2017 when an increase began in explosion rates. The increase peaked during June and then declined through August, returning to background levels in September (figures 104). Thermal energy increased beginning in early May and lasted through mid-August (figure 105). Multiple MODVOLC thermal alerts were issued for Stromboli between 4 May and 25 August 2017. Weekly reports of activity were provided by the Instituto Nazionale de Geofisica e Vulcanologia (INGV), Sezione de Catania, which monitors the gas geochemistry, deformation, and seismology, as well as the surficial activity.

Figure 104. Increased rates of explosive activity at Stromboli were recorded between early April and late August 2017, peaking during mid-June. Rates declined to background levels by early September. The green line represents the number of daily explosions from the S Area, the red line is the number of daily explosions from the N Area, and the blue line is the cumulative of the two areas. Graph includes activity from 28 March-30 October 2017. Courtesy of INGV (Rep. 44/2017, Bollettino settimanale sul monitoraggio vulcanico, geochimico, delle deformazioni del suolo e sismico del vulcano Stromboli del 31/10/2017).

Figure 105. After a lengthy period of low to intermittent thermal activity during 2015 and 2016, a distinct increase in thermal energy was recorded in satellite thermal imagery and is shown in the MIROVA system data for the year ending on 25 August 2017. Courtesy of MIROVA.

Activity during January 2017 consisted of low to moderate intensity explosions from the southern crater area (S Area), and low intensity explosions at the northern crater area (N Area). Two vents in the S Area generated explosive activity. Modest explosions with ash and lapilli occurred regularly from the southernmost vent, and rare explosions were observed from the northernmost vent (figure 106). At the northern crater area (N Area) the southern vent was active, generating ash and lapilli that was ejected a few tens of meters from the vent. There were no explosions from the northern vent in the N Area.

Figure 106. Typical activity at Stromboli's Terrazza Craterica during January 2017 photographed from visible cameras on the Pizzo sopra la Fossa. Left: Explosions at the S Area on 23 January 2017 included moderate activity at the southern vent (yellow arrow) and low activity at the northern vent (white arrow). Right: The southern vent (green arrow) of the N Area showed moderate explosive activity on 17 January 2017. Courtesy of INGV (Rep. 04/2017, Bollettino settimanale sul monitoraggio vulcanico, geochimico, delle deformazioni del suolo e sismico del vulcano Stromboli del 24/01/2017).

There were no notable changes in activity until the second week of February 2017 when explosive activity returned to the northern vent of the N Area. During the third week of February, a gradual increase in the rate and intensity of the explosions at both areas was observed which lasted throughout the rest of the month (figure 107). Coarse pyroclastic material was ejected onto the Terrazza Craterica and occasionally onto the Sciara del Fuoco. The stronger explosions generated modest plumes of dilute ash that quickly dissipated.

Figure 107. Explosive activity at Stromboli during the third week of February 2017: A) The colored arrows indicate the active vents in the S and N Areas as seen by the visible camera of the Pizzo. B) Explosion at the northern vent (blue arrow) of the N area (visible camera). C) Explosion at the southern vent (yellow arrow) of the S area (visible camera). D-F) explosions from the N and S Areas taken by the 400 level Thermal camera. Courtesy of INGV (Rep. 08/2017, Bollettino settimanale sul monitoraggio vulcanico, geochimico, delle deformazioni del suolo e sismico del vulcano Stromboli del 21/02/2017).

During the first week of March 2017, the most active vents were the southernmost vent of the S Area and the northernmost vent of the N Area. The strongest explosions from the northern vent of the N Area produced dilute ash emissions and pyroclastic ejecta that landed on the upper part of the Sciara del Fuoco. By the third week of March, and through the end of the month, most of the activity had shifted to the vents in the N Area and diminished in the S Area. On 28 March, Etna Observatory personnel restored operations at both the infrared and visible cameras on the Pizzo sopra la Fossa which allowed for more detailed observations of the activity at the summit (figure 108).

Figure 108. The Terrazza Craterica at Stromboli seen from the thermal camera on the Pizzo sopra la Fossa on 31 March 2017, showing active vents in the two crater areas (AREA N, AREA CS). The abbreviations and arrows indicate the names and locations of the active vents. Courtesy of INGV (Rep. 14/2017, Bollettino settimanale sul monitoraggio vulcanico, geochimico, delle deformazioni del suolo e sismico del, vulcano Stromboli del 04/04/2017).

Throughout April 2017, the N1 vent produced low (less than 80 m high) to medium (80-150 m) intensity explosions containing ash, lapilli, and bombs. The N2 vent showed sporadic low intensity explosive activity with occasional ash emissions until 20 April when more coarse (lapilli and bombs) material was ejected. Vent C showed continuous degassing throughout the month, and low intensity explosions began there during the third week of April, causing intense spattering on 29 April. The S1 vent showed sporadic and weak explosive activity of low intensity with the ejection of coarse material until the third week when activity ceased. Vent S2 showed explosive activity of medium-low intensity (less than 120 m high) of coarse material sometimes mixed with ash. Explosion rates were around 2-10 events per hour during the first half of the month, rising to 10-15 per hour for the second half of April.

In the N Area, the N1 and N2 vents continued with a similar level of activity throughout May 2017 (figure 109). Explosions of low to medium intensity sent coarse ejecta of lapilli and bombs up to 150 m high at N1 and 120 m high at N2. The rate of explosions in the N Area ranged from 4-12 per hour.

Figure 109. The Terrazza Craterica at Stromboli seen from the thermal camera located on the Pizzo sopra la Fossa on 18 May 2017, showing active vents in the two crater areas (AREA N, AREA CS). The abbreviations and arrows indicate the names and locations of the active vents. The vents in the N Area exhibited similar levels of activity throughout the month. Courtesy of INGV (Rep. 21/2017, Bollettino settimanale sul monitoraggio vulcanico, geochimico, delle deformazioni del suolo e sismico del vulcano Stromboli del 23/05/2017).

In the S Area, activity was more variable during May, and the rate of explosions ranged from 2-10 per hour. Vent C also continued with intense degassing and low-intensity explosions and spattering. On 13 May, two emission points were observed at vent C, one a few meters S of the other. Vent S1 showed no activity until late in the second week of May when low to moderate intensity explosions rose up to 150 m with coarse ejecta. During 14-15 May, a second vent opened a few meters north of S1, and simultaneous explosions from both S1 vents sent jets of gas and incandescent material into the air. Activity decreased to low intensity explosions (less than 80 m high) with ejecta during the third week, but then increased significantly during the last week of the month. Ejecta reached 200 m high from the S1 vents (figure 110). The southern S1 vent built a surrounding hornito and produced high and narrow jets of incandescent material, while the northern emission point produced more modest jets of gas and material. Vent S2 was quiet for most of May, producing only low-intensity explosions of coarse material sometimes mixed with ash for a few days near the beginning of the month.

Figure 110. The Terrazza Craterica at Stromboli seen from the thermal camera on the Pizzo sopra la Fossa on 29 May 2017, showing active vents in the two crater areas (AREA N, AREA CS). The abbreviations and arrows indicate the names and locations of the active vents. The S1 vent in the CS Area produced high intensity jets of incandescent material that rose 200 m during the last week of the month. Courtesy of INGV (Rep. 22/2017, Bollettino settimanale sul monitoraggio vulcanico, geochimico, delle deformazioni del suolo e sismico del vulcano Stromboli del 30/05/2017).

An increase in activity during June 2017 was apparent at both the N and S Areas (figure 111). Video taken by drone and from the summit during 10-12 June shows periodic explosions with ash, lapilli, and bombs ejected around the Terrazza Craterica (See Information Contacts for link). Vent N1 was characterized by low to medium-high intensity explosive activity that ejected lapilli and bombs to 200 m and was sometimes accompanied by ash that drifted S over the island. N2 also showed variable activity which ranged from low to high intensity (ejecta rising over 200 m high) during the first week, and low to medium-high (ejecta rose to 150 m) for the rest of the month (figure 112). Numerous bombs and lapilli were deposited both inside and outside the crater rim. Intense spattering was reported at N2 on 11, 12, 18, 19, and 26 June. The explosion rate in the N Area was 9-18 per hour.

Figure 111. Thermal activity increased during June 2017 at Stromboli. Simultaneous explosions from both the S (left) and N (right) Areas during 10-12 June 2017 were photographed from the summit. Copyrighted photo by Martin Rietze, used with permission.

Figure 112. Increased thermal activity was apparent in the N Area of the Terrazza Craterica at Stromboli as seen from the thermal camera located on the Pizzo sopra la Fossa on 5 June 2017. Courtesy of INGV (Rep. 23/2017, Bollettino settimanale sul monitoraggio vulcanico, geochimico, delle deformazioni del suolo e sismico del vulcano Stromboli del 06/06/2017).

In the CS Area, sporadic low-intensity explosions (less than 80 m high) characterized vent C, with modest spattering reported on 11, 12, 13, 26, 30 June 2017. Activity at S1 continued from two vents simultaneously with low to medium intensity explosive activity (figure 113 and 114). The vent at S2 reactivated briefly on 3 June after about a month of quiet with weak spattering activity but was not active again during the month. The CS Area was characterized by an explosion frequency of 1-10 per hour.

Figure 113. Explosions of incandescent ejecta from the CS Area at Stromboli during 10-12 June 2017. Copyrighted photo by Martin Rietze, used with permission.

Figure 114. Increased activity at the CS Area of Stromboli on 26 June 2017 was recorded by the thermal camera located on the Pizzo sopra la Fossa. Activity at S1 continued from two vents simultaneously with low to medium intensity explosive activity for most of the month. Courtesy of INGV (Rep. 26/2017, Bollettino settimanale sul monitoraggio vulcanico, geochimico, delle deformazioni del suolo e sismico del vulcano Stromboli del 27/06/2017).

During July 2017, thermal activity at the vents remained moderate to high; explosions at the N1 vent sent lapilli and bombs, sometimes mixed with ash, to 200 m above the vent. At vent N2, lapilli and bombs were ejected outside the crater rim, sometimes rolling down the Sciara del Fuoco to the ocean. The hourly frequency of explosions ranged from 5-18. At S1, both vents exploded simultaneously with lapilli, bombs and occasional ash rising to 150 m numerous times.

Beginning in the afternoon of 26 July, an explosive sequence at the CS Area lasting about 90 seconds was recorded with the thermal and visible image cameras on the Pizzo sopra la Fossa (figure 115). It began with explosions from vents C and S1, followed by a second explosion at S2. More explosions from C and S1 sent debris to the SE and were followed by fountaining to about 50 m from the vents for about a minute. INGV personnel witnessed 10-cm-diameter bombs on the SW side of the Pizzo at about 850 m elevation during a 30 July site visit.

Figure 115. The explosive sequence of 26 July 2017 at Stromboli was recorded by the thermal and visible cameras located on the Pizzo sopra la Fossa. Details of the 90-second-long event are described in the text. Courtesy of INGV (Rep. 31/2017, Bollettino settimanale sul monitoraggio vulcanico, geochimico, delle deformazioni del suolo e sismico del vulcano Stromboli del 01/08/2017).

A return to background activity during August consisted of explosions of varying intensity from low (less than 80 m) to medium-low (ejecta sometimes reached 120 m in height) at both the N and CS Area vents. Explosion frequency ranged from 2-11 per hour, decreasing significantly by the end of the month. Activity continued to diminish during September. Periodic spattering from vent C occurred. Only one vent was active in the CS Area during the month. A brief increase in intensity at vent N1 during 8-9 September sent ejecta over 150 m high. By the end of September, few explosions reached over 80 m in height. A brief episode of intense spattering at vent C on 24 September sent bombs and lapilli to 40 m above the vent. Explosion frequency averaged only 2-6 per hour by the end of September.

Continuous spattering, occasionally intense, from vent C continued during October. The vents in the N Area produced low to moderate intensity explosions, and one vent in the CS Area produced low intensity explosions. A strong explosive sequence in the CS Area lasted for about five minutes on 23 October 2017 (figure 116). The first explosion of the sequence came from vent C and lasted 30 seconds. It destroyed the hornito formed around the vent. About a minute later, two explosions occurred at the S1 vent, reaching about 120 m in height and dispersing to the SE. Another explosion at vent C about 3 minutes later sent ejecta 100 m high. The event ended with a series of small ash emissions that rose a few tens of meters. Low intensity activity continued from both areas through the end of October, with low explosion rates of around 2-6 per hour.

Figure 116. An explosive sequence from the CS Area at Stromboli on 23 October 2017 lasted about five minutes. Ejecta from vents C and S1 rose 100-150 m above the vents and dispersed SE. Courtesy of INGV (Rep. 43/2017, Bollettino settimanale sul monitoraggio vulcanico, geochimico, delle deformazioni del suolo e sismico del vulcano Stromboli del 24/10/2017).

Geologic Background. Spectacular incandescent nighttime explosions at Stromboli have long attracted visitors to the "Lighthouse of the Mediterranean" in the NE Aeolian Islands. This volcano has lent its name to the frequent mild explosive activity that has characterized its eruptions throughout much of historical time. The small island is the emergent summit of a volcano that grew in two main eruptive cycles, the last of which formed the western portion of the island. The Neostromboli eruptive period took place between about 13,000 and 5,000 years ago. The active summit vents are located at the head of the Sciara del Fuoco, a prominent scarp that formed about 5,000 years ago due to a series of slope failures which extends to below sea level. The modern volcano has been constructed within this scarp, which funnels pyroclastic ejecta and lava flows to the NW. Essentially continuous mild Strombolian explosions, sometimes accompanied by lava flows, have been recorded for more than a millennium.

Information Contacts: Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione di Catania, Piazza Roma 2, 95123 Catania, Italy, (URL: http://www.ct.ingv.it/en/); 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/); Martin Rietze, Taubenstr. 1, D-82223 Eichenau, Germany (URL: https://mrietze.com/, https://www.youtube.com/channel/UC5LzAA_nyNWEUfpcUFOCpJw/videos, http://mrietze.com/web16/Stromb_Vesuv17.htm).

Remote Tinakula lies 100 km NE of the Solomon Trench at the N end of the Santa Cruz Islands, part of the country of the Solomon Islands, which generally lie 400 km to the W. It has been uninhabited since an eruption with lava flows and ash explosions in 1971 when the small population was evacuated (CSLP 87-71). The nearest inhabitants live on Te Motu (Trevanion) Island (about 30 km S), Nupani (40 km N), and the Reef Islands (60 km E); they occasionally report explosion noises from Tinakula. Ashfall from larger explosions has historically reached these islands. The last reported evidence of activity came from MODVOLC thermal alerts between August 2010 and October 2012, and observations of incandescent lava blocks rolling into the sea in May 2012. A new eruptive episode with a large ash explosion and substantial SO₂ plume during 21-26 October 2017 is reported below, along with newly available historical newspaper accounts of earlier eruptions.

Reports of ash plumes are issued by the Wellington Volcanic Ash Advisory Center (VAAC); the National Disaster Management Office (NDMO) of the Solomon Islands Government also issues situation reports when significant activity is reported. Satellite data from infrared, visual, and SO₂ monitoring instruments are an important source of information for this remote volcano. News reports from local (and social) media are often the only sources of information for the smaller events. Recently identified 19th- and 20th-century newspaper accounts of eruptive activity witnessed by sailors passing nearby is a valuable new resource for previously unreported events.

Eruption of 21-26 October 2017. Reports of a substantial explosion with an ash plume from Tinakula appeared on social media and in the local press during 22-26 October 2017. Staff from the Lata Met Service Office approached the island by boat on 23 October to make direct observations (figures 17-19). A video clip from the Himawari8 Satellite showing the ash plume explosion was posted by Stephan Armbruster on Twitter on 22 October. The Solomon Islands NDMO issued a situation report on 26 October showing ashfall covering vegetation on the island. According to the NDMO, ashfall was concentrated on the island, although a small amount of ash drifted SE and was reported to briefly contaminate drinking water in several communities in the nearby Reef Islands (60 km ENE) . Ashfall was also reported on Fenualoa Island (50 km ENE) (Radio New Zealand). The eruption was categorized by NMDO as a VEI 3. A team of geologists from NDMO brought seismic monitoring equipment to Tinakula in early November, and measured a high frequency volcanic tremor on 5 November 2017.

Figure 17. View from the SE of the eruption at Tinakula on 23 October 2017 during a site visit by staff from the Lata Office of the Solomon Islands Meteorological Service. Photo by Okano Gamara.

Figure 18. Ash and steam emissions rose from Tinakula on 23 October 2017 during a site visit by staff from the Lata Office of the Solomon Islands Meteorological Service. Photo by Okano Gamara.

Figure 19. Ash emission from Tinakula on 23 October 2017 during a site visit by staff from the Lata Office of the Solomon Islands Meteorological Service. Photo by Okano Gamara.

The Wellington VAAC first reported an ash plume visible in satellite imagery shortly after midnight (UTC) on 21 October 2017. The plume was estimated to be at 4.6 km altitude and drifting N. About 90 minutes later they reported a second eruption with a much higher plume drifting SE at 10.7 km altitude using IR imagery cloud top temperatures to estimate the altitude. They reported ongoing ash emissions visible in satellite imagery drifting SE at 6.1 km altitude throughout the morning, dropping to 3 km altitude by the end of the day. The following day, 22 October, intermittent ash emissions were reported at 3.7 km altitude moving E. By that afternoon, they had dropped to 2.4 km, and had lowered to 1.8 km by late on 23 October. Ongoing low-level ash emission (2.1 km altitude) continued through 25 October; by early on 26 October, there was no further evidence of ongoing activity.

No MODVOLC thermal alerts were associated with this event, but there was a brief MIROVA signal from the MODIS infrared data during 20-23 October 2017 (figure 20). A major SO₂ plume was released from Tinakula on 21 October, and a smaller one was recorded on 28 October as well (figure 21).

Figure 20. Moderate thermal signals were recorded from Tinakula on 20 and 23 October 2017 (top graph) by the MIROVA system that captures MODIS infrared satellite data. Another signal reported during the first week of March 2017 (bottom graph) could also have been an eruptive event, but no other corroborating evidence is available. Courtesy of MIROVA.

Figure 21. Major SO2 plumes from Tinakula and the Vanatu volcanoes of Ambae and Ambrym were released during October 2017. A substantial SO2 plume drifted in several directions from Tinakula on 21 October 2017 (left). Much smaller plumes are also visible from Ambae and Ambrym which are located farther south. On 28 October (right), a smaller SO2 plume was drifting SE from Tinakula while much larger plumes were apparent from Ambae and Ambrym. Data gathered by the OMI instrument on the Aura Satellite. Courtesy of NASA Goddard Space Flight Center.

Summary of activity during 1971-2012. After the 1971 eruption, intermittent ash emissions, lava bombs, and pyroclastic flows were reported by geologists and sailors passing nearby in 1984, 1985, 1989-1990, 1995, and 1999. Infrared MODIS thermal data was first reported as MODVOLC thermal alerts beginning in 2000 and has provided satellite-based confirmation of thermal activity since then. Months with thermal activity included February 2000-May 2001, February 2006-November 2007, September-November 2008, August 2009, and January 2010-October 2012 (figure 22). No additional thermal alerts were issued through 2017. Since 2004, SO₂ data has been gathered by satellite instruments and processed by NASA Goddard Space Flight Center; in February and April 2006 small SO₂ plumes were recorded (figure 23).

Figure 22. Months with MODVOLC thermal alerts from MODIS infrared data for Tinakula, during January 2000-December 2017. The orange boxes indicate months where at least one MODVOLC thermal alert was issued; the number of alerts is indicated inside the square. Months highlighted in green represent contiguous periods of time of three months or greater with no recorded MODVOLC thermal alerts. Pale orange squares indicate months with no MODVOLC thermal alerts issued, but within a three-month buffer of an earlier thermal alert. Data courtesy of MODVOLC.

Figure 23. SO2 emission data captured by the OMI instrument on the Aura satellite indicated small plumes from Tinakula (top center of images) on 12 and 14 February 2006 (top) and 21 and 23 April 2006 (bottom). Small plumes were also visible from Ambrym on 12 February, and from Ambae and Ambrym on 14 February and 21 and 23 April 2006. Courtesy of NASA Goddard Space Flight Center.

Eruption reports during 1868-1932. Reports of eruptions at Tinakula between 1868 and 1932 have recently been found in 19th and 20th century newspaper accounts from Australia and New Zealand (table 6). The accounts describe incandescence, water discoloration of the sea, explosions, ash plumes, and lava flows extending from the summit to the ocean.

Table 6. Newly discovered historical newspaper accounts of volcanic activity from ships passing near Tinakula between 1868 and 1932. This is not a full eruptive history for the time period. Online links provided in the References section. Courtesy of Steve Hutcheon.

References. The Age (Melbourne, Victoria) 10 November 1868, page 2b (URL: http://nla.gov.au/nla.news-article177002744).

The Empire (Sydney, NSW) 27 October 1869, page 2a, (URL: http://nla.gov.au/nla.news-article60895166).

The Sydney Morning Herald (NSW) 19 Februay 1872, page 6a (URL: http://nla.gov.au/nla.news-article13252748).

The Daily Telegraph (Sydney, NSW) 1887 20 July, page 4f (URL: http://nla.gov.au/nla.news-article239817295).

The Daily Telegraph (Sydney, NSW) 1 September 1910, page 7a (URL: http://nla.gov.au/nla.news-article237993807; http://nla.gov.au/nla.news-article15183461 ).

The New Zealand Herald (Auckland, NZ) 27 June 1932, page 6a (URL: https://paperspast.natlib.govt.nz/newspapers/NZH19320627.2.19 ).

The Auckland Star (NZ) 10 September 1932, page 1h (Supplement) (URL: https://paperspast.natlib.govt.nz/newspapers/AS19320910.2.180.6 ).

Geologic Background. The small 3.5-km-wide island of Tinakula is the exposed summit of a massive stratovolcano at the NW end of the Santa Cruz islands. It has a breached summit crater that extends from the summit to below sea level. Landslides enlarged this scarp in 1965, creating an embayment on the NW coast. The Mendana cone is located on the SE side. The dominantly andesitic volcano has frequently been observed in eruption since the era of Spanish exploration began in 1595. In about 1840, an explosive eruption apparently produced pyroclastic flows that swept all sides of the island, killing its inhabitants. Recorded eruptions have frequently originated from a cone constructed within the large breached crater. These have left the upper flanks and the steep apron of lava flows and volcaniclastic debris within the breach unvegetated.

Information Contacts: National Disaster Management Office (NDMO), Solomon Islands Government, Prince Philip Highway, Ranadi, Solomon Islands (URL: http://www.ndmo.gov.sb); Wellington Volcanic Ash Advisory Centre (VAAC), Meteorological Service of New Zealand Ltd (MetService), PO Box 722, Wellington, New Zealand (URL: http://www.metservice.com/vaac/, http://www.ssd.noaa.gov/VAAC/OTH/NZ/messages.html); 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/); NASA Goddard Space Flight Center (NASA/GSFC), Global Sulfur Dioxide Monitoring Page, Atmospheric Chemistry and Dynamics Laboratory, 8800 Greenbelt Road, Goddard, Maryland, USA (URL: http://so2.gsfc.nasa.gov/index.html ); Radio New Zealand (URL: http://www.radionz.co.nz/international/pacific-news/342267/solomons-pm-calls-for-calm-in-communities-close-to-volcano); Solomon Islands Broadcasting Corporation, SIBC Voice of the Nation, Honiara, Solomon Islands (URL: http://www.sibconline.com.sb/no-its-not-snow-in-the-solomons-its-ash-from-the-tinakula-volcano/); Andy Prata, AIRES Atmospheric Industrial Research and Environmental Solutions, Melbourne, Australia (URL: https://www.aires.space/, https://twitter.com/andyprata/status/922177129944625157); Gamara Okzman Bencarson, Facebook.

Episodic eruptive activity at Ecuador's Tungurahua has persisted since November 2011. Periods of activity over several weeks that included ash plumes, Strombolian activity, pyroclastic flows, and lava flows were often followed by quiescence for a similar time span. This type of activity continued throughout 2015 (BGVN 42:08, 42:12); Strombolian activity, significant ash emissions, and SO₂ plumes in mid-November 2015 marked the last significant activity for that year. The next episode began in late February 2016 and is discussed below with information provided by the Observatorio del Volcán Tungurahua (OVT) of the Instituto Geofísico (IG-EPN) of Ecuador, aviation alerts from the Washington Volcanic Ash Advisory Center (VAAC), and other sources of satellite data.

The latest eruptive episode at Tungurahua lasted from 26 February-16 March 2016. Multiple explosions with ash plumes that rose 3-8 km were frequent. Incandescent blocks were ejected up to 1,500 m down most flanks. Pyroclastic flows affected many of the ravines, although no communities reported damage. Significant SO₂ emissions were recorded by satellite data between 27 February-8 March. An inflationary trend was recorded from early March through late September 2016, after which a period of deflation began. Tungurahua had occasional seismic swarms after the eruption, but no reported surface activity for the remainder of 2016 and 2017.

IG reported an ash emission on 5 January 2016 that rose 2 km above the crater and drifted NE, causing minor ashfall in the Pondoa and Bilbao sectors. Otherwise, no volcanic activity was reported until a new episode began on 26 February 2016 with a seismic swarm followed by a series of explosions and ash plumes that rose 3-8 km above the crater (figures 96 and 97). Incandescent blocks were ejected up to a kilometer down the NW, W, and SW flanks (figure 98). Pyroclastic flows were also generated that descended through the gorges of Juive, La Hacienda, Mandur and Cusúa, reaching distances of 500-1,500 m (figure 99).

Figure 96. An ash emission at Tungurahua observed from OVT on 26 February 2016. Courtesy of IG-EPN, (Explosion en el Volcan Tunguraha, No. 20 [1], Informe especial Tungurahia No. 1).

Figure 97. Ejecta traveled 1,000 m from the crater, an ash plume rose 2 km, and pyroclastic flows traveled down several drainages on the NW flank at Tungurahua on 26 February 2016 in this thermal image taken from the Mandur camera. Courtesy of OVT, IG-EPN (INFORME No. 836, SÍNTESIS SEMANAL DEL ESTADO DEL VOLCÁN TUNGURAHUA, Semana: Del 23 de febrero al 01 de marzo de 2016).

Figure 98. Incandescent blocks descended 1,000 m down the NW, W, and SW flanks of Tungurahua on 26 February 2016, and explosions were audible at OVT. Photo by F. Vásconez, courtesy of OVT, IG-EPN (INFORME No. 836, SÍNTESIS SEMANAL DEL ESTADO DEL VOLCÁN TUNGURAHUA, Semana: Del 23 de febrero al 01 de marzo de 2016).

Figure 99. Pyroclastic flows descended the Mandur, La Hacienda and other ravines on the W flank of Tungurahua on 26 February 2016 as far as 1 km. Photo by F. Vásconez, courtesy of OVT, IG-EPN (INFORME No. 836, SÍNTESIS SEMANAL DEL ESTADO DEL VOLCÁN TUNGURAHUA, Semana: Del 23 de febrero al 01 de marzo de 2016).

Continuous emissions with low to moderate ash content drifted W and SW on 27 February. The communities most affected by ashfall were Choglontus, Cotaló, El Manzano, Palitahua, Bilbao, Pillate, Juive, Ambato, Tisaleo, Riobamba, and Quero. The ash was mostly fine-grained, except in the area near Pillate and Choglontus, where the grain size reached up to 3 mm and consisted of reddish, black, gray, and beige fragments (figure 100). On the morning of 1 March 2015, several pyroclastic flows were observed descending through the Juive, Mandur, Achupashal, La Hacienda, and Romero ravines; they traveled 1.5-1.7 km (figure 101).

Figure 100. Coarse-grained ash fragments from Tungurahua collected in Ambato on 26 February 2016. Photo by Marco Montesdeoca (ECU911 Ambato), Courtesy of OVT, IG-EPN (Explosion en el Volcan Tunguraha, No. 2, Informe especial Tungurahia No. 2, 26 de febrero del 2016 (16h45)).

Figure 101. A pyroclastic flow descended 1.5 km down the Hacienda Ravine on 1 March 2016 at Tungurahua and was captured by the Mandur thermal camera. Courtesy of OVT, IG-EPN (INFORME No. 836, SÍNTESIS SEMANAL DEL ESTADO DEL VOLCÁN TUNGURAHUA, Semana: Del 23 de febrero al 01 de marzo de 2016).

Ash emissions were constant throughout the first week in March (figures 102 and 103). During 1-5 March they drifted NW, SW and E, with ashfall reported in the towns of Pillate, Manzano, Choglontus, Palictahua and El Altar (figure 104). Incandescent blocks descended most of the flanks (figure 105). Beginning on 6 March, plumes drifted SW and S, with variable ash content. Pyroclastic flows along the W and NW flanks descended the Cusua, Juive, Mandur, Ashupashal, Romero, and Rhea drainages (figure 106), the farthest traveled went 2.2 km down the Ashupashal on 7 March. In addition to ash and other explosive debris, daily sulfur dioxide emissions were identified from 27 February-8 March 2016 by the OMI instrument on the Aura satellite (figure 107).

Figure 102. Constant ash emissions rose at least 1 km above the summit of Tungurahua during the first week of March 2016. Photo take on 3 March 2016 by P. Espin. Courtesy of OVT, IG-EPN (INFORME No. 837, SÍNTESIS SEMANAL DEL ESTADO DEL VOLCÁN TUNGURAHUA, Semana: Del 01 al 08 de marzo de 2016).

Figure 103. A dark ash plume formed a mushroom cloud over Tungurahua on 5 March 2016; it rose 2 km above the summit and drifted SW. Photo by E. Telenchana , courtesy of OVT, IG-EPN (INFORME No. 837, SÍNTESIS SEMANAL DEL ESTADO DEL VOLCÁN TUNGURAHUA, Semana: Del 01 al 08 de marzo de 2016).

Figure 104. Ashfall in Choglontus on 6 March 2016 from Tungurahua. Photo by P. Espín, courtesy of OVT, IG-EPN (INFORME No. 837, SÍNTESIS SEMANAL DEL ESTADO DEL VOLCÁN TUNGURAHUA, Semana: Del 01 al 08 de marzo de 2016).

Figure 105. Strombolian explosions send incandescent blocks down the flanks of Tungurahua on 6 March 2016. Photo by E. Gaunt, courtesy of OVT, IG-EPN (INFORME No. 837, SÍNTESIS SEMANAL DEL ESTADO DEL VOLCÁN TUNGURAHUA, Semana: Del 01 al 08 de marzo de 2016).

Figure 106. Visual (upper) and thermal (lower) images of Tungurahua taken from Cotalo showing a pyroclastic flow extending down the Achupashal drainage on 6 March 2016. Photo by E. Gaunt, thermal image by M. Almeida, courtesy of OVT, IG-EPN (INFORME No. 837, SÍNTESIS SEMANAL DEL ESTADO DEL VOLCÁN TUNGURAHUA, Semana: Del 01 al 08 de marzo de 2016).

Figure 107. Substantial SO2 emissions from Tungurahua were measured daily during 27 February-8 March 2016 by the OMI instrument on the Aura satellite. The plumes drifted 300 km or more W on 27 February, 1, 3, and 5 March. Colombia's Nevado del Riuz (upper plume in images) also produced SO2 emissions during this same period. Courtesy of NASA Goddard Space Flight Center.

Beginning on 28 February, a strong inflationary trend (almost 3 cm) was observed in the GPS data at the Mazón (SW flank) station. Three inclinometers on the NW flank also indicated inflation during 28 February-4 March.

Episodic explosions on 8 March 2016 produced plumes with high ash contents that rose 6 km. Small pyroclastic flows descended the NW flank in the Mandur, Rea, Achupashal, and La Hacienda ravines. Sporadic emissions continued for most of the second week of March, with varying ash contents, reaching between 1.5 and 4 km above the crater and drifting to the SSW. Reports of ashfall were received in the sectors of Choglontús, Manzano, Pillate, El Altar, and Palitahua, and minor ashfall in Juive and Cusúa. Several ash plumes (figure 108) and a small pyroclastic flow were observed on 13 March 2016. The Manzano lookout reported loud noises on 14 March, and ashfall in the afternoon, but weather obscured views of emissions. Rainy weather on 16 March also obscured views, but Manzano, Chacauco, Cusúa, and Juive lookouts reported ashfall and explosions. There were no further reports from the observatory of ash emissions, ashfall, or explosions; only minor steam plumes were observed on clear days after 16 March 2016.

Figure 108. An ash emission at Tungurahua on 13 March 2016 was the last photographed for the eruption. Photo by M. Córdova from OVT, courtesy of IG-EPN (INFORME No. 838, SÍNTESIS SEMANAL DEL ESTADO DEL VOLCÁN TUNGURAHUA, Semana: Del 08 al 15 de marzo de 2016).

The Washington VAAC reported possible ash emissions on 31 March 2016, but information from OVT indicated no surface activity. Intense rain on 28 March generated a small lahar that descended through the La Pampa ravine. Significant rainfall on 2 April caused lahars to affect Vazcun, Juive, Pondoa, Bilbao, Achupashal, Chontapamba and Malpayacu drainages. Seismicity continued to decrease throughout April 2016. A small swarm of Long Period seismic events (LP's) occurred between 1 and 20 May that were associated with fluid movements. The Washington VAAC reported ash emissions on 3, 8, and 13 May, but OVT reported no surface activity during the entire month (figure 109).

Figure 109. Clear skies on 31 May 2016 at Tungurahua revealed a snow-covered summit with no evidence of emissions. Photo by M. Córdova, courtesy of OVT, IG-EPN (INFORME No. 849, SÍNTESIS SEMANAL DEL ESTADO DEL VOLCÁN TUNGURAHUA, Semana: Del 24 al 31 de mayo del 2016).

In a Special Report released on 2 June 2016, IG-EPN noted a clear inflationary trend in data collected from two stations at Tungurahua since the end of the eruption in mid-March. The Retu inclinometer, located N of the crater, showed inflation on the radial axis of about 600 μrad (microradians), and about 200 μrad on the tangential axis. The same axis at the Mandur inclinometer (on the NW flank) had a smaller but distinct (~30 μrad) inflationary signal (figure 110).

Figure 110. The pattern of deformation registered at the Retu (Refugio Tungurahua) and Mndr (Mandur) inclinometers from 14 February-30 May 2016 at Tungurahua. The gray area corresponds to the eruption of 26 February -16 March. An inflationary trend is apparent on both axes at the Retu instrument and on the tangential axis of the Mndr site. Courtesy of IG-EPN (Informe Especial Volcán Tungurahua - N°6, 2 de Junio de 2016).

A Washington VAAC report on 1 June 2016 noted that the Guayaquil Meteorological Weather Office (MWO) reported an ash plume at Tungurahua, but OVT confirmed no surface activity. A very small lahar was recorded in the La Pampa ravine on 2 June. Although there were rains of varying intensity many days during June, they did not generate significant lahars, except one of medium size that occurred on 21 June in the Achupashal ravine. The Washington VAAC noted a report from the Guayaquil MWO of an ash emission on 5 July, but it was not detected in satellite imagery, and the OVT reported no surface activity. There was no surface activity reported by OVT from July to mid-September (figure 111), and internal seismicity remained very low. Occasional rainy periods generated muddy water in the ravines, but no significant lahars were reported.

Figure 111. The summit of Tungurahua showed no sign of surface activity on 1 August 2016. Photo by Bernard J., courtesy of OVT, IG-EPN (INFORME No. 858, SÍNTESIS SEMANAL DEL ESTADO DEL VOLCÁN TUNGURAHUA, Semana: Del 26 de julio al 02 de agosto de 2016).

A significant increase in the number of LP seismic events began on 12 September 2016, and a small seismic swarm was recorded on 18 September (figure 112). Small fumaroles were visible at the edges of the crater on 15 and 16 September (figure 113). At this same time, the inflationary trend that had been ongoing since the eruption earlier in the year switched to deflation as measured at the Retu inclinometer.

Figure 112. The number of different types of seismic events and explosions recorded at Tungurahua between 1 January and 18 September 2016. The largest spike between 26 February and 16 March corresponds to the eruption of that period. Other episodes of seismicity were recorded during May and mid-September, but did not result in ash emissions or explosions. Courtesy of IG-EPN (Informe Especial Volcán Tungurahua - N°7, 18 de Septiembre de 2016).

Figure 113. Closeup images of the summit of Tungurahua on 15 (top) and 16 (bottom) September 2016 reveal minor fumarolic activity. Top: Steam rises from two snow free areas on 15 September (INFORME No. 865, SÍNTESIS SEMANAL DEL ESTADO DEL VOLCÁN TUNGURAHUA, Semana: Del 13 al 20 de septiembre de 2016). Bottom: Fumarolic activity was also apparent in this telephoto image taken from OVT on 16 September. Photo by P. Ramón (Informe Especial Volcán Tungurahua - N°7, 18 de Septiembre de 2016). Courtesy of OVT, IG-EPN.

Another increase in LP seismicity and tremors occurred on 24 September, but there were no reports of surface activity other than minor steam fumaroles. Seismicity remained elevated through early October; a one-hour tremor event was reported on 1 October. Seismicity decreased gradually over the following two weeks. Low-energy steam and gas emissions from fumaroles located on the S and SW flanks were observed during a flyover on 7 October 2016. This corresponded to the warmest areas revealed in the thermal image of the summit (figure 114). with a TMA (maximum apparent temperature) of 47.9°C and 36.5°C.

Figure 114. A thermal image of the summit of Tungurahua taken during a flyover on 7 October 2016 showed two areas on the crater rim with slightly elevated temperatures where fumarolic activity was occasionally observed. Image by P. Ramón, courtesy of OVT, IG-EPN (INFORME No. 868, SÍNTESIS SEMANAL DEL ESTADO DEL VOLCÁN TUNGURAHUA, Semana: Del 4 al 11 de octubre de 2016).

Re-suspended ash from high winds in mid-November 2016 caused several VAAC notices to be issued, but no new emissions were reported by OVT through the end of 2016.

Tungurahua remained quiet throughout 2017. A 90-minute seismic swarm on 8 January 2017 and a minor increase in seismicity in the second half of March were the only seismic events above background levels. There were no emissions except for occasional minor fumarolic activity around the crater rim. Periods of heavy rainfall occasionally produced muddy water in the ravines; the only lahars were reported during 5-6 January, late April and 15 November.

Geologic Background. Tungurahua, a steep-sided andesitic-dacitic stratovolcano that towers more than 3 km above its northern base, is one of Ecuador's most active volcanoes. Three major edifices have been sequentially constructed since the mid-Pleistocene over a basement of metamorphic rocks. Tungurahua II was built within the past 14,000 years following the collapse of the initial edifice. Tungurahua II collapsed about 3,000 years ago and produced a large debris-avalanche deposit to the west. The modern glacier-capped stratovolcano (Tungurahua III) was constructed within the landslide scarp. Historical eruptions have all originated from the summit crater, accompanied by strong explosions and sometimes by pyroclastic flows and lava flows that reached populated areas at the volcano's base. Prior to a long-term eruption beginning in 1999 that caused the temporary evacuation of the city of Baños at the foot of the volcano, the last major eruption had occurred from 1916 to 1918, although minor activity continued until 1925.

Information Contacts: Instituto Geofísico (IG), Escuela Politécnica Nacional, Casilla 17-01-2759, Quito, Ecuador (URL: http://www.igepn.edu.ec ); NASA Goddard Space Flight Center (NASA/GSFC), Global Sulfur Dioxide Monitoring Page, Atmospheric Chemistry and Dynamics Laboratory, 8800 Greenbelt Road, Goddard, Maryland, USA (URL: https://so2.gsfc.nasa.gov/); Washington Volcanic Ash Advisory Center (VAAC), Satellite Analysis Branch (SAB), NOAA/NESDIS OSPO, NOAA Science Center Room 401, 5200 Auth Rd, Camp Springs, MD 20746, USA (URL: www.ospo.noaa.gov/Products/atmosphere/vaac, archive at: http://www.ssd.noaa.gov/VAAC/archive.html).

Regular monitoring reports about Yasur from the Vanuatu Meteorology and Geo-Hazards Department (VMGD) indicated that the centuries-long eruptive activity continued from mid-June 2017 through January 2018. VMGD volcano bulletins on 21 July, 30 August, 29 September, 31 October, and 8 December 2017, and 30 January 2018, stated that major unrest was continuing, and the Alert Level remained at 2 (on a scale of 0-4). Based on seismic data, explosions continued to be intense. Visitors were reminded of the closed 395-m-radius Permanent Exclusion Zone (figure 47) and that volcanic ash and gas could impact other areas near the volcano due to trade winds.

Figure 47. Oblique aerial photograph of Yasur with an overlay of designated hazard zones that may be closed depending on the level of eruptive activity. Courtesy of Vanuatu Meteorology and Geo-Hazards Department.

During the reporting period thermal anomalies based on MODIS satellite instruments analyzed using the MODVOLC algorithm were numerous every month. The MIROVA (Middle InfraRed Observation of Volcanic Activity) system also detected numerous hotspots every month (figure 48).

Figure 48. Thermal anomalies detected in MODIS data by the MIROVA system (log radiative power) at Yasur for the year ending 23 February 2018. Courtesy of MIROVA.

Geologic Background. Yasur has exhibited essentially continuous Strombolian and Vulcanian activity at least since Captain Cook observed ash eruptions in 1774. This style of activity may have continued for the past 800 years. Located at the SE tip of Tanna Island in Vanuatu, this pyroclastic cone has a nearly circular, 400-m-wide summit crater. The active cone is largely contained within the small Yenkahe caldera, and is the youngest of a group of Holocene volcanic centers constructed over the down-dropped NE flank of the Pleistocene Tukosmeru volcano. The Yenkahe horst is located within the Siwi ring fracture, a 4-km-wide open feature associated with eruption of the andesitic Siwi pyroclastic sequence. Active tectonism along the Yenkahe horst accompanying eruptions has raised Port Resolution harbor more than 20 m during the past century.

Information Contacts: Geo-Hazards Division, Vanuatu Meteorology and Geo-Hazards Department, Ministry of Climate Change Adaptation, Meteorology, Geo-Hazards, Energy, Environment and Disaster Management, Private Mail Bag 9054, Lini Highway, Port Vila, Vanuatu (URL: http://www.vmgd.gov.vu/, https://www.facebook.com/VanuatuGeohazardsObservatory/); Radio New Zealand (URL: https://www.radionz.co.nz); 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/).