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Bulletin of the Global Volcanism Network

All reports of volcanic activity published by the Smithsonian since 1968 are available through a monthly table of contents or by searching for a specific volcano. Until 1975, reports were issued for individual volcanoes as information became available; these have been organized by month for convenience. Later publications were done in a monthly newsletter format. Links go to the profile page for each volcano with the Bulletin tab open.

Information is preliminary at time of publication and subject to change.

Recently Published Bulletin Reports

Ibu (Indonesia) Daily ash explosions continue, along with thermal anomalies in the crater, October 2022-May 2023

Dukono (Indonesia) Continuing ash emissions, SO2 plumes, and thermal signals during October 2022-May 2023

Sabancaya (Peru) Explosions, gas-and-ash plumes, and thermal activity persist during November 2022-April 2023

Sheveluch (Russia) Significant explosions destroyed part of the lava-dome complex during April 2023

Bezymianny (Russia) Explosions, ash plumes, lava flows, and avalanches during November 2022-April 2023

Chikurachki (Russia) New explosive eruption during late January-early February 2023

Marapi (Indonesia) New explosive eruption with ash emissions during January-March 2023

Kikai (Japan) Intermittent white gas-and-steam plumes, discolored water, and seismicity during May 2021-April 2023

Lewotolok (Indonesia) Strombolian eruption continues through April 2023 with intermittent ash plumes

Barren Island (India) Thermal activity during December 2022-March 2023

Villarrica (Chile) Nighttime crater incandescence, ash emissions, and seismicity during October 2022-March 2023

Fuego (Guatemala) Daily explosions, gas-and-ash plumes, avalanches, and ashfall during December 2022-March 2023



Ibu (Indonesia) — June 2023 Citation iconCite this Report

Ibu

Indonesia

1.488°N, 127.63°E; summit elev. 1325 m

All times are local (unless otherwise noted)


Daily ash explosions continue, along with thermal anomalies in the crater, October 2022-May 2023

Persistent eruptive activity since April 2008 at Ibu, a stratovolcano on Indonesian’s Halmahera Island, has consisted of daily explosive ash emissions and plumes, along with observations of thermal anomalies (BGVN 47:04). The current eruption continued during October 2022-May 2023, described below, based on advisories issued by the Pusat Vulkanologi dan Mitigasi Bencana Geologi (PVMBG, also known as Indonesian Center for Volcanology and Geological Hazard Mitigation, CVGHM), daily reports by MAGMA Indonesia (a PVMBG platform), and the Darwin Volcanic Ash Advisory Centre (VAAC), and various satellite data. The Alert Level during the reporting period remained at 2 (on a scale of 1-4), except raised briefly to 3 on 27 May, and the public was warned to stay at least 2 km away from the active crater and 3.5 km away on the N side of the volcano.

According to MAGMA Indonesia, during October 2022-May 2023, daily gray-and-white ash plumes of variable densities rose 200-1,000 m above the summit and drifted in multiple directions. On 30 October and 11 November, plumes rose a maximum of 2 km and 1.5 km above the summit, respectively (figures 42 and 43). According to the Darwin VAAC, discrete ash emissions on 13 November rose to 2.1 km altitude, or 800 m above the summit, and drifted W, and multiple ash emissions on 15 November rose 1.4 km above the summit and drifted NE. Occasional larger ash explosions through May 2023 prompted PVMBG to issue Volcano Observatory Notice for Aviation (VONA) alerts (table 6); the Aviation Color Code remained at Orange throughout this period.

Figure (see Caption) Figure 42. Larger explosion from Ibu’s summit crater on 30 October 2022 that generated a plume that rose 2 km above the summit. Photo has been color corrected. Courtesy of MAGMA Indonesia.
Figure (see Caption) Figure 43. Larger explosion from Ibu’s summit crater on 11 November 2022 that generated a plume that rose 1.5 km above the summit. Courtesy of MAGMA Indonesia.

Table 6. Volcano Observatory Notice for Aviation (VONA) ash plume alerts for Ibu issued by PVMBG during October 2022-May 2023. Maximum height above the summit was estimated by a ground observer. VONAs in January-May 2023 all described the ash plumes as dense.

Date Time (local) Max height above summit Direction
17 Oct 2022 0858 800 m SW
18 Oct 2022 1425 800 m S
19 Oct 2022 2017 600 m SW
21 Oct 2022 0916 800 m NW
16 Jan 2023 1959 600 m NE
22 Jan 2023 0942 1,000 m E
29 Jan 2023 2138 1,000 m E
10 May 2023 0940 800 m NW
10 May 2023 2035 600 m E
21 May 2023 2021 600 m W
21 May 2023 2140 1,000 m W
29 May 2023 1342 800 m N
31 May 2023 1011 1,000 m SW

Sentinel-2 L1C satellite images throughout the reporting period show two, sometimes three persistent thermal anomalies in the summit crater, with the most prominent hotspot from the top of a cone within the crater. Clear views were more common during March-April 2023, when a vent and lava flows on the NE flank of the intra-crater cone could be distinguished (figure 44). White-to-grayish emissions were also observed during brief periods when weather clouds allowed clear views.

Figure (see Caption) Figure 44. Sentinel-2 L2A satellite images of Ibu on 10 April 2023. The central cone within the summit crater (1.3 km diameter) and lava flows (gray) can be seen in the true color image (left, bands 4, 3, 2). Thermal anomalies from the small crater of the intra-crater cone, a NE-flank vent, and the end of the lava flow are apparent in the infrared image (right, bands 12, 11, 8A). Courtesy of Copernicus Browser.

The MIROVA space-based volcano hotspot detection system recorded almost daily thermal anomalies throughout the reporting period, though cloud cover often interfered with detections. Data from imaging spectroradiometers aboard NASA’s Aqua and Terra satellites and processed using the MODVOLC algorithm (MODIS-MODVOLC) recorded hotspots on one day during October 2022 and December 2022, two days in April 2023, three days in November 2022 and May 2023, and four days in March 2023.

Geologic Background. The truncated summit of Gunung Ibu stratovolcano along the NW coast of Halmahera Island has large nested summit craters. The inner crater, 1 km wide and 400 m deep, has contained several small crater lakes. The 1.2-km-wide outer crater is breached on the N, creating a steep-walled valley. A large cone grew ENE of the summit, and a smaller one to the WSW has fed a lava flow down the W flank. A group of maars is located below the N and W flanks. The first observed and recorded eruption was a small explosion from the summit crater in 1911. Eruptive activity began again in December 1998, producing a lava dome that eventually covered much of the floor of the inner summit crater along with ongoing explosive ash emissions.

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 (Multiplatform Application for Geohazard Mitigation and Assessment in Indonesia), Kementerian Energi dan Sumber Daya Mineral (URL: https://magma.esdm.go.id/v1); Copernicus Browser, Copernicus Data Space Ecosystem, European Space Agency (URL: https://dataspace.copernicus.eu/browser/); 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/).


Dukono (Indonesia) — June 2023 Citation iconCite this Report

Dukono

Indonesia

1.6992°N, 127.8783°E; summit elev. 1273 m

All times are local (unless otherwise noted)


Continuing ash emissions, SO2 plumes, and thermal signals during October 2022-May 2023

Dukono, a remote volcano on Indonesia’s Halmahera Island, has been erupting continuously since 1933, with frequent ash explosions and sulfur dioxide plumes (BGVN 46:11, 47:10). This activity continued during October 2022 through May 2023, based on reports from the Pusat Vulkanologi dan Mitigasi Bencana Geologi (PVMBG; also known as Indonesian Center for Volcanology and Geological Hazard Mitigation, CVGHM), the Darwin Volcanic Ash Advisory Centre (VAAC), and satellite data. During this period, the Alert Level remained at 2 (on a scale of 1-4) and the public was warned to remain outside of the 2-km exclusion zone. The highest reported plume of the period reached 9.4 km above the summit on 14 November 2022.

According to MAGMA Indonesia (a platform developed by PVMBG), white, gray, or dark plumes of variable densities were observed almost every day during the reporting period, except when fog obscured the volcano (figure 33). Plumes generally rose 25-450 m above the summit, but rose as high as 700-800 m on several days, somewhat lower than the maximum heights reached earlier in 2022 when plumes reached as high as 1 km. However, the Darwin VAAC reported that on 14 November 2022, a discrete ash plume rose 9.4 km above the summit (10.7 km altitude), accompanied by a strong hotspot and a sulfur dioxide signal observed in satellite imagery; a continuous ash plume that day and through the 15th rose to 2.1-2.4 km altitude and drifted NE.

Figure (see Caption) Figure 33. Webcam photo of a gas-and-steam plume rising from Dukono on the morning of 28 January 2023. Courtesy of MAGMA Indonesia.

Sentinel-2 images were obscured by weather clouds almost every viewing day during the reporting period. However, the few reasonably clear images showed a hotspot and white or gray emissions and plumes. Strong SO2 plumes from Dukono were present on many days during October 2022-May 2023, as detected using the TROPOMI instrument on the Sentinel-5P satellite (figure 34).

Figure (see Caption) Figure 34. A strong SO2 signal from Dukono on 23 April 2023 was the most extensive plume detected during the reporting period. Courtesy of the NASA Global Sulfur Dioxide Monitoring Page.

Geologic Background. Reports from this remote volcano in northernmost Halmahera are rare, but Dukono has been one of Indonesia's most active volcanoes. More-or-less continuous explosive eruptions, sometimes accompanied by lava flows, have occurred since 1933. During a major eruption in 1550 CE, a lava flow filled in the strait between Halmahera and the N-flank Gunung Mamuya cone. This complex volcano presents a broad, low profile with multiple summit peaks and overlapping craters. Malupang Wariang, 1 km SW of the summit crater complex, contains a 700 x 570 m crater that has also been active during historical time.

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 (Multiplatform Application for Geohazard Mitigation and Assessment in 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/); 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/); Sentinel Hub Playground (URL: https://www.sentinel-hub.com/explore/sentinel-playground).


Sabancaya (Peru) — May 2023 Citation iconCite this Report

Sabancaya

Peru

15.787°S, 71.857°W; summit elev. 5960 m

All times are local (unless otherwise noted)


Explosions, gas-and-ash plumes, and thermal activity persist during November 2022-April 2023

Sabancaya is located in Peru, NE of Ampato and SE of Hualca Hualca. Eruptions date back to 1750 and have been characterized by explosions, phreatic activity, ash plumes, and ashfall. The current eruption period began in November 2016 and has more recently consisted of daily explosions, gas-and-ash plumes, and thermal activity (BGVN 47:11). This report updates activity during November 2022 through April 2023 using information from Instituto Geophysico del Peru (IGP) that use weekly activity reports and various satellite data.

Intermittent low-to-moderate power thermal anomalies were reported by the MIROVA project during November 2022 through April 2023 (figure 119). There were few short gaps in thermal activity during mid-December 2022, late December-to-early January 2023, late January to mid-February, and late February. According to data recorded by the MODVOLC thermal algorithm, there were a total of eight thermal hotspots: three in November 2022, three in February 2023, one in March, and one in April. On clear weather days, some of this thermal anomaly was visible in infrared satellite imagery showing the active lava dome in the summit crater (figure 120). Almost daily moderate-to-strong sulfur dioxide plumes were recorded during the reporting period by the TROPOMI instrument on the Sentinel-5P satellite (figure 121). Many of these plumes exceeded 2 Dobson Units (DU) and drifted in multiple directions.

Figure (see Caption) Figure 119. Intermittent low-to-moderate thermal anomalies were detected during November 2022 through April 2023 at Sabancaya, as shown in this MIROVA graph (Log Radiative Power). There were brief gaps in thermal activity during mid-December 2022, late December-to-early January 2023, late January to mid-February, and late February. Courtesy of MIROVA.
Figure (see Caption) Figure 120. Infrared (bands 12, 11, 8A) satellite images showed a constant thermal anomaly in the summit crater of Sabancaya on 14 January 2023 (top left), 28 February 2023 (top right), 5 March 2023 (bottom left), and 19 April 2023 (bottom right), represented by the active lava dome. Sometimes gas-and-steam and ash emissions also accompanied this activity. Courtesy of Copernicus Browser.
Figure (see Caption) Figure 121. Moderate-to-strong sulfur dioxide plumes were detected almost every day, rising from Sabancaya by the TROPOMI instrument on the Sentinel-5P satellite throughout the reporting period; the DU (Dobson Unit) density values were often greater than 2. Plumes from 23 November 2022 (top left), 26 December 2022 (top middle), 10 January 2023 (top right), 15 February 2023 (bottom left), 13 March 2023 (bottom middle), and 21 April 2023 (bottom right) that drifted SW, SW, W, SE, W, and SW, respectively. Courtesy of NASA Global Sulfur Dioxide Monitoring Page.

IGP reported that moderate activity during November and December 2022 continued; during November, an average number of explosions were reported each week: 30, 33, 36, and 35, and during December, it was 32, 40, 47, 52, and 67. Gas-and-ash plumes in November rose 3-3.5 km above the summit and drifted E, NE, SE, S, N, W, and SW. During December the gas-and-ash plumes rose 2-4 km above the summit and drifted in different directions. There were 1,259 volcanic earthquakes recorded during November and 1,693 during December. Seismicity also included volcano-tectonic-type events that indicate rock fracturing events. Slight inflation was observed in the N part of the volcano near Hualca Hualca (4 km N). Thermal activity was frequently reported in the crater at the active lava dome (figure 120).

Explosive activity continued during January and February 2023. The average number of explosions were reported each week during January (51, 50, 60, and 59) and February (43, 54, 51, and 50). Gas-and-ash plumes rose 1.6-2.9 km above the summit and drifted NW, SW, and W during January and rose 1.4-2.8 above the summit and drifted W, SW, E, SE, N, S, NW, and NE during February. IGP also detected 1,881 volcanic earthquakes during January and 1,661 during February. VT-type earthquakes were also reported. Minor inflation persisted near Hualca Hualca. Satellite imagery showed continuous thermal activity in the crater at the lava dome (figure 120).

During March, the average number of explosions each week was 46, 48, 31, 35, and 22 and during April, it was 29, 41, 31, and 27. Accompanying gas-and-ash plumes rose 1.7-2.6 km above the summit crater and drifted W, SW, NW, S, and SE during March. According to a Buenos Aires Volcano Ash Advisory Center (VAAC) notice, on 22 March at 1800 through 23 March an ash plume rose to 7 km altitude and drifted NW. By 0430 an ash plume rose to 7.6 km altitude and drifted W. On 24 and 26 March continuous ash emissions rose to 7.3 km altitude and drifted SW and on 28 March ash emissions rose to 7.6 km altitude. During April, gas-and-ash plumes rose 1.6-2.5 km above the summit and drifted W, SW, S, NW, NE, and E. Frequent volcanic earthquakes were recorded, with 1,828 in March and 1,077 in April, in addition to VT-type events. Thermal activity continued to be reported in the summit crater at the lava dome (figure 120).

Geologic Background. Sabancaya, located in the saddle NE of Ampato and SE of Hualca Hualca volcanoes, is the youngest of these volcanic centers and the only one to have erupted in historical time. The oldest of the three, Nevado Hualca Hualca, is of probable late-Pliocene to early Pleistocene age. The name Sabancaya (meaning "tongue of fire" in the Quechua language) first appeared in records in 1595 CE, suggesting activity prior to that date. Holocene activity has consisted of Plinian eruptions followed by emission of voluminous andesitic and dacitic lava flows, which form an extensive apron around the volcano on all sides but the south. Records of historical eruptions date back to 1750.

Information Contacts: Instituto Geofisico del Peru (IGP), Centro Vulcanológico Nacional (CENVUL), Calle Badajoz N° 169 Urb. Mayorazgo IV Etapa, Ate, Lima 15012, Perú (URL: https://www.igp.gob.pe/servicios/centro-vulcanologico-nacional/inicio); Buenos Aires Volcanic Ash Advisory Center (VAAC), Servicio Meteorológico Nacional-Fuerza Aérea Argentina, 25 de mayo 658, Buenos Aires, Argentina (URL: http://www.smn.gov.ar/vaac/buenosaires/inicio.php); 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 MD 20771, USA (URL: https://so2.gsfc.nasa.gov/); Copernicus Browser, Copernicus Data Space Ecosystem, European Space Agency (URL: https://dataspace.copernicus.eu/browser/).


Sheveluch (Russia) — May 2023 Citation iconCite this Report

Sheveluch

Russia

56.653°N, 161.36°E; summit elev. 3283 m

All times are local (unless otherwise noted)


Significant explosions destroyed part of the lava-dome complex during April 2023

Sheveluch (also spelled Shiveluch) in Kamchatka, has had at least 60 large eruptions during the last 10,000 years. The summit is truncated by a broad 9-km-wide caldera that is breached to the S, and many lava domes occur on the outer flanks. The lava dome complex was constructed within the large open caldera. Frequent collapses of the dome complex have produced debris avalanches; the resulting deposits cover much of the caldera floor. A major south-flank collapse during a 1964 Plinian explosion produced a scarp in which a “Young Sheveluch” dome began to form in 1980. Repeated episodes of dome formation and destruction since then have produced major and minor ash plumes, pyroclastic flows, block-and-ash flows, and “whaleback domes” of spine-like extrusions in 1993 and 2020 (BGVN 45:11). The current eruption period began in August 1999 and has more recently consisted of lava dome growth, explosions, ash plumes, and avalanches (BGVN 48:01). This report covers a significant explosive eruption during early-to-mid-April 2023 that generated a 20 km altitude ash plume, produced a strong sulfur dioxide plume, and destroyed part of the lava-dome complex; activity described during January through April 2023 use information primarily from the Kamchatka Volcanic Eruptions Response Team (KVERT) and various satellite data.

Satellite data. Activity during the majority of this reporting period was characterized by continued lava dome growth, strong fumarole activity, explosions, and hot avalanches. According to the MODVOLC Thermal Alerts System, 140 hotspots were detected through the reporting period, with 33 recorded in January 2023, 29 in February, 44 in March, and 34 in April. Frequent strong thermal activity was recorded during January 2023 through April, according to the MIROVA (Middle InfraRed Observation of Volcanic Activity) graph and resulted from the continuously growing lava dome (figure 94). A slightly stronger pulse in thermal activity was detected in early-to-mid-April, which represented the significant eruption that destroyed part of the lava-dome complex. Thermal anomalies were also visible in infrared satellite imagery at the summit crater (figure 95).

Figure (see Caption) Figure 94. Strong and frequent thermal activity was detected at Sheveluch during January through April 2023, according to this MIROVA graph (Log Radiative Power). These thermal anomalies represented the continuously growing lava dome and frequent hot avalanches that affected the flanks. During early-to-mid-April a slightly stronger pulse represented the notable explosive eruption. Courtesy of MIROVA.
Figure (see Caption) Figure 95. Infrared (bands B12, B11, B4) satellite imagery showed persistent thermal anomalies at the lava dome of Sheveluch on 14 January 2023 (top left), 26 February 2023 (top right), and 15 March 2023 (bottom left). The true color image on 12 April 2023 (bottom right) showed a strong ash plume that drifted SW; this activity was a result of the strong explosive eruption during 11-12 April 2023. Courtesy of Copernicus Browser.

During January 2023 KVERT reported continued growth of the lava dome, accompanied by strong fumarolic activity, incandescence from the lava dome, explosions, ash plumes, and avalanches. Satellite data showed a daily thermal anomaly over the volcano. Video data showed ash plumes associated with collapses at the dome that generated avalanches that in turn produced ash plumes rising to 3.5 km altitude and drifting 40 km W on 4 January and rising to 7-7.5 km altitude and drifting 15 km SW on 5 January. A gas-and-steam plume containing some ash that was associated with avalanches rose to 5-6 km altitude and extended 52-92 km W on 7 January. Explosions that same day produced ash plumes that rose to 7-7.5 km altitude and drifted 10 km W. According to a Volcano Observatory Notice for Aviation (VONA) issued at 1344 on 19 January, explosions produced an ash cloud that was 15 x 25 km in size and rose to 9.6-10 km altitude, drifting 21-25 km W; as a result, the Aviation Color Code (ACC) was raised to Red (the highest level on a four-color scale). Another VONA issued at 1635 reported that no more ash plumes were observed, and the ACC was lowered to Orange (the second highest level on a four-color scale). On 22 January an ash plume from collapses and avalanches rose to 5 km altitude and drifted 25 km NE and SW; ash plumes associated with collapses extended 70 km NE on 27 and 31 January.

Lava dome growth, fumarolic activity, dome incandescence, and occasional explosions and avalanches continued during February and March. A daily thermal anomaly was visible in satellite data. Explosions on 1 February generated ash plumes that rose to 6.3-6.5 km altitude and extended 15 km NE. Video data showed an ash cloud from avalanches rising to 5.5 km altitude and drifting 5 km SE on 2 February. Satellite data showed gas-and-steam plumes containing some ash rose to 5-5.5 km altitude and drifted 68-110 km ENE and NE on 6 February, to 4.5-5 km altitude and drifted 35 km WNW on 22 February, and to 3.7-4 km altitude and drifted 47 km NE on 28 February. Scientists from the Kamchatka Volcanological Station (KVS) went on a field excursion on 25 February to document the growing lava dome, and although it was cloudy most of the day, nighttime incandescence was visible. Satellite data showed an ash plume extending up to 118 km E during 4-5 March. Video data from 1150 showed an ash cloud from avalanches rose to 3.7-5.5 km altitude and drifted 5-10 km ENE and E on 5 March. On 11 March an ash plume drifted 62 km E. On 27 March ash plumes rose to 3.5 km altitude and drifted 100 km E. Avalanches and constant incandescence at the lava dome was focused on the E and NE slopes on 28 March. A gas-and-steam plume containing some ash rose to 3.5 km altitude and moved 40 km E on 29 March. Ash plumes on 30 March rose to 3.5-3.7 km altitude and drifted 70 km NE.

Similar activity continued during April, with lava dome growth, strong fumarolic activity, incandescence in the dome, occasional explosions, and avalanches. A thermal anomaly persisted throughout the month. During 1-4 April weak ash plumes rose to 2.5-3 km altitude and extended 13-65 km SE and E.

Activity during 11 April 2023. The Institute of Volcanology and Seismology, Far Eastern Branch, Russian Academy of Sciences (IVS FEB RAS) reported a significant increase in seismicity around 0054 on 11 April, as reported by strong explosions detected on 11 April beginning at 0110 that sent ash plumes up to 7-10 km altitude and extended 100-435 km W, WNW, NNW, WSW, and SW. According to a Tokyo VAAC report the ash plume rose to 15.8 km altitude. By 0158 the plume extended over a 75 x 100 km area. According to an IVS FEB RAS report, the eruptive column was not vertical: the initial plume at 0120 on 11 April deviated to the NNE, at 0000 on 12 April, it drifted NW, and by 1900 it drifted SW. KVS reported that significant pulses of activity occurred at around 0200, 0320, and then a stronger phase around 0600. Levin Dmitry took a video from near Békés (3 km away) at around 0600 showing a rising plume; he also reported that a pyroclastic flow traveled across the road behind him as he left the area. According to IVS FEB RAS, the pyroclastic flow traveled several kilometers SSE, stopping a few hundred meters from a bridge on the road between Klyuchi and Petropavlovsk-Kamchatsky.

Ashfall was first observed in Klyuchi (45 km SW) at 0630, and a large, black ash plume blocked light by 0700. At 0729 KVERT issued a Volcano Observatory Notice for Aviation (VONA) raising the Aviation Color Code to Red (the highest level on a four-color scale). It also stated that a large ash plume had risen to 10 km altitude and drifted 100 km W. Near-constant lightning strikes were reported in the plume and sounds like thunderclaps were heard until about 1000. According to IVS FEB RAS the cloud was 200 km long and 76 km wide by 0830, and was spreading W at altitudes of 6-12 km. In the Klyuchi Village, the layer of both ash and snow reached 8.5 cm (figure 96); ashfall was also reported in Kozyrevsk (112 km SW) at 0930, Mayskoye, Anavgay, Atlasovo, Lazo, and Esso. Residents in Klyuchi reported continued darkness and ashfall at 1100. In some areas, ashfall was 6 cm deep and some residents reported dirty water coming from their plumbing. According to IVS FEB RAS, an ash cloud at 1150 rose to 5-20 km altitude and was 400 km long and 250 km wide, extending W. A VONA issued at 1155 reported that ash had risen to 10 km and drifted 340 km NNW and 240 km WSW. According to Simon Carn (Michigan Technological University), about 0.2 Tg of sulfur dioxide in the plume was measured in a satellite image from the TROPOMI instrument on the Sentinel-5P satellite acquired at 1343 that covered an area of about 189,000 km2 (figure 97). Satellite data at 1748 showed an ash plume that rose to 8 km altitude and drifted 430 km WSW and S, according to a VONA.

Figure (see Caption) Figure 96. Photo of ash deposited in Klyuchi village on 11 April 2023 by the eruption of Sheveluch. About 8.5 cm of ash was measured. Courtesy of Kam 24 News Agency.
Figure (see Caption) Figure 97. A strong sulfur dioxide plume from the 11 April 2023 eruption at Sheveluch was visible in satellite data from the TROPOMI instrument on the Sentinel-5P satellite. Courtesy of Simon Carn, MTU.

Activity during 12-15 April 2023. On 12 April at 0730 satellite images showed ash plumes rose to 7-8 km altitude and extended 600 km SW, 1,050 km ESE, and 1,300-3,000 km E. By 1710 that day, the explosions weakened. According to news sources, the ash-and-gas plumes drifted E toward the Aleutian Islands and reached the Gulf of Alaska by 13 April, causing flight disruptions. More than 100 flights involving Alaska airspace were cancelled due to the plume. Satellite data showed ash plumes rising to 4-5.5 km altitude and drifted 400-415 km SE and ESE on 13 April. KVS volcanologists observed the pyroclastic flow deposits and noted that steam rose from downed, smoldering trees. They also noted that the deposits were thin with very few large fragments, which differed from previous flows. The ash clouds traveled across the Pacific Ocean. Flight cancellations were also reported in NW Canada (British Columbia) during 13-14 April. During 14-15 April ash plumes rose to 6 km altitude and drifted 700 km NW.

Alaskan flight schedules were mostly back to normal by 15 April, with only minor delays and far less cancellations; a few cancellations continued to be reported in Canada. Clear weather on 15 April showed that most of the previous lava-dome complex was gone and a new crater roughly 1 km in diameter was observed (figure 98); gas-and-steam emissions were rising from this crater. Evidence suggested that there had been a directed blast to the SE, and pyroclastic flows traveled more than 20 km. An ash plume rose to 4.5-5.2 km altitude and drifted 93-870 km NW on 15 April.

Figure (see Caption) Figure 98. A comparison of the crater at Sheveluch showing the previous lava dome (top) taken on 29 November 2022 and a large crater in place of the dome (bottom) due to strong explosions during 10-13 April 2023, accompanied by gas-and-ash plumes. The bottom photo was taken on 15 April 2023. Photos has been color corrected. Both photos are courtesy of Yu. Demyanchuk, IVS FEB RAS, KVERT.

Activity during 16-30 April 2023. Resuspended ash was lifted by the wind from the slopes and rose to 4 km altitude and drifted 224 km NW on 17 April. KVERT reported a plume of resuspended ash from the activity during 10-13 April on 19 April that rose to 3.5-4 km altitude and drifted 146-204 km WNW. During 21-22 April a plume stretched over the Scandinavian Peninsula. A gas-and-steam plume containing some ash rose to 3-3.5 km altitude and drifted 60 km SE on 30 April. A possible new lava dome was visible on the W slope of the volcano on 29-30 April (figure 99); satellite data showed two thermal anomalies, a bright one over the existing lava dome and a weaker one over the possible new one.

Figure (see Caption) Figure 99. Photo showing new lava dome growth at Sheveluch after a previous explosion destroyed much of the complex, accompanied by a white gas-and-steam plume. Photo has been color corrected. Courtesy of Yu. Demyanchuk, IVS FEB RAS, KVERT.

References. Girina, O., Loupian, E., Horvath, A., Melnikov, D., Manevich, A., Nuzhdaev, A., Bril, A., Ozerov, A., Kramareva, L., Sorokin, A., 2023, Analysis of the development of the paroxysmal eruption of Sheveluch volcano on April 10–13, 2023, based on data from various satellite systems, ??????????? ???????? ??? ?? ???????, 20(2).

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 Eastern Branch, 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/); Kamchatka Volcanological Station, Kamchatka Branch of Geophysical Survey, (KB GS RAS), Klyuchi, Kamchatka Krai, Russia (URL: http://volkstat.ru/); 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/); Copernicus Browser, Copernicus Data Space Ecosystem, European Space Agency (URL: https://dataspace.copernicus.eu/browser/); Kam 24 News Agency, 683032, Kamchatka Territory, Petropavlovsk-Kamchatsky, Vysotnaya St., 2A (URL: https://kam24.ru/news/main/20230411/96657.html#.Cj5Jrky6.dpuf); Simon Carn, Geological and Mining Engineering and Sciences, Michigan Technological University, 1400 Townsend Drive, Houghton, MI 49931, USA (URL: http://www.volcarno.com/, Twitter: @simoncarn).


Bezymianny (Russia) — May 2023 Citation iconCite this Report

Bezymianny

Russia

55.972°N, 160.595°E; summit elev. 2882 m

All times are local (unless otherwise noted)


Explosions, ash plumes, lava flows, and avalanches during November 2022-April 2023

Bezymianny is located on the Kamchatka Peninsula of Russia as part of the Klyuchevskoy volcano group. Historic eruptions began in 1955 and have been characterized by dome growth, explosions, pyroclastic flows, ash plumes, and ashfall. During the 1955-56 eruption a large open crater was formed by collapse of the summit and an associated lateral blast. Subsequent episodic but ongoing lava-dome growth, accompanied by intermittent explosive activity and pyroclastic flows, has largely filled the 1956 crater. The current eruption period began in December 2016 and more recent activity has consisted of strong explosions, ash plumes, and thermal activity (BGVN 47:11). This report covers activity during November 2022 through April 2023, based on weekly and daily reports from the Kamchatka Volcano Eruptions Response Team (KVERT) and satellite data.

Activity during November and March 2023 was relatively low and mostly consisted of gas-and-steam emissions, occasional small collapses that generated avalanches along the lava dome slopes, and a persistent thermal anomaly over the volcano that was observed in satellite data on clear weather days. According to the Tokyo VAAC and KVERT, an explosion produced an ash plume that rose to 6 km altitude and drifted 25 km NE at 1825 on 29 March.

Gas-and-steam emissions, collapses generating avalanches, and thermal activity continued during April. According to two Volcano Observatory Notice for Aviation (VONA) issued on 2 and 6 April (local time) ash plumes rose to 3 km and 3.5-3.8 km altitude and drifted 35 km E and 140 km E, respectively. Satellite data from KVERT showed weak ash plumes extending up to 550 km E on 2 and 5-6 April.

A VONA issued at 0843 on 7 April described an ash plume that rose to 4.5-5 km altitude and drifted 250 km ESE. Later that day at 1326 satellite data showed an ash plume that rose to 5.5-6 km altitude and drifted 150 km ESE. A satellite image from 1600 showed an ash plume extending as far as 230 km ESE; KVERT noted that ash emissions were intensifying, likely due to avalanches from the growing lava dome. The Aviation Color Code (ACC) was raised to Red (the highest level on a four-color scale). At 1520 satellite data showed an ash plume rising to 5-5.5 km altitude and drifting 230 km ESE. That same day, Kamchatka Volcanological Station (KVS) volcanologists traveled to Ambon to collect ash; they reported that a notable eruption began at 1730, and within 20 minutes a large ash plume rose to 10 km altitude and drifted NW. KVERT reported that the strong explosive phase began at 1738. Video and satellite data taken at 1738 showed an ash plume that rose to 10-12 km altitude and drifted up to 2,800 km SE and E. Explosions were clearly audible 20 km away for 90 minutes, according to KVS. Significant amounts of ash fell at the Apakhonchich station, which turned the snow gray; ash continued to fall until the morning of 8 April. In a VONA issued at 0906 on 8 April, KVERT stated that the explosive eruption had ended; ash plumes had drifted 2,000 km E. The ACC was lowered to Orange (the third highest level on a four-color scale). The KVS team saw a lava flow on the active dome once the conditions were clear that same day (figure 53). On 20 April lava dome extrusion was reported; lava flows were noted on the flanks of the dome, and according to KVERT satellite data, a thermal anomaly was observed in the area. The ACC was lowered to Yellow (the second lowest on a four-color scale).

Figure (see Caption) Figure 53. Photo showing an active lava flow descending the SE flank of Bezymianny from the lava dome on 8 April 2023. Courtesy of Yu. Demyanchuk, IVS FEB RAS, KVERT.

Satellite data showed an increase in thermal activity beginning in early April 2023. A total of 31 thermal hotspots were detected by the MODVOLC thermal algorithm on 4, 5, 7, and 12 April 2023. The elevated thermal activity resulted from an increase in explosive activity and the start of an active lava flow. The MIROVA (Middle InfraRed Observation of Volcanic Activity) volcano hotspot detection system based on the analysis of MODIS data also showed a pulse in thermal activity during the same time (figure 54). Infrared satellite imagery captured a continuous thermal anomaly at the summit crater, often accompanied by white gas-and-steam emissions (figure 55). On 4 April 2023 an active lava flow was observed descending the SE flank.

Figure (see Caption) Figure 54. Intermittent and low-power thermal anomalies were detected at Bezymianny during December 2022 through mid-March 2023, according to this MIROVA graph (Log Radiative Power). In early April 2023, an increase in explosive activity and eruption of a lava flow resulted in a marked increase in thermal activity. Courtesy of MIROVA.
Figure (see Caption) Figure 55. Infrared satellite images of Bezymianny showed a persistent thermal anomaly over the lava dome on 18 November 2022 (top left), 28 December 2022 (top right), 15 March 2023 (bottom left), and 4 April 2023 (bottom right), often accompanied by white gas-and-steam plumes. On 4 April a lava flow was active and descending the SE flank. Images using infrared (bands 12, 11, 8a). Courtesy of Copernicus Browser.

Geologic Background. The modern Bezymianny, much smaller than its massive neighbors Kamen and Kliuchevskoi on the Kamchatka Peninsula, was formed about 4,700 years ago over a late-Pleistocene lava-dome complex and an edifice built about 11,000-7,000 years ago. Three periods of intensified activity have occurred during the past 3,000 years. The latest period, which was preceded by a 1,000-year quiescence, began with the dramatic 1955-56 eruption. This eruption, similar to that of St. Helens in 1980, produced a large open crater that was formed by collapse of the summit and an associated lateral blast. Subsequent episodic but ongoing lava-dome growth, accompanied by intermittent explosive activity and pyroclastic flows, has largely filled the 1956 crater.

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/); Kamchatka Volcanological Station, Kamchatka Branch of Geophysical Survey, (KB GS RAS), Klyuchi, Kamchatka Krai, Russia (URL: http://volkstat.ru/); 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/); Copernicus Browser, Copernicus Data Space Ecosystem, European Space Agency (URL: https://dataspace.copernicus.eu/browser/).


Chikurachki (Russia) — May 2023 Citation iconCite this Report

Chikurachki

Russia

50.324°N, 155.461°E; summit elev. 1781 m

All times are local (unless otherwise noted)


New explosive eruption during late January-early February 2023

Chikurachki, located on Paramushir Island in the northern Kuriles, has had Plinian eruptions during the Holocene. Lava flows have reached the sea and formed capes on the NW coast; several young lava flows are also present on the E flank beneath a scoria deposit. Reported eruptions date back to 1690, with the most recent eruption period occurring during January through October 2022, characterized by occasional explosions, ash plumes, and thermal activity (BGVN 47:11). This report covers a new eruptive period during January through February 2023 that consisted of ash explosions and ash plumes, based on information from the Kamchatka Volcanic Eruptions Response Team (KVERT) and satellite data.

According to reports from KVERT, an explosive eruption began around 0630 on 29 January. Explosions generated ash plumes that rose to 3-3.5 km altitude and drifted 6-75 km SE and E, based on satellite data. As a result, the Aviation Color Code (ACC) was raised to Orange (the second highest level on a four-color scale). At 1406 and 1720 ash plumes were identified in satellite images that rose to 4.3 km altitude and extended 70 km E. By 2320 the ash plume had dissipated. A thermal anomaly was visible at the volcano on 31 January, according to a satellite image, and an ash plume was observed drifting 66 km NE.

Occasional explosions and ash plumes continued during early February. At 0850 on 1 February an ash plume rose to 3.5 km altitude and drifted 35 km NE. Satellite data showed an ash plume that rose to 3.2-3.5 km altitude and drifted 50 km NE at 1222 later that day (figure 22). A thermal anomaly was detected over the volcano during 5-6 February and ash plumes drifted as far as 125 km SE, E, and NE. Explosive events were reported at 0330 on 6 February that produced ash plumes rising to 4-4.5 km altitude and drifting 72-90 km N, NE, and ENE. KVERT noted that the last gas-and steam plume that contained some ash was observed on 8 February and drifted 55 km NE before the explosive eruption ended. The ACC was lowered to Yellow and then Green (the lowest level on a four-color scale) on 18 February.

Figure (see Caption) Figure 22. Satellite image showing a true color view of a strong ash plume rising above Chikurachki on 1 February 2023. The plume drifted NE and ash deposits (dark brown-to-gray) are visible on the NE flank due to explosive activity. Courtesy of Copernicus Browser.

Geologic Background. Chikurachki, the highest volcano on Paramushir Island in the northern Kuriles, is a relatively small cone constructed on a high Pleistocene edifice. Oxidized basaltic-to-andesitic scoria deposits covering the upper part of the young cone give it a distinctive red color. Frequent basaltic Plinian eruptions have occurred during the Holocene. Lava flows have reached the sea and formed capes on the NW coast; several young lava flows are also present on the E flank beneath a scoria deposit. The Tatarinov group of six volcanic centers is located immediately to the south, and the Lomonosov cinder cone group, the source of an early Holocene lava flow that reached the saddle between it and Fuss Peak to the west, lies at the southern end of the N-S-trending Chikurachki-Tatarinov complex. In contrast to the frequently active Chikurachki, the Tatarinov centers are extensively modified by erosion and have a more complex structure. Tephrochronology gives evidence of an eruption around 1690 CE from Tatarinov, although its southern cone contains a sulfur-encrusted crater with fumaroles that were active along the margin of a crater lake until 1959.

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


Marapi (Indonesia) — May 2023 Citation iconCite this Report

Marapi

Indonesia

0.38°S, 100.474°E; summit elev. 2885 m

All times are local (unless otherwise noted)


New explosive eruption with ash emissions during January-March 2023

Marapi in Sumatra, Indonesia, is a massive stratovolcano that rises 2 km above the Bukittinggi Plain in the Padang Highlands. A broad summit contains multiple partially overlapping summit craters constructed within the small 1.4-km-wide Bancah caldera and trending ENE-WSW, with volcanism migrating to the west. Since the end of the 18th century, more than 50 eruptions, typically characterized by small-to-moderate explosive activity, have been recorded. The previous eruption consisted of two explosions during April-May 2018, which caused ashfall to the SE (BGVN 43:06). This report covers a new eruption during January-March 2023, which included explosive events and ash emissions, as reported by Pusat Vulkanologi dan Mitigasi Bencana Geologi (PVMBG, also known as Indonesian Center for Volcanology and Geological Hazard Mitigation, CVGHM) and MAGMA Indonesia.

According to a press release issued by PVMBG and MAGMA Indonesia on 26 December, primary volcanic activity at Marapi consisted of white gas-and-steam puffs that rose 500-100 m above the summit during April-December 2022. On 25 December 2022 there was an increase in the number of deep volcanic earthquakes and summit inflation. White gas-and-steam emissions rose 80-158 m above the summit on 5 January. An explosive eruption began at 0611 on 7 January 2023, which generated white gas-and-steam emissions and gray ash emissions mixed with ejecta that rose 300 m above the summit and drifted SE (figure 10). According to ground observations, white-to-gray ash clouds during 0944-1034 rose 200-250 m above the summit and drifted SE and around 1451 emissions rose 200 m above the summit. Seismic signals indicated that eruptive events also occurred at 1135, 1144, 1230, 1715, and 1821, but no ash emissions were visually observed. On 8 January white-and-gray emissions rose 150-250 m above the summit that drifted E and SE. Seismic signals indicated eruptive events at 0447, 1038, and 1145, but again no ash emissions were visually observed on 8 January. White-to-gray ash plumes continued to be observed on clear weather days during 9-15, 18-21, 25, and 29-30 January, rising 100-1,000 m above the summit and drifted generally NE, SE, N, and E, based on ground observations (figure 11).

Figure (see Caption) Figure 10. Webcam image of the start of the explosive eruption at Marapi at 0651 on 7 January 2023. White gas-and-steam emissions are visible to the left and gray ash emissions are visible on the right, drifting SE. Distinct ejecta was also visible mixed within the ash cloud. Courtesy of PVMBG and MAGMA Indonesia.
Figure (see Caption) Figure 11. Webcam image showing thick, gray ash emissions rising 500 m above the summit of Marapi and drifting N and NE at 0953 on 11 January 2023. Courtesy of PVMBG and MAGMA Indonesia.

White-and-gray and brown emissions persisted in February, rising 50-500 m above the summit and drifting E, S, SW, N, NE, and W, though weather sometimes prevented clear views of the summit. An eruption at 1827 on 10 February produced a black ash plume that rose 400 m above the summit and drifted NE and E (figure 12). Similar activity was reported on clear weather days, with white gas-and-steam emissions rising 50 m above the summit on 9, 11-12, 20, and 27 March and drifted E, SE, SW, NE, E, and N. On 17 March white-and-gray emissions rose 400 m above the summit and drifted N and E.

Figure (see Caption) Figure 12. Webcam image showing an eruptive event at 1829 on 10 February 2023 with an ash plume rising 400 m above the summit and drifting NE and E. Courtesy of PVMBG and MAGMA Indonesia.

Geologic Background. Gunung Marapi, not to be confused with the better-known Merapi volcano on Java, is Sumatra's most active volcano. This massive complex stratovolcano rises 2,000 m above the Bukittinggi Plain in the Padang Highlands. A broad summit contains multiple partially overlapping summit craters constructed within the small 1.4-km-wide Bancah caldera. The summit craters are located along an ENE-WSW line, with volcanism migrating to the west. More than 50 eruptions, typically consisting of small-to-moderate explosive activity, have been recorded since the end of the 18th century; no lava flows outside the summit craters have been reported in historical time.

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).


Kikai (Japan) — May 2023 Citation iconCite this Report

Kikai

Japan

30.793°N, 130.305°E; summit elev. 704 m

All times are local (unless otherwise noted)


Intermittent white gas-and-steam plumes, discolored water, and seismicity during May 2021-April 2023

Kikai, located just S of the Ryukyu islands of Japan, contains a 19-km-wide mostly submarine caldera. The island of Satsuma Iwo Jima (also known as Satsuma-Iwo Jima and Tokara Iojima) is located at the NW caldera rim, as well as the island’s highest peak, Iodake. Its previous eruption period occurred on 6 October 2020 and was characterized by an explosion and thermal anomalies in the crater (BGVN 45:11). More recent activity has consisted of intermittent thermal activity and gas-and-steam plumes (BGVN 46:06). This report covers similar low-level activity including white gas-and-steam plumes, nighttime incandescence, seismicity, and discolored water during May 2021 through April 2023, using information from the Japan Meteorological Agency (JMA) and various satellite data. During this time, the Alert Level remained at a 2 (on a 5-level scale), according to JMA.

Activity was relatively low throughout the reporting period and has consisted of intermittent white gas-and-steam emissions that rose 200-1,400 m above the Iodake crater and nighttime incandescence was observed at the Iodake crater using a high-sensitivity surveillance camera. Each month, frequent volcanic earthquakes were detected, and sulfur dioxide masses were measured by the University of Tokyo Graduate School of Science, Kyoto University Disaster Prevention Research Institute, Mishima Village, and JMA (table 6).

Table 6. Summary of gas-and-steam plume heights, number of volcanic earthquakes detected, and amount of sulfur dioxide emissions in tons per day (t/d). Courtesy of JMA monthly reports.

Month Max plume height (m) Volcanic earthquakes Sulfur dioxide emissions (t/d)
May 2021 400 162 900-1,300
Jun 2021 800 117 500
Jul 2021 1,400 324 800-1,500
Aug 2021 1,000 235 700-1,000
Sep 2021 800 194 500-1,100
Oct 2021 800 223 600-800
Nov 2021 900 200 400-900
Dec 2021 1,000 161 500-1,800
Jan 2022 1,000 164 600-1,100
Feb 2022 1,000 146 500-1,600
Mar 2022 1,200 171 500-1,200
Apr 2022 1,000 144 600-1,000
May 2022 1,200 126 300-500
Jun 2022 1,000 154 400
Jul 2022 1,300 153 600-1,100
Aug 2022 1,100 109 600-1,500
Sep 2022 1,000 170 900
Oct 2022 800 249 700-1,200
Nov 2022 800 198 800-1,200
Dec 2022 700 116 600-1,500
Jan 2023 800 146 500-1,400
Feb 2023 800 135 600-800
Mar 2023 1,100 94 500-600
Apr 2023 800 82 500-700

Sentinel-2 satellite images show weak thermal anomalies at the Iodake crater on clear weather days, accompanied by white gas-and-steam emissions and occasional discolored water (figure 24). On 17 January 2022 JMA conducted an aerial overflight in cooperation with the Japan Maritime Self-Defense Force’s 1st Air Group, which confirmed a white gas-and-steam plume rising from the Iodake crater (figure 25). They also observed plumes from fumaroles rising from around the crater and on the E, SW, and N slopes. In addition, discolored water was reported near the coast around Iodake, which JMA stated was likely related to volcanic activity (figure 25). Similarly, an overflight taken on 11 January 2023 showed white gas-and-steam emissions rising from the Iodake crater, as well as discolored water that spread E from the coast around the island. On 14 February 2023 white fumaroles and discolored water were also captured during an overflight (figure 26).

Figure (see Caption) Figure 24. Sentinel-2 satellite images of Satsuma Iwo Jima (Kikai) showing sets of visual (true color) and infrared (bands 12, 11, 8a) views on 7 December 2021 (top), 23 October 2022 (middle), and 11 January 2023 (bottom). Courtesy of Copernicus Browser.
Figure (see Caption) Figure 25. Aerial image of Satsuma Iwo Jima (Kikai) showing a white gas-and-steam plume rising above the Iodake crater at 1119 on 17 January 2022. There was also green-yellow discolored water surrounding the coast of Mt. Iodake. Courtesy of JMSDF via JMA.
Figure (see Caption) Figure 26. Aerial image of Satsuma Iwo Jima (Kikai) showing white gas-and-steam plumes rising above the Iodake crater on 14 February 2023. Green-yellow discolored water surrounded Mt. Iodake. Courtesy of JCG.

Geologic Background. Multiple eruption centers have exhibited recent activity at Kikai, a mostly submerged, 19-km-wide caldera near the northern end of the Ryukyu Islands south of Kyushu. It was the source of one of the world's largest Holocene eruptions about 6,300 years ago when rhyolitic pyroclastic flows traveled across the sea for a total distance of 100 km to southern Kyushu, and ashfall reached the northern Japanese island of Hokkaido. The eruption devastated southern and central Kyushu, which remained uninhabited for several centuries. Post-caldera eruptions formed Iodake (or Iwo-dake) lava dome and Inamuradake scoria cone, as well as submarine lava domes. Recorded eruptions have occurred at or near Satsuma-Iojima (also known as Tokara-Iojima), a small 3 x 6 km island forming part of the NW caldera rim. Showa-Iojima lava dome (also known as Iojima-Shinto), a small island 2 km E of Satsuma-Iojima, was formed during submarine eruptions in 1934 and 1935. Mild-to-moderate explosive eruptions have occurred during the past few decades from Iodake, a rhyolitic lava dome at the eastern end of Satsuma-Iojima.

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); Japan Coast Guard (JCG) Volcano Database, Hydrographic and Oceanographic Department, 3-1-1, Kasumigaseki, Chiyoda-ku, Tokyo 100-8932, Japan (URL: https://www1.kaiho.mlit.go.jp/kaiikiDB/kaiyo30-2.htm); Copernicus Browser, Copernicus Data Space Ecosystem, European Space Agency (URL: https://dataspace.copernicus.eu/browser/).


Lewotolok (Indonesia) — May 2023 Citation iconCite this Report

Lewotolok

Indonesia

8.274°S, 123.508°E; summit elev. 1431 m

All times are local (unless otherwise noted)


Strombolian eruption continues through April 2023 with intermittent ash plumes

The current eruption at Lewotolok, in Indonesian’s Lesser Sunda Islands, began in late November 2020 and has included Strombolian explosions, occasional ash plumes, incandescent ejecta, intermittent thermal anomalies, and persistent white and white-and-gray emissions (BGVN 47:10). Similar activity continued during October 2022-April 2023, as described in this report based on information provided by Pusat Vulkanologi dan Mitigasi Bencana Geologi (PVMBG, also known as CVGHM, or the Center of Volcanology and Geological Hazard Mitigation), MAGMA Indonesia, the Darwin Volcanic Ash Advisory Centre (VAAC), and satellite data.

During most days in October 2022 white and white-gray emissions rose as high as 200-600 m above the summit. Webcam images often showed incandescence above the crater rim. At 0351 on 14 October, an explosion produced a dense ash plume that rose about 1.2 km above the summit and drifted SW (figure 43). After this event, activity subsided and remained low through the rest of the year, but with almost daily white emissions.

Figure (see Caption) Figure 43. Webcam image of Lewotolok on 14 October 2022 showing a dense ash plume and incandescence above the crater. Courtesy of MAGMA Indonesia.

After more than two months of relative quiet, PVMBG reported that explosions at 0747 on 14 January 2023 and at 2055 on 16 January produced white-and-gray ash plumes that rose around 400 m above the summit and drifted E and SE (figure 44). During the latter half of January through April, almost daily white or white-and-gray emissions were observed rising 25-800 m above the summit, and nighttime webcam images often showed incandescent material being ejected above the summit crater. Strombolian activity was visible in webcam images at 2140 on 11 February, 0210 on 18 February, and during 22-28 March. Frequent hotspots were recorded by the MIROVA detection system starting in approximately the second week of March 2023 that progressively increased into April (figure 45).

Figure (see Caption) Figure 44. Webcam image of an explosion at Lewotolok on 14 January 2023 ejecting a small ash plume along with white emissions. Courtesy of MAGMA Indonesia.
Figure (see Caption) Figure 45. MIROVA Log Radiative Power graph of thermal anomalies detected by the VIIRS satellite instrument at Lewotolok’s summit crater for the year beginning 24 July 2022. Clusters of mostly low-power hotspots occurred during August-October 2022, followed by a gap of more than four months before persistent and progressively stronger anomalies began in early March 2023. Courtesy of MIROVA.

Explosions that produced dense ash plumes as high as 750 m above the summit were described in Volcano Observatory Notices for Aviation (VONA) at 0517, 1623, and 2016 on 22 March, at 1744 on 24 March, at 0103 on 26 March, at 0845 and 1604 on 27 March (figure 46), and at 0538 on 28 March. According to the Darwin VAAC, on 6 April another ash plume rose to 1.8 km altitude (about 370 m above the summit) and drifted N.

Figure (see Caption) Figure 46. Webcam image of Lewotolok at 0847 on 27 March 2023 showing a dense ash plume from an explosion along with clouds and white emissions. Courtesy of MAGMA-Indonesia.

Sentinel-2 images over the previous year recorded thermal anomalies as well as the development of a lava flow that descended the NE flank beginning in June 2022 (figure 47). The volcano was often obscured by weather clouds, which also often hampered ground observations. Ash emissions were reported in March 2022 (BGVN 47:10), and clear imagery from 4 March 2022 showed recent lava flows confined to the crater, two thermal anomaly spots in the eastern part of the crater, and mainly white emissions from the SE. Thermal anomalies became stronger and more frequent in mid-May 2022, followed by strong Strombolian activity through June and July (BGVN 47:10); Sentinel-2 images on 2 June 2022 showed active lava flows within the crater and overflowing onto the NE flank. Clear images from 23 April 2023 (figure 47) show the extent of the cooled NE-flank lava flow, more extensive intra-crater flows, and two hotspots in slightly different locations compared to the previous March.

Figure (see Caption) Figure 47. Sentinel-2 satellite images of Lewotolok showing sets of visual (true color) and infrared (bands 12, 11, 8a) views on 4 March 2022, 2 June 2022, and 23 April 2023. Courtesy of Copernicus Browser.

Geologic Background. The Lewotolok (or Lewotolo) stratovolcano occupies the eastern end of an elongated peninsula extending north into the Flores Sea, connected to Lembata (formerly Lomblen) Island by a narrow isthmus. It is symmetrical when viewed from the north and east. A small cone with a 130-m-wide crater constructed at the SE side of a larger crater forms the volcano's high point. Many lava flows have reached the coastline. Eruptions recorded since 1660 have consisted of explosive activity from the summit crater.

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/).


Barren Island (India) — April 2023 Citation iconCite this Report

Barren Island

India

12.278°N, 93.858°E; summit elev. 354 m

All times are local (unless otherwise noted)


Thermal activity during December 2022-March 2023

Barren Island is part of a N-S-trending volcanic arc extending between Sumatra and Burma (Myanmar). The caldera, which is open to the sea on the west, was created during a major explosive eruption in the late Pleistocene that produced pyroclastic flow and surge deposits. Eruptions dating back to 1787, have changed the morphology of the pyroclastic cone in the center of the caldera, and lava flows that fill much of the caldera floor have reached the sea along the western coast. Previous activity was detected during mid-May 2022, consisting of intermittent thermal activity. This report covers June 2022 through March 2023, which included strong thermal activity beginning in late December 2022, based on various satellite data.

Activity was relatively quiet during June through late December 2022 and mostly consisted of low-power thermal anomalies, based on the MIROVA (Middle InfraRed Observation of Volcanic Activity) graph. During late December, a spike in both power and frequency of thermal anomalies was detected (figure 58). There was another pulse in thermal activity in mid-March, which consisted of more frequent and relatively strong anomalies.

Figure (see Caption) Figure 58. Occasional thermal anomalies were detected during June through late December 2022 at Barren Island, but by late December through early January 2023, there was a marked increase in thermal activity, both in power and frequency, according to this MIROVA graph (Log Radiative Power). After this spike in activity, anomalies occurred at a more frequent rate. In late March, another pulse in activity was detected, although the power was not as strong as that initial spike during December-January. Courtesy of MIROVA.

The Suomi NPP/VIIRS sensor data showed five thermal alerts on 29 December 2022. The number of alerts increased to 19 on 30 December. According to the Darwin VAAC, ash plumes identified in satellite images captured at 2340 on 30 December and at 0050 on 31 December rose to 1.5 km altitude and drifted SW. The ash emissions dissipated by 0940. On 31 December, a large thermal anomaly was detected; based on a Sentinel-2 infrared satellite image, the anomaly was relatively strong and extended to the N (figure 59).

Figure (see Caption) Figure 59. Thermal anomalies of varying intensities were visible in the crater of Barren Island on 31 December 2022 (top left), 15 January 2023 (top right), 24 February 2023 (bottom left), and 31 March 2023 (bottom right), as seen in these Sentinel-2 infrared satellite images. The anomalies on 31 December and 31 March were notably strong and extended to the N and N-S, respectively. Images using “Atmospheric penetration” rendering (bands 12, 11, 8a). Courtesy of Sentinel Hub Playground.

Thermal activity continued during January through March. Sentinel-2 infrared satellite data showed some thermal anomalies of varying intensity on clear weather days on 5, 10, 15, 20, and 30 January 2023, 9, 14, 19, and 24 February 2023, and 21, 26, and 31 March (figure 59). According to Suomi NPP/VIIRS sensor data, a total of 30 thermal anomalies were detected over 18 days on 2-3, 7, 9-14, 16-17, 20, 23, 25, and 28-31 January. The sensor data showed a total of six hotspots detected over six days on 1, 4-5, and 10-12 February. During March, a total of 33 hotspots were visible over 11 days on 20-31 March. Four MODVOLC thermal alerts were issued on 25, 27, and 29 March.

Geologic Background. Barren Island, a possession of India in the Andaman Sea about 135 km NE of Port Blair in the Andaman Islands, is the only historically active volcano along the N-S volcanic arc extending between Sumatra and Burma (Myanmar). It is the emergent summit of a volcano that rises from a depth of about 2250 m. The small, uninhabited 3-km-wide island contains a roughly 2-km-wide caldera with walls 250-350 m high. The caldera, which is open to the sea on the west, was created during a major explosive eruption in the late Pleistocene that produced pyroclastic-flow and -surge deposits. Historical eruptions have changed the morphology of the pyroclastic cone in the center of the caldera, and lava flows that fill much of the caldera floor have reached the sea along the western 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/); MIROVA (Middle InfraRed Observation of Volcanic Activity), a collaborative project between the Universities of Turin and Florence (Italy) supported by the Centre for Volcanic Risk of the Italian Civil Protection Department (URL: http://www.mirovaweb.it/); Hawai'i Institute of Geophysics and Planetology (HIGP) - MODVOLC Thermal Alerts System, School of Ocean and Earth Science and Technology (SOEST), Univ. of Hawai'i, 2525 Correa Road, Honolulu, HI 96822, USA (URL: http://modis.higp.hawaii.edu/); Sentinel Hub Playground (URL: https://www.sentinel-hub.com/explore/sentinel-playground); NASA Worldview (URL: https://worldview.earthdata.nasa.gov/).


Villarrica (Chile) — April 2023 Citation iconCite this Report

Villarrica

Chile

39.42°S, 71.93°W; summit elev. 2847 m

All times are local (unless otherwise noted)


Nighttime crater incandescence, ash emissions, and seismicity during October 2022-March 2023

Villarrica, located in central Chile, consists of a 2-km-wide caldera that formed about 3,500 years ago, located at the base of the presently active cone. Historical eruptions date back to 1558 and have been characterized by mild-to-moderate explosive activity with occasional lava effusions. The current eruption period began in December 2014 and has recently consisted of ongoing seismicity, gas-and-steam emissions, and thermal activity (BGVN 47:10). This report covers activity during October 2022 through March 2023 and describes Strombolian explosions, ash emissions, and crater incandescence. Information for this report primarily comes from the Southern Andes Volcano Observatory (Observatorio Volcanológico de Los Andes del Sur, OVDAS), part of Chile's National Service of Geology and Mining (Servicio Nacional de Geología y Minería, SERNAGEOMIN) and satellite data.

Seismicity during October consisted of discrete long-period (LP)-type events, tremor (TR), and volcano-tectonic (VT)-type events. Webcam images showed eruption plumes rising as high as 460 m above the crater rim; plumes deposited tephra on the E, S, and SW flanks within 500 m of the crater on 2, 18, 23, and 31 October. White gas-and-steam emissions rose 80-300 m above the crater accompanied by crater incandescence during 2-3 October. There was a total of 5 VT-type events, 10,625 LP-type events, and 2,232 TR-type events detected throughout the month. Sulfur dioxide data was obtained by the Differential Absorption Optical Spectroscopy Equipment (DOAS) installed 6 km in an ESE direction. The average value of the sulfur dioxide emissions was 535 ± 115 tons per day (t/d); the highest daily maximum was 1,273 t/d on 13 October. These values were within normal levels and were lower compared to September. During the night of 3-4 October Strombolian activity ejected blocks as far as 40 m toward the NW flank. Small, gray-brown ash pulses rose 60 m above the crater accompanied white gas-and-steam emissions that rose 40-300 m high during 4-5 October. In addition, crater incandescence and Strombolian explosions that ejected blocks were reported during 4-5 and 9-11 October. Based on satellite images from 12 October, ballistic ejecta traveled as far as 400 m and the resulting ash was deposited 3.2 km to the E and SE and 900 m to the NW.

Satellite images from 14 October showed an active lava lake that covered an area of 36 square meters in the E part of the crater floor. There was also evidence of a partial collapse (less than 300 square meters) at the inner SSW crater rim. POVI posted an 18 October photo that showed incandescence above the crater rim, noting that crater incandescence was visible during clear weather nights. In addition, webcam images at 1917 showed lava fountaining and Strombolian explosions; tourists also described seeing splashes of lava ejected from a depth of 80 m and hearing loud degassing sounds. Tephra deposits were visible around the crater rim and on the upper flanks on 24 October. On 25 October SERNAGEOMIN reported that both the number and amplitude of LP earthquakes had increased, and continuous tremor also increased; intense crater incandescence was visible in satellite images. On 31 October Strombolian explosions intensified and ejected material onto the upper flanks.

Activity during November consisted of above-baseline seismicity, including intensifying continuous tremor and an increase in the number of LP earthquakes. On 1 November a lava fountain was visible rising above the crater rim. Nighttime crater incandescence was captured in webcam images on clear weather days. Strombolian explosions ejected incandescent material on the NW and SW flanks during 1, 2, and 6-7 November. POVI reported that the width of the lava fountains that rose above the crater rim on 2 November suggested that the vent on the crater floor was roughly 6 m in diameter. Based on reports from observers and analyses of satellite imagery, material that was deposited on the upper flanks, primarily to the NW, consisted of clasts up to 20 cm in diameter. During an overflight on 19 November SERNAGEOMIN scientists observed a cone on the crater floor with an incandescent vent at its center that contained a lava lake. Deposits of ejecta were also visible on the flanks. That same day a 75-minute-long series of volcano-tectonic earthquakes was detected at 1940; a total of 21 events occurred 7.8 km ESE of the crater. Another overflight on 25 November showed the small cone on the crater floor with an incandescent lava lake at the center; the temperature of the lava lake was 1,043 °C, based data gathered during the overflight.

Similar seismicity, crater incandescence, and gas-and-steam emissions continued during December. On 1 December incandescent material was ejected 80-220 m above the crater rim. During an overflight on 6 December, intense gas-and-steam emissions from the lava lake was reported, in addition to tephra deposits on the S and SE flanks as far as 500 m from the crater. During 7-12 December seismicity increased slightly and white, low-altitude gas-and-steam emissions and crater incandescence were occasionally visible. On 24 December at 0845 SERNAGEOMIN reported an increase in Strombolian activity; explosions ejected material that generally rose 100 m above the crater, although one explosion ejected incandescent tephra as far as 400 m from the crater onto the SW flank. According to POVI, 11 explosions ejected incandescent material that affected the upper SW flank between 2225 on 25 December to 0519 on 26 December. POVI recorded 21 Strombolian explosions that ejected incandescent material onto the upper SW flank from 2200 on 28 December to 0540 on 29 December. More than 100 Strombolian explosions ejected material onto the upper W and NW flanks during 30-31 December. On 30 December at 2250 an explosion was detected that generated an eruptive column rising 120 m above the crater and ejecting incandescent material 300 m on the NW flank (figure 120). Explosions detected at 2356 on 31 December ejected material 480 m from the crater rim onto the NW flank and at 0219 material was deposited on the same flank as far as 150 m. Both explosions ejected material as high as 120 m above the crater rim.

Figure (see Caption) Figure 120. Webcam image of a Strombolian explosion at Villarrica on 30 December 2022 (local time) that ejected incandescent material 300 m onto the NW flank, accompanied by emissions and crater incandescence. Courtesy of SERNAGEOMIN (Reporte Especial de Actividad Volcanica (REAV), Region De La Araucania y Los Rios, Volcan Villarrica, 30 de diciembre de 2022, 23:55 Hora local).

During January 2023, Strombolian explosions and lava fountaining continued mainly in the crater, ejecting material 100 m above the crater. Gas-and-steam emissions rose 40-260 m above the crater and drifted in different directions, and LP-type events continued. Emissions during the night of 11 January including some ash rose 80 m above the crater and as far as 250 m NE flank. POVI scientists reported about 70 lava fountaining events from 2130 on 14 January to 0600 on 15 January. At 2211 on 15 January there was an increase in frequency of Strombolian explosions that ejected incandescent material 60-150 m above the crater. Some ashfall was detected around the crater. POVI noted that on 19 January lava was ejected as high as 140 m above the crater rim and onto the W and SW flanks. Explosion noises were heard on 19 and 22 January in areas within a radius of 10 km. During 22-23 January Strombolian explosions ejected incandescent material 60-100 m above the crater that drifted SE. A seismic event at 1204 on 27 January was accompanied by an ash plume that rose 220 m above the crater and drifted E (figure 121); later that same day at 2102 an ash plume rose 180 m above the crater and drifted E.

Figure (see Caption) Figure 121. Webcam image of an ash plume at Villarrica on 27 January rising 220 m above the crater and drifting E. Courtesy of SERNAGEOMIN (Reporte Especial de Actividad Volcanica (REAV), Region De La Araucania y Los Rios, Volcan Villarrica, 27 de enero de 2023, 12:35 Hora local).

Seismicity, primarily characterized by LP-type events, and Strombolian explosions persisted during February and March. POVI reported that three explosions were heard during 1940-1942 on 6 February, and spatter was seen rising 30 m above the crater rim hours later. On 9 February lava fountains were visible rising 50 m above the crater rim. On 17 February Strombolian explosions ejected material 100 m above the crater rim and onto the upper SW flank. Webcam images from 20 February showed two separate fountains of incandescent material, which suggested that a second vent had opened to the E of the first vent. Spatter was ejected as high as 80 m above the crater rim and onto the upper NE flank. A sequence of Strombolian explosions was visible from 2030 on 20 February to 0630 on 21 February. Material was ejected as high as 80 m above the crater rim and onto the upper E flank. LP-type earthquakes recorded 1056 and at 1301 on 27 February were associated with ash plumes that rose 300 m above the crater and drifted NE (figure 122). Crater incandescence above the crater rim was observed in webcam images on 13 March, which indicated Strombolian activity. POVI posted a webcam image from 2227 on 18 March showing Strombolian explosions that ejected material as high as 100 m above the crater rim. Explosions were heard up to 8 km away. On 19 March at 1921 an ash emission rose 340 m above the crater and drifted NE. On 21 and 26 March Strombolian explosions ejected material 100 and 110 m above the crater rim, respectively. On 21 March Strombolian explosions ejected material 100 m above the crater rim. Low-intensity nighttime crater incandescence was detected by surveillance cameras on 24 March.

Figure (see Caption) Figure 122. Photo of an ash plume rising 300 m above the crater of Villarrica and drifting NE on 27 February 2023. Courtesy of SERNAGEOMIN (Reporte Especial de Actividad Volcanica (REAV), Region De La Araucania y Los Rios, Volcan Villarrica, 27 de febrero de 2023, 11:10 Hora local).

Infrared MODIS satellite data processed by MIROVA (Middle InfraRed Observation of Volcanic Activity) detected an increase in thermal activity during mid-November, which corresponds to sustained Strombolian explosions, lava fountaining, and crater incandescence (figure 123). This activity was also consistently captured on clear weather days throughout the reporting period in Sentinel-2 infrared satellite images (figure 124).

Figure (see Caption) Figure 123. Low-power thermal anomalies were detected during August through October 2022 at Villarrica, based on this MIROVA graph (Log Radiative Power). During mid-November, the power and frequency of the anomalies increased and remained at a consistent level through March 2023. Thermal activity consisted of Strombolian explosions, lava fountains, and crater incandescence. Courtesy of MIROVA.
Figure (see Caption) Figure 124. Consistent bright thermal anomalies were visible at the summit crater of Villarrica in Sentinel-2 infrared satellite images throughout the reporting period, as shown here on 19 December 2022 (left) and 9 February 2023 (right). Occasional gas-and-steam emissions also accompanied the thermal activity. Images use Atmospheric penetration rendering (bands 12, 11, 8a). Courtesy of Sentinel Hub Playground.

Geologic Background. The glacier-covered Villarrica stratovolcano, in the northern Lakes District of central Chile, is ~15 km south of the city of Pucon. A 2-km-wide caldera that formed about 3,500 years ago is located at the base of the presently active, dominantly basaltic to basaltic-andesite cone at the NW margin of a 6-km-wide Pleistocene caldera. More than 30 scoria cones and fissure vents are present on the flanks. Plinian eruptions and pyroclastic flows that have extended up to 20 km from the volcano were produced during the Holocene. Lava flows up to 18 km long have issued from summit and flank vents. Eruptions documented since 1558 CE have consisted largely of mild-to-moderate explosive activity with occasional lava effusion. Glaciers cover 40 km2 of the volcano, and lahars have damaged towns on its flanks.

Information Contacts: Servicio Nacional de Geología y Minería (SERNAGEOMIN), Observatorio Volcanológico de Los Andes del Sur (OVDAS), Avda Sta María No. 0104, Santiago, Chile (URL: http://www.sernageomin.cl/); Proyecto Observación Villarrica Internet (POVI) (URL: http://www.povi.cl/); MIROVA (Middle InfraRed Observation of Volcanic Activity), a collaborative project between the Universities of Turin and Florence (Italy) supported by the Centre for Volcanic Risk of the Italian Civil Protection Department (URL: http://www.mirovaweb.it/); Sentinel Hub Playground (URL: https://www.sentinel-hub.com/explore/sentinel-playground).


Fuego (Guatemala) — April 2023 Citation iconCite this Report

Fuego

Guatemala

14.473°N, 90.88°W; summit elev. 3763 m

All times are local (unless otherwise noted)


Daily explosions, gas-and-ash plumes, avalanches, and ashfall during December 2022-March 2023

Fuego, one of three large stratovolcanoes overlooking the city of Antigua, Guatemala, has been vigorously erupting since January 2002, with recorded eruptions dating back to 1531 CE. Eruptive activity has included major ashfalls, pyroclastic flows, lava flows, and lahars. Frequent explosions with ash emissions, block avalanches, and lava flows have persisted since 2018. More recently, activity remained relatively consistent with daily explosions, ash plumes, ashfall, avalanches, and lahars (BGVN 48:03). This report covers similar activity during December 2022 through March 2023, based on information from the Instituto Nacional de Sismologia, Vulcanología, Meteorología e Hidrologia (INSIVUMEH) daily reports, Coordinadora Nacional para la Reducción de Desastres (CONRED) newsletters, and various satellite data.

Daily explosions reported throughout December 2022-March 2023 generated ash plumes to 6 km altitude that drifted as far as 60 km in multiple directions. The explosions also caused rumbling sounds of varying intensities, with shock waves that vibrated the roofs and windows of homes near the volcano. Incandescent pulses of material rose 100-500 m above the crater, which caused block avalanches around the crater and toward the Santa Teresa, Taniluyá (SW), Ceniza (SSW), El Jute, Honda, Las Lajas (SE), Seca (W), and Trinidad (S) drainages. Fine ashfall was also frequently reported in nearby communities (table 27). MIROVA (Middle InfraRed Observation of Volcanic Activity) analysis of MODIS satellite data showed frequent, moderate thermal activity throughout the reporting period; however, there was a brief decline in both power and frequency during late-to-mid-January 2023 (figure 166). A total of 79 MODVOLC thermal alerts were issued: 16 during December 2022, 17 during January 2023, 23 during February, and 23 during March. Some of these thermal evets were also visible in Sentinel-2 infrared satellite imagery at the summit crater, which also showed occasional incandescent block avalanches descending the S, W, and NW flanks, and accompanying ash plumes that drifted W (figure 167).

Table 27. Activity at Fuego during December 2022 through March 2023 included multiple explosions every hour. Ash emissions rose as high as 6 km altitude and drifted generally W and SW as far as 60 km, causing ashfall in many communities around the volcano. Data from daily INSIVUMEH reports and CONRED newsletters.

Month Explosions per hour Ash plume altitude (max) Ash plume distance (km) and direction Drainages affected by block avalanches Communities reporting ashfall
Dec 2022 1-12 6 km WSW, W, SW, NW, S, SE, NE, and E, 10-30 km Santa Teresa, Taniluyá, Ceniza, El Jute, Honda, Las Lajas, Seca, and Trinidad Panimaché I and II, Morelia, Santa Sofía, El Porvenir, Finca Palo Verde, Yepocapa, Yucales, Sangre de Cristo, La Rochela, Ceilán, San Andrés Osuna, and Aldea La Cruz
Jan 2023 1-12 5 km W, SW, NW, S, N, NE, E, and SE, 7-60 km Ceniza, Las Lajas, Santa Teresa, Taniluyá, Trinidad, Seca, Honda, and El Jute Panimaché I and II, Morelia, Santa Sofía, El Porvenir, Palo Verde, Yucales, Yepocapa, Sangre de Cristo, La Rochela, Ceylon, Alotenango, and San Andrés Osuna
Feb 2023 1-12 4.9 km SW, W, NW, and N, 10-30 km Santa Teresa, Taniluyá, Ceniza, Las Lajas, Seca, Trinidad, El Jute, and Honda Panimaché I and II, Morelia, Santa Sofía, Palo Verde, San Pedro Yepocapa, El Porvenir, Sangre de Cristo, La Soledad, Acatenango, El Campamento, and La Asunción
Mar 2023 3-11 5 km W, SW, NW, NE, N, S, SE, and E, 10-30 km Seca, Ceniza, Taniluyá, Las Lajas, Honda, Trinidad, El Jute, and Santa Teresa Yepocapa, Sangre de Cristo, Panimaché I and II, Morelia, Santa Sofía, El Porvenir, La Asunción, Palo Verde, La Rochela, San Andrés Osuna, Ceilán, and Aldeas
Figure (see Caption) Figure 166. Thermal activity at Fuego shown in the MIROVA graph (Log Radiative Power) was at moderate levels during a majority of December 2022 through March 2023, with a brief decline in both power and frequency during late-to-mid-January 2023. Courtesy of MIROVA.
Figure (see Caption) Figure 167. Frequent incandescent block avalanches descended multiple drainages at Fuego during December 2022 through March 2023, as shown in these Sentinel-2 infrared satellite images on 10 December 2022 (top left), 4 January 2023 (top right), 18 February 2023 (bottom left), and 30 March 2023 (bottom right). Gray ash plumes were also occasionally visible rising above the summit crater and drifting W, as seen on 4 January and 30 March. Avalanches affected the NW and S flanks on 10 December, the SW and W flanks on 18 February, and the NW, W, and SW flanks on 30 March. Images use Atmospheric penetration rendering (bands 12, 11, 8a). Courtesy of Sentinel Hub Playground.

Daily explosions ranged between 1 and 12 per hour during December 2022, generating ash plumes that rose to 4.5-6 km altitude and drifted 10-30 km in multiple directions. These explosions created rumbling sounds with a shock wave that vibrated the roofs and windows of homes near the volcano. Frequent white gas-and-steam plumes rose to 4.6 km altitude. Strombolian activity resulted in incandescent pulses that generally rose 100-500 m above the crater, which generated weak-to-moderate avalanches around the crater and toward the Santa Teresa, Taniluyá, Ceniza, El Jute, Honda, Las Lajas, Seca, and Trinidad drainages, where material sometimes reached vegetation. Fine ashfall was recorded in Panimaché I and II (8 km SW), Morelia (9 km SW), Santa Sofía (12 km SW), El Porvenir (8 km ENE), Finca Palo Verde, Yepocapa (8 km NW), Yucales (12 km SW), Sangre de Cristo (8 km WSW), La Rochela, Ceilán, San Andrés Osuna, and Aldea La Cruz. INSIVUMEH reported that on 10 December a lava flow formed in the Ceniza drainage and measured 800 m long; it remained active at least through 12 December and block avalanches were reported at the front of the flow. A pyroclastic flow was reported at 1100 on 10 December, descending the Las Lajas drainage for several kilometers and reaching the base of the volcano. Pyroclastic flows were also observed in the Ceniza drainage for several kilometers, reaching the base of the volcano on 11 December. Ash plumes rose as high as 6 km altitude, according to a special bulletin from INSIVUMEH. On 31 December explosions produced incandescent pulses that rose 300 m above the crater, which covered the upper part of the cone.

Activity during January 2023 consisted of 1-12 daily explosions, which produced ash plumes that rose to 4.2-5 km altitude and drifted 7-60 km in multiple directions (figure 168). Incandescent pulses of material were observed 100-350 m above the crater, which generated avalanches around the crater and down the Ceniza, Las Lajas, Santa Teresa, Taniluyá, Trinidad, Seca, Honda, and El Jute drainages. Sometimes, the avalanches resuspended older fine material 100-500 m above the surface that drifted W and SW. Ashfall was recorded in Panimaché I and II, Morelia, Santa Sofía, El Porvenir, Palo Verde, Yucales, Yepocapa, Sangre de Cristo, La Rochela, Ceylon, Alotenango, and San Andrés Osuna. Intermittent white gas-and-steam plumes rose to 4.5 km altitude and drifted W and NW.

Figure (see Caption) Figure 168. Webcam image showing an ash plume rising above Fuego on 15 January 2023. Courtesy of INSIVUMEH.

There were 1-12 daily explosions recorded through February, which generated ash plumes that rose to 4.2-4.9 km altitude and drifted 10-30 km SW, W, NW, and N. Intermittent white gas-and-steam emissions rose 4.5 km altitude and drifted W and SW. During the nights and early mornings, incandescent pulses were observed 100-400 m above the crater. Weak-to-moderate avalanches were also observed down the Santa Teresa, Taniluyá, Ceniza, Las Lajas, Seca, Trinidad, El Jute, and Honda drainages, sometimes reaching the edge of vegetated areas. Occasional ashfall was reported in Panimaché I and II, Morelia, Santa Sofía, Palo Verde, San Pedro Yepocapa, El Porvenir, Sangre de Cristo, La Soledad, Acatenango, El Campamento, and La Asunción. On 18 February strong winds resuspended previous ash deposits as high as 1 km above the surface that blew 12 km SW and S.

During March, daily explosions ranged from 3-11 per hour, producing ash plumes that rose to 4-5 km altitude and drifted 10-30 km W, SW, NW, NE, N, S, SE, and E. During the night and early morning, crater incandescence (figure 169) and incandescent pulses of material were observed 50-400 m above the crater. Weak-to-moderate avalanches affected the Seca, Ceniza, Taniluyá, Las Lajas, Honda, Trinidad, El Jute, and Santa Teresa drainages, sometimes reaching the edge of vegetation. Frequent ashfall was detected in Yepocapa, Sangre de Cristo, Panimaché I and II, Morelia, Santa Sofía, El Porvenir, La Asunción, Palo Verde, La Rochela, San Andrés Osuna, Ceilán, and Aldeas. Weak ashfall was recorded in San Andrés Osuna, La Rochela, Ceylon during 8-9 March. A lahar was reported in the Ceniza drainage on 15 March, carrying fine, hot volcanic material, tree branches, trunks, and blocks from 30 cm to 1.5 m in diameter. On 18 March lahars were observed in the Las Lajas and El Jute drainages, carrying fine volcanic material, tree branches and trunks, and blocks from 30 cm to 1.5 m in diameter. As a result, there was also damage to the road infrastructure between El Rodeo and El Zapote.

Figure (see Caption) Figure 169. Sentinel-2 infrared satellite image showing Fuego’s crater incandescence accompanied by a gas-and-ash plume that drifted SW on 25 March 2023. Images use bands 12, 11, 5. Courtesy of INSIVUMEH.

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: 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/); Sentinel Hub Playground (URL: https://www.sentinel-hub.com/explore/sentinel-playground).

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Bulletin of the Global Volcanism Network - Volume 37, Number 09 (September 2012)

Managing Editor: Richard Wunderman

Bandaisan (Japan)

Mild, 45-second volcanic tremor in June 2012

Esan (Japan)

Minor steam plumes in March 2012

Havre Seamount (New Zealand)

Source of large pumice rafts traced to Havre seamount eruption

Popocatepetl (Mexico)

Intermittent ash plumes and diminished seismicity during July-October 2012

Purace (Colombia)

Expanded monitoring efforts and persistent seismicity in 2012

Sotara (Colombia)

Monitoring efforts and recent seismic unrest



Bandaisan (Japan) — September 2012 Citation iconCite this Report

Bandaisan

Japan

37.601°N, 140.072°E; summit elev. 1816 m

All times are local (unless otherwise noted)


Mild, 45-second volcanic tremor in June 2012

Our previous report on Bandai (also called Bandai-san) discussed a significant increase in seismicity during 14-16 August 2000 (BGVN 25:08). However, no eruption resulted and no large change in GPS data was noted. The volcano is located in Fukushima Prefecture, Japan, about 220 km N of Tokyo (figure 2). This report notes that volcanic tremor was recorded in June 2012.

Figure (see Caption) Figure 2. A map of the major volcanoes of Japan. Bandai is just N of Tokyo. Courtesy of the U.S. Geological Survey.

Recent monthly reports of volcanic activity from the Japan Meteorological Agency (JMA), translated into English, resumed in October 2010; the only recent report on Bandai was in June 2012. Thus, in this report, we lack JMA reports between January 2005 and May 2012 and only summarize activity during June 2012.

According to JMA, on 25 June 2012 volcanic tremor with a duration of 45 seconds was recorded, the first since 9 June 2009. No change in volcanic earthquakes, ground deformation, or fumarolic activity was observed. Volcanic earthquakes have remained at a low level at least through September 2012. A camera located at Kengamine (~7 km N of the summit) showed that gas emissions remained low, rising less than 100 m in height.

Geologic Background. One of Japan's most noted volcanoes, Bandaisan rises above the north shore of Lake Inawashiro. This complex is formed of several overlapping andesitic stratovolcanoes, the largest of which is Obandai. Kobandaisan peak, which collapsed in 1888, was formed about 50,000 years ago. Obandai was constructed about 40,000 years ago after a Plinian eruption resulted in the collapse of an older edifice and the Okinajima debris avalanche to the SW. The last magmatic eruption took place more than 25,000 years ago, but four major phreatic eruptions have occurred during the past 5,000 years, most recently in 806 and 1888 CE. Seen from the south, Bandaisan presents a conical profile, but much of the north side of the volcano is missing as a result of the collapse of Kobandaisan during the 1888 eruption, causing a debris avalanche that buried several villages and formed several large lakes.

Information Contacts: Japan Meteorological Agency (JMA), Otemachi, 1-3-4, Chiyoda-ku Tokyo 100-8122, Japan (URL: http://www.jma.go.jp/).


Esan (Japan) — September 2012 Citation iconCite this Report

Esan

Japan

41.805°N, 141.166°E; summit elev. 618 m

All times are local (unless otherwise noted)


Minor steam plumes in March 2012

E-san is located in S Hokkaido, the northernmost of Japan's 47 prefectures (figure 1). Recent monthly reports of volcanic activity from the Japan Meteorological Agency (JMA), translated into English, resumed in October 2010. The only recent JMA report on E-san was in March 2012. This is the first BGVN report discussing E-san.

Figure (see Caption) Figure 1. A map showing a few of the major volcanoes of Japan, with their respective Alert Levels in March 2012. E-san is in the northernmost prefecture of Japan, Hokkaido. Courtesy of JMA.

According to JMA, in March 2012 steam plumes rose to heights of less than 100 m above the crater rim. Aerial visual and infrared observations coducted in cooperation with Japan's Ministry of Land, Infrastructure, Transportation, and Tourism, and the Japan Coast Guard on 16 and 23 March, repectively, found no changes.

A small-amplitude and short-duration volcanic tremor occurred on 30 March. After that, the number of small volcanic earthquakes increased until early on 31 March. No steam plumes could be observed on 31 March due to cloud cover; however, JMA reported no change in air vibrations or crustal deformation data. Field surveys on 2 April found no change in either the steam plumes from the crater or crustal deformation (GPS).

Geologic Background. Esan is a small volcanic complex of seven overlapping andesitic-to-dacitic lava domes on the eastern tip of the Oshima Peninsula across the Tsugaru Strait from Honshu. The complex consists of five late Pleistocene and two early Holocene lava domes, Esan and Misaki. A minor phreatic eruption in 1846 produced a mudflow that caused many fatalities. The latest activity was a small eruption in 1874. Active fumaroles occur at a thermal area on the upper NW flank.

Information Contacts: Japan Meteorological Agency (JMA), Otemachi, 1-3-4, Chiyoda-ku Tokyo 100-8122, Japan (URL: http://www.jma.go.jp/).


Havre Seamount (New Zealand) — September 2012 Citation iconCite this Report

Havre Seamount

New Zealand

31.08°S, 179.033°W; summit elev. -897 m

All times are local (unless otherwise noted)


Source of large pumice rafts traced to Havre seamount eruption

Large pumice rafts observed floating in the SW Pacific Ocean in the central Kemadec Islands, midway between North Island (New Zealand) and Tonga, have been traced by various investigators and monitoring systems to a mid-July 2012 eruption of the Havre submarine seamount (figure 1). The eruption was strong enough to result in thermal alerts and produce an ash plume that breached the ocean surface from a depth of at least 700 m.

Figure (see Caption) Figure 1. Map showing New Zealand and its territory that is associated with subduction along the Kermadec-Tonga trench system. A scale and key for features are shown in the bottom left. To the NNE reside the Kermadec chain of islands and associated rocks and seamounts (submarine volcanoes, closed triangles). Havre seamount, Havre Rock, and L'Esperance Rock appear in the central part of the Kermadecs. The insert in the lower right-hand corner shows the location of the map with respect to the S Pacific Ocean. The Kermadec Islands Marine Reserve is New Zealand's largest marine reserve, covering 7,450 km2 (Gardner and others, 2006). The areas of the marine reserve (gray circles), extend 22.2 km (12 nautical miles, nmi) out to the edge of the territorial sea from the cliffs and boulder beaches of various Kermadec Islands and rocks (Raoul and adjacent islands; Macauley, Curtis, and adjacent islands; and L'Esperance and Havre Rocks). The New Zealand Exclusive Economic Zone, prescribed under the 1982 United Nations Convention of the Law of the Sea, covers the areas within red arcs at a distance of ~370 km (200 nmi) from shorelines of the two major New Zealand islands and its smaller territorial islands. Courtesy of Pew Environment Group.

Early observations. Maggie de Grauw, resident of Paeroa, New Zealand, took photographs (one of which is shown in figure 2) on 31 July 2012, from a commercial airplane (Virgin Pacific flight ##DJ94 from Apia, Samoa to Auckland, New Zealand) of a "peculiar large mass floating on the ocean between Tonga and Auckland."

Figure (see Caption) Figure 2. Pumice raft photographed at 1440 on 31 July 2012 NZST between Tonga and Auckland, NZ. The rainbow effect is the result of the combination of a standard polarizer on the camera lens and the airplane window. Courtesy of Maggie de Grauw.

She noted that there was another larger mass nearby, but was unable to photograph it because of the difficult angle. Believing it to be a pumice raft, she emailed the photos to Scott Bryan, author of an article on pumice rafts (Bryan and others, 2012), who forwarded it to Bulletin staff.

de Grauw noted that "the date stamp on the photograph says 1441 NZST [New Zealand standard time], which meant we had another 1 hour and 15 minutes flying time to Auckland. Total flight time was estimated at 3 and a half to 4 hours. Looking at the map, that would have put us some where near the Kermadec trench/ridge or islands. (Though I did not see any islands nearby)."

On 4 August, Bryan commented that the source of the pumice, if in the Kermadecs, may be Raoul, Macauley, Giggenbach, or Volcano W. He suggested that Monowai seamount seemed too far away. Brad Scott, New Zealand's GNS Science, noted that around the same time North Island of New Zealand had two volcanoes erupting (Tongariro and White Island) and seismic signals indicated that Monowai seamount (in the Kermadec Islands) was erupting as well.

On 10 August 2012, the New Zealand Defence Force (NZDF) reported an area of floating pumice in the open ocean. The area where the pumice was abundant was 463 km (250 nmi) in length and 56 km (30 nmi) wide, for a total area of 25,700 km2 (7,500 nmi2). A photograph taken on 9 August 2012 shows an example of the pumice as seen from a Royal New Zealand Air Force (RNZAF) Orion patrol plane flying between Samoa and New Zealand (figure 3); video of the raft from this aircraft was shown in a press release from NZDF (2012).

Figure (see Caption) Figure 3. Pumice raft photographed by a Royal New Zealand Air Force (RNZAF) Orion patrol plane flying between Samoa and New Zealand (9 August 2012). Courtesy of NZDF.

The pilots relayed the information to the Royal New Zealand Navy vessel HMNZS Canterbury, which later that day encountered floating pumice ~160 km (85 nmi) WSW of Raoul island (29.27°S, 177.92°W). The Canterbury crew found that the pumice raft was ~0.6 m thick, 1 km wide, and extended to their right and left as far as the eye could see. The crew retrieved some pieces of pumice from the ship's water filters for later analysis and documentation. According to a news article by Priestley (2012) other samples of pumice were collected using buckets. These samples ranged from golf ball to soccer ball sized (figures 4 and 5). The pumice samples were "rough around the edges and irregular shapes." At that time, the origin of the pumice was still unknown.

Figure (see Caption) Figure 4. A handfull of pumice pebbles from a pumice raft, recovered from water filters of HMNZS Canterbury. From Priestley (2012).
Figure (see Caption) Figure 5. Large piece of pumice collected by the HMNZS Canterbury on 10 August 2012. From Priestley (2012).

In addition, Alain Bernard of the Laboratoire de Volcanologie, Université Libre de Bruxelles, Belgium, and Olivier Hyvernaud of the Laboratoire de Géophysique, Tahiti, observed the pumice raft in MODIS/Terra satellite images taken 3 August 2012.

Search for the pumice source. The search for the pumice source involved a number of investigators and their institutions, and several monitoring systems. Table 1 gives a summary of locations of the pumice source based on various observed phenomena associated with the July 2012 eruption as determined from various investigators.

Table 1. Summary of reported locations for events and features associated with tracking the source of the pumice rafts from the July 2012 eruption of Havre seamount. These locations may be compared with the location of Havre seamount (table 2) from Wright, Worthington and Gamble (2006). Compiled from listed references.

Source - Feature Coordinates (as reported) Coordinates (decimal degrees) Dates and comments Reference(s)
Seismic - source of pumice raft 31.13°S, 178.96°W 31.13°S, 178.96°W 17-18 July 2012, short seismic swarm Hyvernaud (2012), Laboratoire de Géophysique, Papeete, Polynesian Network (Scott, 2012)
MODIS satellite - hot spot 31°7'S, 179°12'W 31.1°S, 179.2°W 1050 on 18 July 2012 UTC; band 22, 3.959 µm Bernard (2012)
MODIS satellite - point of vapor plume 31°5'S, 179°1'W 31.1°S, 179.0°W 2150 on 18 July 2012 UTC; band 20, 3.75 µm; plume image "pointing to the source of the eruption" Bernard (2012)
Satellite - source of pumice 30.95°S, 179.13°W 30.95°S, 179.13°W 19 July 2012 UTC, satellite data, raft becomes visible after 0205 Laboratoire de Géophysique, Papeete, Polynesian Network (Scott, 2012)

Table 2. Locations of Havre seamount and other nearby features, for comparison with early locations of pumice rafts' source vent (table 1). Compiled from listed references.

Feature Coordinates (as reported) Coordinates (decimal degrees) Comments Reference(s)
Havre Seamount 31°6.500'S, 179°2.450'W 31.11°S, 179.04°W Summit depth 720 m, basal depth 1,750 m; used in this report and by Klemetti (2012a). Wright, Worthington, and Gamble (2006)
Havre Rock 31°17.3'S, 178°54.7'W 31.29°S, 178.9°W Summit elevation ~70 m. New Zealand Land Information (2008)
L'Esperance Rock 31°21.4'S, 178°48.4'W 31.36°S, 178.82°W Summit slightly above sea level. New Zealand Land Information (2008)

GNS Science issued a news bulletin on 11 August 2012 (Scott, 2012) noting that a report from the Laboratoire de Géophysique, Tahiti, confirmed two indications of eruptive activity in the Kermadec Islands, one from satellite tracking and another from seismic monitoring.

An examination of satellite data by the Laboratoire de Géophysique traced the pumice back to a source at 30.95°S, 179.13°W, 72 km SW of Curtis Island at 0205 on 19 July 2012 UTC. According to Olivier Hyvernaud (2012), between 0733 on 17 July 2012 UTC and 0300 on 18 July 2012 UTC, 157 hydroacoustic events from Kermadec ridge were measured. He noted that "the waveforms are all very similar, with a short length and a steep rise. For some events, seismic Rayleigh and Pn phases from regional seismic stations were associated." Among the 157 events of magnitudes between 3.0 and 4.8, 68 events were located (figures 6 and 7).

Figure (see Caption) Figure 6. Cumulative number of hydroacoustic events recorded by the Laboratoire de Géophysique for the period 0800 on 17 July 2012 UTC through 0900 on 18 July 2012 UTC. Courtesy of Olivier Hyvernaud.
Figure (see Caption) Figure 7. Locations in the Kermadec Islands from events having both seismic and hydroacoustic phases (red spots for epicenters and red error ellipses) and from events having only hydroacoustic phases (green dots for epicenters and green error ellipses) during the period from 0733 on 17 July 2012 UTC to 0300 on 18 July 2012 UTC. Havre seamount volcano (labeled 'Volcano') is located by a plus sign (+). Courtesy of Olivier Hyvernaud.

According to Hyvernaud, the "mean location is at 31.13°S, 178.96°W, a position in the vicinity of Havre seamount. The best locations are obtained with a mix of hydroacoustic and seismic phases. The focal depths are impossible to constrain, but we assume that they are shallow. Usually, we record several types of hydroacoustic events during volcanic submarine activity: submarine explosions, tremors and small earthquakes. Submarine explosions and tremors are never recorded in seismic [data] (unless you have a very close seismic station). For Havre, the strongest events have both seismic and hydroacoustic [signals], that's why I interpret them as small earthquakes. The weakest have only hydroacoustic phase[s], because seismic phases are below the detection threshold. Tremors and explosions have not been recorded for Havre: why?, I don't know...Perhaps the explosive sources are on the opposite side of the volcano and couldn't propagate towards French Polynesia?..."

Alain Bernard sent an email to the Bulletin reporting that he had analyzed nighttime imagery from a MODIS satellite and found a thermal hot spot from the eruption at 1050 on 18 July 2012 UTC, the earliest evidence of a hot spot from the Havre Seamount eruption reaching the ocean surface (figure 8a). He noted that "apparently, the first appearance of pumice rafting is on MODIS/Terra [satellite images] of July 18 [2012]...There is an intriguing feature associated with the raft, it looks like a plume of vapour(?) with a clear thermal contrast as seen in band 20 at 3.75µm [figure 8b]. I really don't know what this could be and if this feature is pointing to the source of the eruption. Anyway, the geographic location is close to 31°5'S and 179°1'W but as far as I know there is no identified submarine volcano there."

Figure (see Caption) Figure 8. (A) First appearance of thermal hot spot from MODIS/Terra satellite (band 22; 3.959 µm) at 1050 on 18 July 2012 UTC, showing a cold airborne eruptive plume (dark color) drifting toward the NW from a hot spot (2 white pixels, circled). The hot spot location was 31°7'S, 179°12'W. Sea surface temperatures were around 22-23°C for the hot pixels, with an average sea temperature around 17-18°C; pixels are 1 km2. (B) Brightness temperature image from MODIS/Terra satellite (band 20; 3.75 µm) at 2150 on 18 July 2012 UTC, showing white plume whose source appears to be located at 31°5'S, 179°1'W. Courtesy of Bernard (2012).

Havre identified as pumice source. According to a report by Erik Klemetti (2012), he and Robert Simmon, both working independently of GNS Science and using NASA's Moderate Resolution Imaging Spectroradiometer (MODIS) Terra and Aqua images, discovered the first signs of the eruption (discolored water, gray pumice, and a volcanic plume) in imagery from 0950 and 1410 on 19 July 2012 (local time) between Macauley Island and Volcano W. NASA satellite images acquired during 18-21 July 2012 show an obvious plume on both 18 and 19 July, then only the pumice raft on 20 July, suggesting the eruption may have only lasted a couple of days (figure 9). The eruption was strong enough to generate a thermal pulse from a depth of at least 700 m that could be measured at the ocean surface by satellite (figure 8a).

Figure (see Caption) Figure 9. (A) MODIS/Terra satellite imagery taken at 2150 on 18 July 2012 UTC. Site of the eruption is hidden by clouds, but a plume, pumice, and discolored water are clearly visible. (B) MODIS/Terra satellite image taken at 2220 on 21 July 2012 UTC. (C) MODIS/Terra satellite image taken at 2220 on 30 July 2012 UTC. Courtesy of NASA Earth Observatory.

To identify known features on the sea floor that might correspond to the source vent for the pumice, Klemetti overlaid the MODIS/Terra image on Google Earth to find the location relative to Macauley volcano and Volcano W. Bathymetric maps indicated that the source of the plume appeared to be a U-shaped edifice that had no label in the Smithsonian's Global Volcanism Program Google Earth layer. However, from a map of the Kermadec Islands (Smith and Price, 2006), it appeared that the edifice was Havre seamount (near Havre Rock), a relatively unknown seamount volcano without documented eruptive history.

Klemetti concluded his report saying that this event "shows how easily an eruption can happen in the middle of the ocean and not be noticed for 3 weeks - even in the 21st century!... Most eruptions will be noticed either as heat spots or sources of sulfur dioxide emissions if not visually on these satellite images. However, sometimes we get the evidence of an eruption well after it happened and have to backtrack through remote sensing data to find the source and in the case of Havre, this was the only way that the source could be found so quickly."

By 21 July 2012, the eruption appeared to have waned, leaving behind rafts of pumice. Winds and currents spread the pumice into a series of twisted filaments, spread over an area of ~450 by 250 km as of 13 August. A 31 August 2012 issue of New Zealand Notices to Mariners (New Zealand Land Information, 2012) announced a recent insertion, "Volcanic Activity," to Chart NZ 222 (SW Pacific - Kermadec Islands; New Zealand Land Information, 2008) at a position 30°57.00'S, 179°07.80'W (figure 10). This location is identical to the location for the source of the ash plume as identified from satellite images by the Laboratoire de Géophysique.

Figure (see Caption) Figure 10. Portion of Chart NZ 222 showing the location of Havre Rock, L'Esperance Rock, and, in the upper left, the recently inserted location at 30.95°S, 179.13°W, labeled "Volcanic Activity (2012)," an early location for the eruption site. From New Zealand Land Information (2008, 2012).

Fate of pumice rafts. According to Bernard, Hyvernaud, Klemetti, and Simmon, satellite images revealed that Havre seamount erupted a tightly-packed raft of floating pumice on 19 and 20 July 2012. Over several weeks, wind and waves dispersed the pumice to the W, NW, N, and then E. A 28 July image showed one pumice raft, twisted by ocean currents, appearing as a well-defined strand (figure 11). By 6 August, the pumice was largely dispersed, spread over an area at least 450 km wide (figure 12a). Filaments of pumice remained in the area on 13 August, and the pumice was spread over an area of ~450 by 258 km (figure 12b). None appeared to reach Raoul Island, site of a permanently staffed meteorological station.

Figure (see Caption) Figure 11. This satellite image taken on 28 July 2012 shows the pumice floating in cuniform elongate rafts over a wide area of the sea to the NW and NE of Havre seamount. The natural-color image was acquired by the MODIS/Aqua satellite. Courtesy of NASA Earth Observatory; image courtesy of Jeff Schmaltz; caption by Robert Simmon.
Figure (see Caption) Figure 12. (A) By 6 August, the pumice was largely dispersed, spread over an area at least 450 km wide. (B) Filaments of pumice remained in the area on 13 August. These natural-color satellite images were acquired by the MODIS/Terra satellite. Courtesy of NASA Earth Observatory; image courtesy of Jeff Schmaltz; caption by Robert Simmon.

The NASA Earth Observatory continued tracking the spread of the pumice from the Havre eruption. By 19 August 2012 the pumice was spread over an area of 270,000 km2 of the Pacific Ocean and was continuing to spread. This pumice will likely stay afloat for months if not longer and eventually make landfall wherever the currents dictate - potentially as far away as South America.

According to GNS, the crew on a flight between Auckland and Apia on 1 October 2012 reported "floating pumice in the Kermadec Islands NE of New Zealand. The GeoNet duty volcanologist received this from the MetService Aviation Forecaster as part of the routine exchange of volcano data and observations between the organisations and airline pilots." "It is most likely this pumice raft is the same one [generated in mid-July 2012 and attributed to Havre as a source], just more spread out now. We have no direct evidence that Havre has erupted again."

The fate of the Havre pumice is unknown at this time, but a recent study by Scott Bryan and others (2012) details what happened to pumice from the 2006 Home Reef eruption in Tonga (see BGVN 31:09, 31:10, 31:12, 32:04, 33:05, and 33:12). That 2006 eruption (VEI 2 where the main vent was likely tens of meters below the ocean surface) was strong enough to create an ash plume that likely reached as high as 15 km altitude at its maximum, and did produce a small island that might have been as high as 75 m above sea level (wave action quickly removed the tephra forming the island). For the Home Reef eruption, the drifting pumice quickly hosted upwards of 80 different species of marine life over the course of its journey. Pumice rafts might be one of the ways that the ocean can redistribute organisms throughout the world oceans. Within eight months of the eruption, some of the pumice clasts had traveled over 5,000 km. Many clasts stayed afloat for ~2 years (Bryan and others 2012).

October 2012 cruise confirms Havre as pumice source. On 26 October 2012 the New Zealand National Institute of Water and Atmospheric Research's (NIWA) Research Vessel Tangaroa mapped Havre submarine volcano. NIWA ocean geology scientist Joshu Mountjoy announced finding a new volcanic cone which has formed on the edge of the volcano, towering 240 m above the crater rim that was first mapped in 2002 (Wright and others, 2006). The 2012 Havre eruption was strong enough to breach the ocean surface from a depth of more than 700 m by producing an ash plume, thermal alert, and a pumice raft that covered an area of 22,000 km2, all visible by satellite.

According to a press release from NIWA (2012), the voyage leader, NIWA's volcanologist Richard Wysoczanski, said that "we know the shape of the volcano from previous research. Using the multibeam echosounder, we made a before and after comparison of the volcano to determine the size of the eruption and the change it has made to the seafloor." NIWA previously mapped Havre volcano in 2002 (Wright and others, 2006), showing a 1-km-high undersea mountain with a 5-km-wide, 800-m-deep central crater. This central steep-walled crater is a caldera, which is a collapse feature of volcanoes, like Lake Taupo, often known to produce large and violent eruptions.

Mountjoy noted that "One side of the caldera wall is bulging in towards the volcano's centre. The bulging may indicate where an eruption may occur in the future, or it might lead to an undersea avalanche." Several cubic kilometers of new material had been added to the volcano. Large volumes of freshly erupted pumice have accumulated on the caldera floor, raising the floor by up to 10 m. Glassy volcanic rocks were sampled from the fresh crater wall, typical of newly erupted material. Wysoczanski noted that there were new volcanic cones in one area. Volcanic rocks were collected, up to beach ball size, that vary in color and texture from black glassy material to white pumice. Round pebbles of pure sulphur were also retrieved.

Havre Seamount background. Smith and Price (2006) published one of the first bathymetric maps showing the main features of the Tonga-Kermadec arc/back-arc system and the location of Havre seamount (figure 13). Wright and others (2006) reported on the first full-scale mapping of Havre seamount in 2002 and some of its geology (figure 14). Table 2 lists locations for Havre seamount and other nearby features.

Figure (see Caption) Figure 13. (A) SW Pacific region showing the main features of the Tonga-Kermadec systems. (B) The Kermadec and Tonga arcs showing segmentation proposed by T.J. Worthington (University of Kiel, unpublished data); Kermadec segment S of 26°S latitude on the left, Tonga segment N of 26°S latitude on the right. Volcanoes are shown as conical symbols; note Havre volcano in middle of left map, Northern Kermadec segment. The ridge crests are defined by 500, 1,000, and 1,500 m bathymetric contours and the trench axis by the 8,000 and 7,000 m bathymetric contours. From Smith and Price (2006).
Figure (see Caption) Figure 14. (A) Regional setting of the Kermadec subduction system and the contiguous Tonga-New Zealand sectors to the N and S, respectively. (B-1, left) Regional setting of the S and central Kermadec subduction system, including newly discovered (2002) volcanoes (closed triangles) of the arc front. Dashed lines show location of the subduction and extensional plate boundaries, E and W of the Kermadec microplate, respectively, with grey arrows showing estimated relative Pacific-Kemadec plate motion and Kemadec-Australian plate motion in millimeters per annum. (B-2, right) Location of S and central Kermadec arc volcanoes relative to earthquake seismicity (from USGS catalog, January 1973-April 2003). (C) Bathymetry (in meters) and synoptic volcanic geology of Havre volcano. From Wright, Worthington, and Gamble (2006).

References. Anonymous, 2012. First sighting responsible for undersea eruption, Bay of Plenty Times, URL: http://www.bayofplentytimes.co.nz/news/first-sighting-responsible-undersea-eruption/1598061/, updated 27 October 2012, accessed 1 November 2012.

Bernard, A., 2012. Hot Spots from the July 18 Eruption in Kermadec volcanic arc, International Association of Volcanology and Chemistry of the Earth's Interior (IAVCEI) Commission of Volcanic Lakes (CVL), URL: http://www.ulb.ac.be/sciences/cvl/havre/pumice_raft_Havre_eruption.html, updated 13 August 2012, accessed 13 August 2012.

Bryan, S.E., Cook, A.G., Evans, J.P., Hebden, K., Hurrey, L., Colla, P., Jell, J.S., Weatherley, D., and Firn, J., 2012. Rapid, Long-Distance Dispersal by Pumice Rafting. PLoS ONE, v. 7, no. 7: e40583 (DOI: 10.1371/journal.pone.0040583).

Bryner, J., 2012. Pumice 'raft' floating off New Zealand coast created by undersea volcano eruption, researchers say, Huffington Post Science, URL: http://www.huffingtonpost.com/2012/10/27/pumice-raft-volcano_n_2028058.html, updated 26 October 2012, accessed 1 November 2012.

de Grauw, M. and Stradling, S., 2012. Personal communication (email to GVP), 10 Septebmer 2012.

Gardner, J.P.A., Curwen, M.J., Long, J., Williamson, R.J., and Wood, A.R., 2006. Benthic community structure and water column characteristics at two sites in the Kermadec Islands Marine Reserve, New Zealand, New Zealand Journal of Marine and Freshwater Research, v. 40, pp. 179-194.

Hyvernaud, O., 2012. Personal communication, Havre seamount volcanic eruption (email to GVP), 10 October 2012.

Klemetti, E., 2012a. Havre Seamount: The source of Kermadec Island pumice raft?, Wired: Eruptions Blog, URL:http://www.wired.com/wiredscience/2012/08/source-of-kermadec-island-pumice-raft-eruption-identified, updated 13 August 2012, accessed 2 October 2012.

Klemetti, E., 2012b. What Is the Fate of Volcanic Pumice Rafts?, Wired: Eruptions Blog, URL: http://www.wired.com/wiredscience/2012/08/the-biology-of-volcanic-pumice-rafts/, updated 22 August 2012, accessed 2 October 2012.

Memmott, M., 2012. 7,500 square miles of pumice floating in the Pacific is 'weirdest thing I've seen', National Public Radio, URL: http://m.npr.org/story/158577099?url=/blogs/thetwo-way/2012/08/10/158577099/7-500-square-miles-of-pumice-floating-in-pacific-is-weirdest-thing-ive-seen, updated 10 August 2012, accessed 13 September 2012.

New Zealand Land Information (LINZ), 2012. New Zealand Notices to Mariners Notices NZ 151-154, Edition 18, pp. 6-9, New Zealand Hydrographic Authority, Wellington, NZ, URL: http://www.linz.govt.nz/docs/hydro/ntm/pdf12/nz18-3108-151-154.pdf, updated 31 August 2012, accessed 13 September 2012.

New Zealand Land Information (LINZ), 2008, Kermadec Islands, South Pacific Ocean, New Zealand, map NZ222, scale 1:300,000, Sourced from Land Information New Zealand data. Crown Copyright Reserved. URL: http://data.linz.govt.nz/layer/1267-chart-nz-222-kermadec-islands/##, updated 27 August 2012, accessed 13 September 2012.

New Zealand National Institute of Water and Atmospheric Research (NIWA), 2012. First sighting of volcano responsible for undersea eruption, Press Release, NIWA, URL: http://www.scoop.co.nz/stories/SC1210/S00054/first-sighting-of-volcano-responsible-for-undersea-eruption.htm, updated 27 October 2012, accessed 1 November 2012.

Priestley, R., 2012. The mystery of the pumice raft, Listener, issue 3774, URL: http://www.listener.co.nz/current-affairs/science/the-mystery-of-the-pumice-raft/, updated 8 September 2012, accessed 25 September 2012 (see also http://blogs.scientificamerican.com/expeditions/2012/08/10/kermadecs-islands-a-serendipitous-event/; http://rebeccapriestley.com/2012/08/12/kermadecs-voyage-2-the-mystery-of-the-floating-pumice).

Scott, B., 2012. Volcanic activity: Kermadec Islands, media release, Institute of Geological and Nuclear Sciences Limited, Wairakei Research Centre, Taupo, NZ.

Smith, I.E.M., and Price, R.C., 2006. The Tonga-Kermadec arc and Havre-Lau back-arc system: Their role in the development of tectonic and magmatic models for the western Pacific, Journal of Volcanology and Geothermal Research, v. 156 (3-4), p. 315-331.

Wright, I.C., Worthington, T.J., and Gamble, J.A., 2006. New multibeam mapping and geochemistry of the 30°-35° S sector, and overview, of southern Kermadec arc volcanism, Journal of Volcanology and Geothermal Research, v. 149 (3-4), p. 263-296.

Geologic Background. Havre Seamount has a caldera capping a 1-km-high edifice. Located on the Kermadec Ridge, it is believed to have erupted in July 2012, the first recorded activity. The caldera has an asymmetric morphology with the N rim comprising mostly a single inner topographic wall, and the S rim comprising both an outer topographic rim and inner wall separated by a 1.1-1.4 km wide terrace. Smaller craters occur on this terrace. Rocks from the caldera wall include aphyric and plagioclase-bearing basalt-andesite, aphyric and plagioclase- and pyroxene-bearing dacite, gabbro, diorite, and pumice (Wright et al., 2006).

Information Contacts: Alain Bernard, Laboratoire de Volcanologie, Dept. Earth and Environmental Sciences CP160/02, Université Libre de Bruxelles 50, Ave. Roosevelt 1050 Brussels, Belgium; Bryan Scott, Queensland University of Technology, Brisbane, AU; Maggie de Grauw, Paeroa, New Zealand; Olivier Hyvernaud, Laboratorie de Géophysique, BP 640 Papeete, Tahiti, French Polynesia; Bradley J. Scott, Institute of Geological and Nuclear Sciences Limited (GNS) (URL: http://www.gns.cri.nz/); Eric Klemetti, Denison University (URL: https://www.wired.com/category/eruptions/); Roger Matthews, Unitec Institute of Technology, Auckland, NZ; NASA Earth Data Near Real Time (Orbit Swath) Images (URL: https://earthdata.nasa.gov/earth-observation-data/near-real-time); New Zealand Listener magazine (URL: http://www.noted.co.nz/the-listener/); New Zealand Defense Force (NZDF) (URL: http://www.nzdf.mil.nz/); Pew Environment Group (URL: http://www.pewenvironment.org); Rebecca Priestley, Victoria University of Wellington, New Zealand (URL: https://rebeccapriestley.com/); Robert Simmon and Jeff Schmaltz, NASA Earth Observatory (URL: http://earthobservatory.nasa.gov).


Popocatepetl (Mexico) — September 2012 Citation iconCite this Report

Popocatepetl

Mexico

19.023°N, 98.622°W; summit elev. 5393 m

All times are local (unless otherwise noted)


Intermittent ash plumes and diminished seismicity during July-October 2012

Since our last report discussing ash plumes and increased seismicity noted in April 2012 (BGVN 37:05), ash plumes from Popocatépetl's summit continued to be emitted at a reduced rate during July-October 2012. During this reporting period, the Centro Nacional de Prevención de Desastres (CENAPRED, based in Mexico City) noted persistent incandescence and gas emissions (sometimes containing ash). Seismicity decreased significantly in August and, on 1 September, CENAPRED reduced the Alert Level from Yellow, Phase Three to Yellow, Phase Two. New volcanic hazard maps were available from investigators focused on ejecta from the summit (Alatorre-Ibargüengoitia and others, 2012) and CENAPRED developed an interactive web interface for compiling layers of hazard zones based on volcanic phenomena expected from Popocatépetl.

Visual observations July-October 2012. From July through October 2012, CENAPRED reported that cloudcover frequently obscured the view of Popocatépetl's summit. During cloud-free conditions, incandescence from the crater could be observed at night and early in the morning. Moderate explosions (many containing incandescent tephra) occurred almost daily.

Several larger explosions were observed by CENAPRED on 21 July, in August (7, 17, 18, 20, 26 and 27), September (10, 14, and 15), and October (17, 18, 20, and 26). These events were captured by web cameras when incandescent tephra was ejected and traveled up to 1.5 km from the summit (figure 64).

Figure (see Caption) Figure 64. On 20 October 2012, the webcamera Altzomoni (located ~10 km to the NNW) captured moderate-sized explosions from Popocatépetl that ejected incandescent tephra across high elevation areas (within 1 km of the summit). From left to right, photos were captured at 05:34:25, 05:34:41, 07:24:23, and 09:36:44. Courtesy of CENAPRED.

When conditions permitted during July-October, gas-and-steam plumes (frequently containing ash), were observed reaching 0.5 to 2.5 km above the crater. Asfall was reported in the community of Ozumba (18 km W) on 21 July 2012. CENAPRED reported that an ash plume rose 4 km above the crater at 1758 on 6 August; incandescence from the crater was also observed that day.

Two lahars were detected in July 2012. The event on 3 July occurred at 1530 and was documented by the Tlamacas web camera (located ~5 km N of the crater). On 12 July, between 1938 and 2135, a lahar occurred on the N flank. Both of these events were attributed to glacial melt high on the flanks of Popocatépetl; no flooding was reported at low elevations.

VAAC ash detection during July-October 2012. The Washington Volcanic Ash Advisory Center (VAAC) announced observations of intermittent ash plumes from Popocatépetl during July-August 2012. At least five announcements were based on CENAPRED reports and imagery from local web cameras; cloud cover frequently obscured remote sensing images. During July-August, plume altitudes were in the range of 6.4-9.1 km (0.97-3.67 km above the crater); plumes tended to drift up to 130 km to the W, S, and SE.

No VAAC reports were released in September 2012 and five reports of observed ash were made in October 2012. During 11-26 October, maximum altitudes of ash plumes reached 7.6 km (~2.2 km above the crater) and tended to drift W, NW, and S.

Seismicity during July-October 2012. Decreasing seismicity was detected at Popocatépetl between July and October 2012. Approximately 30 hours of tremor were recorded by CENAPRED in July and ~18 hours in August, while approximately 9 and 10 hours were recorded in September and October, respectively. Volcano-tectonic (VT) earthquakes also occurred less frequently between July (~53 detected) and September (four detected). In October, ~15 VT events were reported in CENAPRED's online reports.

Hazard map for volcanic ejecta. A recent investigation by Alatorre-Ibargüengoitia and others (2012) highlighted the frequently-occurring Vulcanian eruptions of Popocatépetl and developed a volcanic ejecta risk assessment. Volcanic bombs have impacted the immediate summit area of the volcano as well as locations as distant as 3.7 km (the maximum distance considered in the simulations). The investigators combined video observations of past eruptions, field studies (between 1999 and 2010), and a ballistics model designed for simulating optimal launching conditions. One of the results from this investigation was a map defining three risk zones (figure 65).

Figure (see Caption) Figure 65. This map of Popocatépetl's summit, flanks, and local infrastructure includes hazard zonation for volcanic bombs. Locations with 5-point stars represent observed impact sites from 1998-2006; the 4-point star represents an impact site dating to 14,000 years before present. From Alatorre-Ibargüengoitia and others (2012).

An interactive hazard map for Popocatépetl was available online through the CENAPRED website (figure 66). Basemap options included terrain, streets with major towns, and satellite imagery. Users were able to choose from various volcanic phenomena (lava flows, ash fall, lahars, and pyroclastic flows) to view the predicted aerial extent of the relevant hazard. The flow paths and inundation areas for lava flows, lahars, and pyroclastic flows were determined with TITAN2D software based on data collected by CENAPRED. The zones representing high (red), medium (orange), and low (yellow) risk of ashfall (note the concentric zones in figure 66) were developed based on a 1995 study by CENAPRED (Macias and others, 1995).

Figure (see Caption) Figure 66. This map is a screenshot of CENAPRED's interactive hazard map, showing results from four scenarios; three types of lahar inundation parameters (highlighted drainages within ~40 km of the summit) and zones defining potential ashfall. Note that lahar hazards are within the orange zone of moderate ashfall hazards; the yellow zone indicating minor ashfall reaches Mexico City. The radius of the yellow zone (minor ashfall) is ~70 km. Courtesy of CENAPRED.

References. Alatorre-Ibargüengoitia, M.A., Delgado-Granados, H., and Dingwell, D.B., 2012. Hazard map for volcanic ballistic impacts at Popocatépetl volcano (Mexico), Bulletin of Volcanology, 74(9) pp 2,155-2,169.

Macias, J.L., Carrasco, G., Delgado, H., Martin del Pozzo, A.L., Siebe, C., Hoblitt, R., Sheridan, M.F., and Tilling, R.I., 1995. Mapa de peligros volcanicos del Popocatépetl, Pub especial Inst Geofis, UNAM.

Geologic Background. Volcán Popocatépetl, whose name is the Aztec word for smoking mountain, rises 70 km SE of Mexico City to form North America's 2nd-highest volcano. The glacier-clad stratovolcano contains a steep-walled, 400 x 600 m wide crater. The generally symmetrical volcano is modified by the sharp-peaked Ventorrillo on the NW, a remnant of an earlier volcano. At least three previous major cones were destroyed by gravitational failure during the Pleistocene, producing massive debris-avalanche deposits covering broad areas to the south. The modern volcano was constructed south of the late-Pleistocene to Holocene El Fraile cone. Three major Plinian eruptions, the most recent of which took place about 800 CE, have occurred since the mid-Holocene, accompanied by pyroclastic flows and voluminous lahars that swept basins below the volcano. Frequent historical eruptions, first recorded in Aztec codices, have occurred since Pre-Columbian time.

Information Contacts: Centro Nacional de Prevención de Desastres (CENAPRED), Av. Delfín Madrigal No.665. Coyoacan, México D.F. 04360, México (URL: https://www.gob.mx/cenapred/); Washington Volcanic Ash Advisory Center (VAAC), Satellite Analysis Branch (SAB), NOAA/NESDIS E/SP23, NOAA Science Center Room 401, 5200 Auth Rd, Camp Springs, MD 20746, USA (URL: http://www.ospo.noaa.gov/Products/atmosphere/vaac/).


Purace (Colombia) — September 2012 Citation iconCite this Report

Purace

Colombia

2.32°N, 76.4°W; summit elev. 4650 m

All times are local (unless otherwise noted)


Expanded monitoring efforts and persistent seismicity in 2012

Our previous report on Puracé (BGVN 25:05) described elevated seismicity and swarms from February through April 2000. The Popayán Observatory, part of the Instituto Colombiano de Geología y Minería (INGEOMINAS), released geochemical, geophysical, and visual observations of the volcano since our last report. Here we present the results from their field investigations focused on fumarolic sites, hot springs, and SO2 emissions. Low levels of seismicity persisted at Puracé during January-April 2008 and January 2010-August 2012, but tornillo and tremor events were frequently detected; elevated seismicity was detected in March 2012. Available maps include those for volcanic hazards, monitoring networks, and geomorphology. From January 2008-August 2012, the Alert Level for Puracé has remained at VI (Green; "volcanic behavior is in a typical background, noneruptive state"), the lowest level on a VI-I scale.

Hazard map for the Puracé region. A hazard map has been developed by INGEOMINAS for the Puracé region (figure 2). Three zones encompass the entire volcanic chain and one of the zones (delineating potential ashfall) reaches the town of Popayán (28 km NW).

Figure (see Caption) Figure 2. This hazard map delineates three zones around Puracé volcano (see text). The highest risk area (red) includes the volcanic centers Puracé and Curiquinga and also follows major drainages N and S. The moderate risk area (orange) includes most of the Coconucos volcanic chain and extends NW to include the town of Puracé. The lowest risk area (yellow) extends NW (including Popayán) and as far S as the town of Paletará. Courtesy of INGEOMINAS.

The red zone (highest risk area) indicates areas where lava flows may occur in the future, with inferred events including more than 1 m of ash fall and ballistic ejecta, lahars, volcanic gases, and elevated seismicity. Drainages surrounding the town of Puracé and the sulfur mine (Industrias Puracé) location are within the red zone.

The orange zone (moderate risk) would, in future eruptions, likely experience ashfall on the order of decimeters; pyroclastic flows could reach this region as well as lahars. The towns Coconuco, Puracé, and Pululó are within the orange zone; ~7 km SE of Purace volcano, the peak of Pan de Azúcar is at the boundary between the orange and yellow zones (figure 3).

Figure (see Caption) Figure 3. An aerial view looking SE along the Coconucos volcanic chain taken on 22 October 2011. Puracé is in the foreground and several craters are aligned in the distance. The tallest peak in the background is Pan de Azúcar. Courtesy of INGEOMINAS.

The yellow zone (low risk) distinguishes the largest hazard zone and encompasses Paletará, Paispamba, Timbio, Popayán, El Placer, Calibio, Paniquita, Polindara, Quintana, and other towns. This zone may experience centimeters to millimeters of ashfall in future eruptions. Flooding along rivers could also occur within this zone if volcanic material accumulated during an eruption. INGEOMINAS also noted that shock waves from a large eruption could be experienced within all three zones.

Ground deformation monitoring 1999-2012. In 1999, INGEOMINAS monitored deformation with an electronic tilt station located 1.24 km N of the crater (Guañarita station, 4,248 m a.s.l., GUAI). During January-April 2008, significant changes were absent. From January 2010-October 2011, the tiltmeter network was expanded to include two more electronic tiltmeters (figure 4), however, no major trends in ground deformation were noted during that time. INGEOMINAS noted a decreasing trend between October 2011 and April 2012 at the Lavas Rojas station (LAVI, 2.4 km WNW of the summit, 4,046 m a.s.l.). They calculated -90 µrad in total deflation from the N component and -70 µrad from the E component. At the Guañarita station (GUAI), deflation also began in October 2011 and continued through August 2012.

Figure (see Caption) Figure 4. The geophysical monitoring network for Puracé volcano in 2012 included electronic tiltmeters, GPS stations, line leveling benchmarks, and an EDM network concentrated NW of the edifice. In the lower-right-hand corner, three craters are visible (Puracé, Curiquinga, and Calambas). Courtesy of INGEOMINAS.

In August 2011, two permanent Global Positioning System (GPS) stations were installed on the flanks of Puracé located 1.24 km N (Guañarita, GUAG) and 2.48 km NW (Lavas Rojas, LAROG). A third GPS station, Agua Blanca (AGBG), was added to this network in November 2011, located 0.7 km W of the crater. During October 2011, deflation trends were observed with electronic tiltmeters; GPS and electronic distance measurement (EDM) campaigns showed few variations.

A magnetometer was installed near the Puracé edifice in December 2010 and, in January 2011, INGEOMINAS reported successful real-time transmissions to the Popayán Observatory (26 km NE of Puracé). The site location of the new instrument was 1.6 km N of the volcano in an area of andesitic lava flows emplaced during pre-Puracé development that remains undated. INGEOMINAS reported daily fluctuations in the magnetometer data and also identified anomalous solar activity that was confirmed with global datasets. Data sent from this station reported stable conditions persisting from January 2011 through August 2012.

Investigations at other volcanoes globally have shown successful correlations between magnetic fluctuations and magma intrusions, demonstrating the benefits of magnetometers in early warning systems. A basic unit of magnetism in the SI system is the tesla ("T"); this is a measure of magnetic field strength (a variable frequently denoted as B). [1 tesla = 1 weber/m2 = 1 newton/amp-m = 104 gauss = 109 gamma. Also, 1 nanotesla = 1 gamma (Sheriff, 1982)]. Hurst and others (2004) described examples:

"For instance, the basaltic andesite volcano Poas in Costa Rica showed changes of nearly 200 nanoTesla (Rymer and others, 2000), whereas the basaltic Japanese volcano Izu-Oshima showed changes of only tens of nanoTeslas in 1986 (Sasai and others, 1990). The latter case was one of the few in which magnetic changes clearly occurred before the volcanic activity started, a more marginal case was Unzen, where magnetic changes were recorded in the very early stages of an eruption (Tanaka, 1995)."

Geochemical monitoring. Between 1982 and 1993, INGEOMINAS carried out intermittent site visits to the fumaroles and hot springs located near the flanks and summit crater of Puracé (figure 5). Since 1994, they conducted periodic geochemical monitoring to evaluate the variations in fluid compositions from the hot springs and established a baseline of activity and characteristics.

Figure (see Caption) Figure 5. Photographed on 22 October 2011, a view of the N flank and crater rim of Puracé. Small, white plumes of gas rise from the fumarolic field located on the outside edge of the crater. The rugged peak of Chagarton, considered a pre-Puracé structure, is in view to the right of Puracé's summit (middle ground). In the background on the horizon is the tall, wide peak of Sotará volcano located ~32 km SW. Courtesy of INGEOMINAS.

On 16 April 2008, INGEOMINAS visited three sites located along the lower flanks of Puracé to determine radon-222 emissions: Agua Tibío, Tabío, and Agua Hirviendo. Relative to past records, values obtained from the soil at Agua Hirviendo were slightly higher: 2,035 pico Curies per Liter (pCi/L). Tabío and Agua Tibío respectively measured 323 and 790 pCi/L.

On 14 September 2011, INGEOMINAS scientists walked the crater rim to collect differential optical-absorption spectroscopy (DOAS) measurements to determine SO2 flux. The mobile DOAS campaign confirmed the concentration of gas was located within the fumarolic area on the N rim (figure 6). With a wind speed of 5.0 m/s from the W, total flux was 0.5 metric tons per day.

Figure (see Caption) Figure 6. The path traversed with a mobile DOAS instrument on 14 September 2011 around the crater rim of Puracé (note color coding). The background photo was taken by Colombia's national mapping agency, IGAC, in 1976. Courtesy of INGEOMINAS.

A field campaign to detect sulfur dioxide emissions was also conducted on 29 August 2012. Using a mobile Flyspec, a team of INGEOMINAS scientists focused on the Pozo Azul hot spring located ~8 km SW of the crater (also called PAFT in figure 7). This ultraviolet spectrometer sampled continuously for approximately five minutes while the scientists traversed the area around the hot spring (figure 7). There were four locations along the pathway where SO2 concentrations measured greater than 6.6 ppm-m. INGEOMINAS reported the total SO2 flux was 1.1 tons/day (windspeed of 7.7 m/s from the W).

Figure (see Caption) Figure 7. INGEOMINAS conducted a Flyspec traverse and calculated sulfur dioxide concentrations for the area around Pozo Azul, located ~8 km SW of Puracé's crater. Courtesy of INGEOMINAS.

Radon emissions had been monitored by INGEOMINAS from May 2011 through August 2012. Regular measurements were obtained from 13 stations located at sites around the volcanic edifice up to 12 km away (figure 8). Month-to-month variations tended to show rare correlations except for March-April 2012. In their monthly report from April 2012, INGEOMINAS highlighted this time period as significant for both seismic and radon assessments. Volcano-tectonic (VT) seismicity had been notably elevated during that time (an average of 116 earthquakes per month) and events were frequently occurring directly below the edifice. Long-period seismicity was also higher in March and April (an average of 290 earthquakes per month). Tremor, tornillo, and hybrid earthquakes occurred more frequently during these months compared with seismicity from the past two years.

Figure (see Caption) Figure 8. The geochemical monitoring network in August 2012 included radon emission detectors, hot spring sampling sites, and gas-sampling sites around the flanks of Puracé. (Top) This map shows the entire length of the Coconucos volcanic chain and sites within the monitoring network. (Bottom) Radon emissions were continuously monitored from 26 May 2011 through 18 August 2012, however, few datapoints were available between 23 October 2011 and February 2012. Courtesy of INGEOMINAS.

INGEOMINAS reported in their online August 2012 bulletin that field investigations of fumaroles and hot springs detected stable conditions without significant variations in geochemistry or temperatures. Continuous temperature readings from an in situ thermocouple were available from April 2012 to August 2012. This system was installed for monitoring changes in the fumarolic area located on the NW flank of the volcano in September 2011. Due to equipment problems related to equipment corrosion (a common problem in these extreme environments), the data was only successfully telemetered starting on 14 April 2012.

From January 2010 through August 2012, webcameras frequently captured images of the active fumarolic area located on the NW edge of the crater; small white plumes regularly rose from the fumaroles. During an overflight on 22 October 2011, INGEOMINAS observed small plumes of vapor from a crack in the crater floor and the fumarolic field (figure 9).

Figure (see Caption) Figure 9. Close-up views of vapor plumes observed during an overflight of Puracé on 22 October 2011. (Top) Two adjacent sources of steam merge into a single plume rising from a narrow fumarolic field located on the NW crater rim. Note the bright yellow surfaces where sulfur has precipitated. Past measurements of fumarole temperatures here had reached 128°C. (Bottom) INGEOMINAS noted white vapor rising from a crack within the crater floor. Vapor plumes within the crater were too small to rise above the rim and had not been visible with webcameras. Both features, the fumarolic field outside of the crater and the crack along the crater floor, trend roughly E-W. Courtesy of INGEOMINAS.

Overview of seismicity. Table 2 summarizes available seismic data for 2008-2012. More discussion appears in chronological subsections below.

Table 2. Seismicity at Puracé volcano during January-April 2008 and from January 2010 through August 2012. Volcano-tectonic (VT), long-period, tornillo, hybrid, and tremor events are reported per month. Depths and magnitudes (local magnitudes, ML) of VT events are mainly reported as ranges of dominant activity, however, many magnitudes are the largest events that occurred per month. Courtesy of INGEOMINAS.

Month Volcano-tectonic VT Depths (km) VT Magnitude (ML) Long-period Tornillo Hybrid Tremor
Jan 2008 246 1-20 -0.89-2.27 243 13 1 2
Feb 2008 95 1-24 -0.62-2.4 113 17 5 0
Mar 2008 91 1-6 -0.89-2.27 123 15 1 2
Apr 2008 51 1-4 -0.4-1.25 88 15 0 1
 
Jan 2010 77 1-15 1.7 167 0 0 0
Feb 2010 29 1-17 1.3 127 0 0 0
Mar 2010 76 1-15 2.0 182 30 7 0
Apr 2010 70 1-12 2.2 91 61 0 0
May 2010 54 1-15 2.04 85 45 0 0
Jun 2010 58 0.8-18 1.4 89 21 0 0
Jul 2010 33 0.8-2 1.14 113 37 0 0
Aug 2010 13 0.8-5 1.1 83 34 2 0
Sep 2010 49 5-15 1-4.4 81 28 0 0
Oct 2010 22 3-18 0.3-1.3 122 31 0 0
Nov 2010 112 1-7.5 0.2-2.1 157 31 0 0
Dec 2010 76 0.3-4 2.7 247 9 0 15
Jan 2011 49 0.7-4 1.8 210 7 0 10
Feb 2011 34 1.2-16 1.5 177 20 0 3
Mar 2011 68 1-12 1.6 152 17 0 3
Apr 2011 63 1-12 1.3 137 21 0 1
May 2011 45 1-15 1.7 197 19 0 2
Jun 2011 31 1-15 1.7 143 9 0 3
Jul 2011 26 1-13 2.4 116 13 0 13
Aug 2011 32 2-3 1.8 125 13 0 2
Sep 2011 15 1-2 1.5 154 1 0 2
Oct 2011 25 1-15 2.1 151 17 2 2
Nov 2011 25 1-4.5 1.3 125 15 2 2
Dec 2011 45 1-4.5 1.0 116 28 7 5
Jan 2012 67 0.8-5 0.1-1.8 184 54 17 4
Feb 2012 86 1-17 1.4 248 20 19 4
Mar 2012 143 1-3 2.2 332 46 30 32
Apr 2012 90 1-12 1.7 248 67 40 26
May 2012 31 1-12 1.9 219 29 4 8
Jun 2012 57 1-12 1.8 190 51 22 11
Jul 2012 33 1-12 1.5 181 35 7 2
Aug 2012 28 1-12 2.1 165 48 15 11

Seismicity during January-April 2008. In January 2008, INGEOMINAS reported increased seismicity within 15 km of the Puracé edifice. There were two regions of activity, along the Moras fault system and within the immediate area of the volcano (figure 10). The Moras fault crosses beneath Puracé and was indicated by earthquake locations to the NE (in the San Rafael lake area) and to the SW (in Paletará Valley) (figure 11). These locations were sites for earthquake swarms in February and April 2000 (BGVN 25:05).

Figure (see Caption) Figure 10. A map of epicenters for VT earthquakes located in the region of Puracé in January 2008. A total of 169 events were primarily located beneath the edifice and up to 5 km N in a sulfur mining district. The deepest and most distal earthquakes (to the NE and SW) were attributed to other portions of the Moras fault system, which also cuts through Puracé. Courtesy of INGEOMINAS.
Figure (see Caption) Figure 11. Puracé is the most active and northernmost volcano along the NW-SE trending Coconucos ridge. Numbers correspond to cones with craters (red hashed circles) and major peaks (red triangles): 1 Puracé volcano, 2 Piocollo, 3 Curiquinga, 4 Calambas, 5 Paletará, 6 Quintin, 7 Shaka (a cluster of craters with ponded water), 8 Killa, 9 Machangara (contains a small pond), 10 Pan de Azúcar (a prominent peak with a small summit crater), 11 Pukará, 12 Piki, 13 Amancay, 14 Chagartón (a large crater and peak has been attributed to this structure). Major regional faults are short dashed lines (brown); the local Coconucos fault and Río Vinagre fault zones are long-dashed lines (brown). The shaded terrain was derived from a 90 m SRTM (Shuttle Radar Topography Mission) digital elevation model. Highest elevations (greater than 4,000 m) are indicated by orange shading and reach a maximum of ~4,650 m; lowest elevations (gray shading) begin at 2,500 m. This map was compiled by GVP based on INGEOMINAS Popayán reports, maps, and aerial photos. Place names are from Arcila (1996), Cardona (1998), Kelsey (2001), and Monsalve and Pulgarín (1999).

Another local structure, the 2-3 km wide Río Vinagre fault system, underlies Puracé and trends subparallel with the Coconucos fault. Sturchio and others (1993) described the thermal waters, gases and sulfur deposits from Puracé and concluded that sulfur precipitation was likely resulting from hot magmatic gas ascending through the Río Vinagre fault zone. The hot springs were attributed to descending meteoric water interacting with the magmatic system.

A total of 508 events were detected in January 2008, primarily volcano-tectonic (VT) and long-period (LP) earthquakes, 249 and 243 events respectively (table 2). Tornillo (13 in total), hybrid (1 identified), and tremor (2 events identified) were also detected that month. Magnitudes of VTs were in the range of -0.89 to 2.27 and magnitudes of LPs in the range of 0.09 to 1.59. Focal depths tended to be shallow for those events occurring beneath the edifice (1-6 km) and deeper elsewhere along the fault system (6-20 km).

From February through April 2008, INGEOMINAS reported that seismicity from Puracé was relatively low (table 2). Approximately 210 earthquakes were detected each month, primarily LP and VT earthquakes. Tornillo events were detected throughout this time period averaging ~15 per month. Few hybrid events were detected in February and March (1-5 events), and tremor was detected in March and April (1-2 events). Earthquake magnitudes were largest in February (up to ML 2.4 for VT and LP earthquakes) and depths of earthquake foci were characteristically shallow for those events beneath the volcanic edifice (1-7 km). In February, earthquakes (6-17 km deep) were detected within the Moras fault zone with events in a similar distribution to those located in January 2008 (figure 10).

Episode of seismicity in December 2008.On 13 December 2008, INGEOMINAS released a special report announcing a short period of elevated seismicity. Beginning on 12 December, 625 LP earthquakes were detected over 29 hours. These events were low-magnitude (M 0.5-1) and clustered within the sulfur mine area ~2.8 km N. While these earthquakes were very shallow (

Seismicity during January 2010-August 2012. In 2010 and 2011, seismicity detected at Puracé was generally relatively low (table 2). Magnitudes of VT events during 2010 rarely exceeded 2.0 and earthquake foci were rarely deeper than 15 km. Earthquakes deeper than 10 km were typically beyond the edifice and related to the local fault systems. LP events occurred more frequently than VT events; INGEOMINAS reported that 81-247 LP events were detected per month and 13-112 VT events per month. Up to 61 tornillo earthquakes were detected in April 2010, however, no tornillos were recorded in January and February and only nine were recorded in December. Hybrid and tremor events were also rare; several months passed without detecting these events. In March and August, hybrid earthquakes were detected, and tremor was only reported in December.

Seismicity remained low throughout 2011, however, tremor (1-13 events per month) and tornillo earthquakes (1-28 events per month) were detected every month. Hybrid earthquakes were only reported from October through December 2011. VT and LP events persisted, but at a lower rate compared with the previous year; magnitudes and depths were also in the same range.

From January through August 2012, seismicity was consistently higher than the previous eight months. VT and LP events were more numerous, at rates of 28-143 per month and 165-332 per month, respectively. Magnitudes and depths of earthquakes remained within similar ranges as previously recorded. Tremor and hybrid earthquakes were detected every month.

INGEOMINAS emphasized that seismicity was particularly high in March 2012, with more VT and LP events that month than in any month in the past two years. Numerous tornillo, hybrid, and tremor events were also reported (table 2). Seismicity was still comparatively elevated but less so in the five months that followed March 2012.

References. Arcila, M., 1996. Geophysical monitoring of the Puracé volcano, Colombia, Annali di Geofisica, vol. XXXIX, N. 2, pp. 265-272.

Cardona, C.E., 1998. Caracterización de fuentes sísmicas en el volcán Puracé, Geology thesis, Universidad de Caldas.

Hurst, A.W., Rickerby, P.C., Scott, B.J., and Hashimoto, T., 2004. Magnetic field changes on White Island, New Zealand, and the value of magnetic changes for eruption forecasting, Journal of Volcanology and Geothermal Research, 136, pp. 53-70.

Kelsey, M.R., 2001. Climber's and Hiker's Guide to the World's Mountains & Volcanoes, Kelsey Publishing, Provo, UT, 4th ed., p. 1248.

Monsalve, M.L. and Pulgarín, B., 1999. Cadena Volcánica de los Coconucos (Colombia): Centros eruptivos y producto recientes, Boletín Geológico, 37 (1-3): 17-51.

Sheriff, R.E., 1982. Encyclopedic Dictionary of Exploration Geophysics, Society of Exploration Geophysicists, Tulsa, OK, p. 266.

Sturchio, N.C., Williams, S.N., and Sano, Y., 1993. The hydrothermal system of Volcan Puracé, Colombia, Bulletin of Volcanology, 55, pp. 289-296.

Geologic Background. Puracé in Colombia consists of an andesitic stratovolcano with a 500-m-wide summit crater constructed over a dacitic shield volcano. It lies at the NW end of a volcanic massif opposite Pan de Azúcar stratovolcano, 6 km SE. A NW-SE-trending group of seven cones and craters, Los Coconucos, lies between the two larger edifices. Frequent explosive eruptions in the 19th and 20th centuries have modified the morphology of the summit crater. The largest eruptions occurred in 1849, 1869, and 1885.

Information Contacts: Instituto Colombiano de Geologia y Mineria (INGEOMINAS), Observatorio Vulcanológico y Sismológico de Popayán, Popayán, Colombia.


Sotara (Colombia) — September 2012 Citation iconCite this Report

Sotara

Colombia

2.108°N, 76.592°W; summit elev. 4400 m

All times are local (unless otherwise noted)


Monitoring efforts and recent seismic unrest

Sotará is considered a recently-active volcano within the Sotará volcanic complex described by the Instituto Colombiano de Geología y Minería (INGEOMINAS) as a caldera with resurgent volcanism. Two volcanoes developed within the caldera, Sotará in the center and Cerro Gordo on the S edge (figure 1). Two smaller volcanic peaks, Cerro Negro and Cerro Azafatudo, have been identified on the NW flank of the caldera and described as pre-Sotará features. Monitoring efforts by INGEOMINAS's Popayán Observatory, beginning in 1993, documented persistent seismicity, active fumarolic sites, and thermal springs. Historic eruptions (within 500 years) have not been observed from this complex.

Figure (see Caption) Figure 1. Aerial photos of Sotará volcanic complex were taken on 18 October 2011. (Left) The two volcanic centers, Sotará and Cerro Gordo, are aligned in this photo, looking NW. The taller peak, Sotará, is in the middle-ground and Cerro Gordo is in the foreground. On the horizon to the right is the low, gray peak of Azafatudo volcano. (Right) Looking approximately E into the amphitheater of Sotará, dome rock appears gray, however, much of the talus has been vegetated by red and yellow groundcover. Courtesy of INGEOMINAS.

Expanded monitoring efforts. The INGEOMINAS observatory based in Popayán (37 km NW of Sotará) began monitoring volcanic activity at Sotará in 1993. A seismic station was installed on the NE flank of the volcano that year and in 1995, significant seismicity was detected by that station. A temporary seismic station was added to the area in 1995 and by 2007, the monitoring network was expanded with permanent stations. In August 2012 the network contained eight geophysical stations that included short period and broadband seismic stations, electronic tiltmeters, a webcamera, and electronic distance meter (EDM) measuring sites (reflectors and benchmarks) (figure 2).

Figure (see Caption) Figure 2. The station locations for geophysical monitoring at Sotará volcano. (Left) In August 2012, the deformation network included EDM stations (two benchmarks and two reflectors) and two electronic tiltmeters. (Right) The seismic network included three broadband stations (SOTB, OSOB, and CGOR) and one shortperiod station (SOSO). Courtesy of INGEOMINAS.

Since monitoring began in 1993, the largest earthquake that occurred in this region had a local magnitude (ML) of 4.4 with an epicenter 16 km NW of Sotará. INGEOMINAS recorded the event at 1537 (local time) on 6 June 2010 with a focal depth at 6.9 km. The shaking caused by this earthquake was reported in six communities located as far as 20 km N of the epicenter. There were five aftershocks with magnitudes ranging 0.5-2.6. One of these aftershocks, occurring at 1555, was felt in two towns, Chapa and Coconuco (located 5.5 km NW and 15 km N of the epicenter, respectively). The last aftershock (ML 2.4) was recorded on 7 June with a 6-km focal depth and epicenter 22.7 km NW of the volcano.

INGEOMINAS reported low levels of seismicity from January 2010 through May 2012 (table 1). Volcano-tectonic (VT) earthquakes occurred more frequently than long period (LP) events or events interpreted as rockfalls (RF). VT hypocenters were calculated for 1-14 earthquakes per month except during October 2011, when 50 VT events were located within the Paletará Valley (see subsection Paletará Valley seismicity for details). From 2010 through May 2012, local magnitudes were rarely greater than 2.

Figure (see Caption) Table 1. Earthquakes registered at Sotará volcano from 2010 through September 2012. The "LP or RF" column contains the number of long-period (LP) or rockfall (RF) events counted for that month. Depths are reported in km. The values reported in the volcano-tectonic (VT) events column are located earthquakes; however, several months in 2010 did not include located hypocenters and total VTs are reported instead (underlined, text in red). Note that located earthquakes are a subset of the total number of events classified as VT. In March 2011, LP and RF signatures were classified but not tallied ("undisc."). The range of local magnitudes (ML) per month is shown in the last column. Courtesy of INGEOMINAS.

Paletará Valley seismicity. Beginning in January 2010, INGEOMINAS reported earthquakes frequently occurring within the Paletará Valley. In a roughly circular region ~5 km in diameter, VT earthquakes clustered at a distance 15-25 km NE from Sotará's edifice (figure 3). Many of these events were too small to locate (ML 

Figure (see Caption) Figure 3. VT seismicity during January 2011 was concentrated in an area NE of Sotará volcano. The yellow oval highlights epicenters within the Paletará Valley, a typical location for earthquakes since 2010. Focal depths were between 4 and 7 km. Three seismic stations are labeled in blue text: SOBZ (NNW of Sotará), SOSO (on the NW flank of Sotará), and CGOR (on the NW flank of Cerro Gordo). Courtesy of INGEOMINAS.

In 2011, relatively large earthquakes were detected in October and December within Paletará Valley. INGEOMINAS reported elevated seismicity that began on 14 October at 1423. Low magnitude events, characterized as rockfalls, were also recorded on 14 October. Over the next 24 hours, ~38 earthquakes were recorded and by the end of the month, 54 VT earthquakes were registered with epicenters within ~7-10 km NE of Sotará. Local magnitudes ranged from 0.1-2.7. INGEOMINAS announced in a 15 October assessment that seismicity had not affected the Sotará volcanic system and communities located near the volcano were not at risk.

On 18 December 2011 at 0902 an ML 3.2 earthquake was detected by the INGEOMINAS seismic network. The epicenter was 21 km SW of Sotará and 17.5 km deep. Shaking was reported in the town of La Vega located ~20 km W of Sotará.

Seismic unrest in 2012. In early 2012, ~6 earthquakes were located per month and epicenters tended to cluster NE of the edifice (table 1). In April 2012, several earthquakes also appeared ~10 km SW of Sotará. From January through May 2012, VT earthquakes (no LPs occurred) were shallow (0.5-2 km), however, due to small magnitudes (ML 0.5-2.1), the events did not cause noticeable shaking in local communities.

In their June 2012 technical bulletin, INGEOMINAS noted increased seismicity clustered within 4 km NE of the summit. Local seismic stations detected 744 events and located 120 events classified as VTs. Epicenters were clustered in an elongate region striking 3 km NE. Local magnitudes ranged between -0.5-2.0 with depths ranging 2-6 km.

Seismicity decreased by 30 June; however, on 25 July, numerous VT events were registered. By 31 July, 1,232 VT earthquakes had been detected (575 of which were located), 2,295 events were detected but not classified, and nine LP events were detected. Epicenters were dispersed in a larger zone NE of the summit, however, magnitudes and depths were similar to those detected during the previous month.

A site visit conducted by INGEOMINAS in July included the NW sector of Sotará where hot springs were located. Investigators measured temperatures and assessed the geochemistry of the springs and determined that no significant changes had occurred.

Increased seismicity persisted in early August 2012 and by 8 August, INGEOMINAS reported that, on average, 150 earthquakes were occurring per day (figure 4). In a special bulletin, INGEOMINAS assessed the seismicity and also highlighted new conclusions from the tiltmeter network. They noted that from January 2010 through July 2012, no deformation was detected by the electronic tiltmeters. By early August 2012, an inflation trend was detected in the NE sector that was potentially linked to the cluster of earthquakes in the immediate area. No significant trends were interpreted from the SW sector. On 8 August 2012, INGEOMINAS announced that the Alert Level was raised to III (Yellow; "changes in the behavior of volcanic activity"), or the second lowest level.

Figure (see Caption) Figure 4. The number of VT earthquakes detected at Sotará dramatically increased in July 2012 and continued at a relatively high rate through early August 2012. (Top) In August 2012, earthquakes were clustered within 2 km NE of the edifice; the two cross-sections indicate shallow hypocenters in the range of 2-5 km. (Bottom) The histogram of VT events from June 2012 through August 2012 demonstrates three periods of increased seismicity; while minor LP events were detected during this time interval, they did not appear in the histogram. Courtesy of INGEOMINAS.

INGEOMINAS continued to monitor Sotará closely from September through early October 2012 and noted decreasing seismicity. Fewer earthquakes were registered (22-100 VTs) and magnitudes ranged 0.1-1.6. Clear images captured by the local webcamera (located 3 km NW) showed no morphological changes (figure 5).

Figure (see Caption) Figure 5. A view of Sotará's NW flank from the webcamera location on Cerro Crespo. From left to right, starting at the top, these images were taken on 5, 13, 21, and 26 July 2012. Courtesy of INGEOMINAS.

References. Cediel, F., Shaw, R.P., and Cáceres, C., 2003, Tectonic assembly of the Northern Andean Block, in C. Bartolini, R.T. Buffler, and J. Blickwede, eds., The Circum-Gulf of Mexico and the Caribbean: Hydrocarbon habitats, basin formation, and plate tectonics: AAPG Memoir 79, p. 815-848.

Page, W.D., 1983, Popayán earthquake of 31 March 1983 geologic and seismologic aspects, Woodward Clyde Consultants, San Francisco Area Office, Walnut Creek, CA, USA, p. 51-59.

Geologic Background. Volcán Sotará, also known as Cerro Azafatudo, is an andesitic-dacitic stratovolcano about 25 km SSE of Popayán city in southern Colombia, SW of Puracé volcano. Three calderas, 4.5, 2.5, and 1 km in diameter, give the summit an irregular profile. No historical eruptions are known, though there is current fumarolic and hot spring activity.

Information Contacts: Instituto Colombiano de Geologia y Mineria (INGEOMINAS), Observatorio Vulcanológico y Sismológico de Popayán, Popayán, Colombia.

Atmospheric Effects

The enormous aerosol cloud from the March-April 1982 eruption of Mexico's El Chichón persisted for years in the stratosphere, and led to the Atmospheric Effects section becoming a regular feature of the Bulletin. Descriptions of the initial dispersal of major eruption clouds remain with the individual eruption reports, but observations of long-term stratospheric aerosol loading will be found in this section.

Atmospheric Effects (1980-1989)  Atmospheric Effects (1995-2001)

Special Announcements

Special announcements of various kinds and obituaries.

Special Announcements  Obituaries

Misc Reports

Reports are sometimes published that are not related to a Holocene volcano. These might include observations of a Pleistocene volcano, earthquake swarms, or floating pumice. Reports are also sometimes published in which the source of the activity is unknown or the report is determined to be false. All of these types of additional reports are listed below by subject.

Additional Reports  False Reports