The lava lake in the summit crater of Erebus has been active since at least 1972. Located in Antarctica overlooking the McMurdo Station on Ross Island, it is the southernmost active volcano on the planet. Because of the remote location, activity is primarily monitored by satellites. This report covers activity during 2023.

The number of thermal alerts recorded by the Hawai'i Institute of Geophysics and Planetology’s MODVOLC Thermal Alerts System increased considerably in 2023 compared to the years 2020-2022 (table 9). In contrast to previous years, the MODIS instruments aboard the Aqua and Terra satellites captured data from Erebus every month during 2023. Consistent with previous years, the lowest number of anomalous pixels were recorded in January, November, and December.

Table 9. Number of monthly MODIS-MODVOLC thermal alert pixels recorded at Erebus during 2017-2023. See BGVN 42:06 for data from 2000 through 2016. The table was compiled using data provided by the HIGP – MODVOLC Thermal Alerts System.

Sentinel-2 infrared images showed one or two prominent heat sources within the summit crater, accompanied by adjacent smaller sources, similar to recent years (see BGVN 46:01, 47:02, and 48:01). A unique image was obtained on 25 November 2023 by the OLI-2 (Operational Land Imager-2) on Landsat 9, showing the upper part of the volcano surrounded by clouds (figure 32).

Figure 32. Satellite view of Erebus with the summit and upper flanks visible above the surrounding weather clouds on 25 November 2023. Landsat 9 OLI-2 (Operational Land Imager-2) image with visible and infrared bands. Thermal anomalies are present in the summit crater. The edifice is visible from about 2,000 m elevation to the summit around 3,800 m. The summit crater is ~500 m in diameter, surrounded by a zone of darker snow-free deposits; the larger circular summit area is ~4.5 km diameter. NASA Earth Observatory image by Lauren Dauphin, using Landsat data from the U.S. Geological Survey.

Geologic Background. Mount Erebus, the world's southernmost historically active volcano, overlooks the McMurdo research station on Ross Island. It is the largest of three major volcanoes forming the crudely triangular Ross Island. The summit of the dominantly phonolitic volcano has been modified by one or two generations of caldera formation. A summit plateau at about 3,200 m elevation marks the rim of the youngest caldera, which formed during the late-Pleistocene and within which the modern cone was constructed. An elliptical 500 x 600 m wide, 110-m-deep crater truncates the summit and contains an active lava lake within a 250-m-wide, 100-m-deep inner crater; other lava lakes are sometimes present. The glacier-covered volcano was erupting when first sighted by Captain James Ross in 1841. Continuous lava-lake activity with minor explosions, punctuated by occasional larger Strombolian explosions that eject bombs onto the crater rim, has been documented since 1972, but has probably been occurring for much of the volcano's recent history.

Information Contacts: Hawai'i Institute of Geophysics and Planetology (HIGP) - MODVOLC Thermal Alerts System, School of Ocean and Earth Science and Technology (SOEST), Univ. of Hawai'i, 2525 Correa Road, Honolulu, HI 96822, USA (URL: http://modis.higp.hawaii.edu/); Copernicus Browser, Copernicus Data Space Ecosystem, European Space Agency (URL: https://dataspace.copernicus.eu/browser/); NASA Earth Observatory, EOS Project Science Office, NASA Goddard Space Flight Center, Goddard, Maryland, USA (URL: https://earthobservatory.nasa.gov/images/152134/erebus-breaks-through).

Rincón de la Vieja is a volcanic complex in Costa Rica with a hot convecting acid lake that exhibits frequent weak phreatic explosions, gas-and-steam emissions, and occasional elevated sulfur dioxide levels (BGVN 45:10, 46:03, 46:11). The current eruption period began June 2021. This report covers activity during July-December 2023 and is based on weekly bulletins and occasional daily reports from the Observatorio Vulcanologico Sismologica de Costa Rica-Universidad Nacional (OVSICORI-UNA).

Numerous weak phreatic explosions continued during July-December 2023, along with gas-and-steam emissions and plumes that rose as high as 3 km above the crater rim. Many weekly OVSICORI-UNA bulletins included the previous week's number of explosions and emissions (table 9). For many explosions, the time of explosion was given (table 10). Frequent seismic activity (long-period earthquakes, volcano-tectonic earthquakes, and tremor) accompanied the phreatic activity.

Table 9. Number of reported weekly phreatic explosions and gas-and-steam emissions at Rincón de la Vieja, July-December 2023. Counts are reported for the week before the Weekly Bulletin date; not all reports included these data. Courtesy of OVSICORI-UNA.

Table 10. Summary of activity at Rincón de la Vieja during July-December 2023. Weak phreatic explosions and gas emissions are noted where the time of explosion was indicated in the weekly or daily bulletins. Height of plumes or emissions are distance above the crater rim. Courtesy of OVSICORI-UNA.

According to OVSICORI-UNA, during July-October the average weekly sulfur dioxide (SO₂) flux ranged from 68 to 240 tonnes/day. However, in mid-November the flux increased to as high as 334 tonnes/day, the highest value measured in recent years. The high SO₂ flux in mid-November was also detected by the TROPOMI instrument on the Sentinel-5P satellite (figure 43).

Figure 43. Sulfur dioxide (SO2) maps from Rincón de la Vieja recorded by the TROPOMI instrument aboard the Sentinel-5P satellite on 16 November (left) and 20 November (right) 2023. Mass estimates are consistent with measurements by OVSICORI-UNA near ground level. Some of the plume on 20 November may be from other volcanoes (triangle symbols) in Costa Rica and Nicaragua. Courtesy of the NASA Global Sulfur Dioxide Monitoring Page.

Geologic Background. Rincón de la Vieja, the largest volcano in NW Costa Rica, is a remote volcanic complex in the Guanacaste Range. The volcano consists of an elongated, arcuate NW-SE-trending ridge constructed within the 15-km-wide early Pleistocene Guachipelín caldera, whose rim is exposed on the south side. Sometimes known as the "Colossus of Guanacaste," it has an estimated volume of 130 km3 and contains at least nine major eruptive centers. Activity has migrated to the SE, where the youngest-looking craters are located. The twin cone of Santa María volcano, the highest peak of the complex, is located at the eastern end of a smaller, 5-km-wide caldera and has a 500-m-wide crater. A Plinian eruption producing the 0.25 km3 Río Blanca tephra about 3,500 years ago was the last major magmatic eruption. All subsequent eruptions, including numerous historical eruptions possibly dating back to the 16th century, have been from the prominent active crater containing a 500-m-wide acid lake located ENE of Von Seebach crater.

Information Contacts: Observatorio Vulcanológico Sismológica de Costa Rica-Universidad Nacional (OVSICORI-UNA), Apartado 86-3000, Heredia, Costa Rica (URL: http://www.ovsicori.una.ac.cr/); 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/).

Bezymianny, located on Russia’s Kamchatka Peninsula, has had eruptions since 1955 characterized by dome growth, explosions, pyroclastic flows, ash plumes, and ashfall. Activity during November 2022-April 2023 included gas-and-steam emissions, lava dome collapses generating avalanches, and persistent thermal activity. Similar eruptive activity continued from May through October 2023, described here based on information from weekly and daily reports of the Kamchatka Volcano Eruptions Response Team (KVERT), notices from Tokyo VAAC (Volcanic Ash Advisory Center), and from satellite data.

Overall activity decreased after the strong period of activity in late March through April 2023, which included ash explosions during 29 March and 7-8 April 2023 that sent plumes as high as 10-12 km altitude, along with dome growth and lava flows (BGVN 48:05). This reduced activity can be seen in the MIROVA thermal detection system graph (figure 56), which was consistent with data from the MODVOLC thermal detection system and with Sentinel-2 satellite images that showed persistent hotspots in the summit crater when conditions allowed observations. A renewed period of strong activity began in mid-October 2023.

Figure 56. The MIROVA (Log Radiative Power) thermal data for Bezymianny during 20 November 2022 through October 2023 shows heightened activity in the first half of April and second half of October 2023, with lower levels of thermal anomalies in between those times. Courtesy of MIROVA.

Activity increased significantly on 17 October 2023 when large collapses began during 0700-0830 on the E flanks of the lava dome and continued to after 0930 the next day (figure 57). Ash plumes rose to an altitude of 4.5-5 km, extending 220 km NNE by 18 October. A large explosion at 1630 on 18 October produced an ash plume that rose to an altitude of 11 km (8 km above the summit) and drifted NNE and then NW, extending 900 km NW within two days at an altitude of 8 km. Minor ashfall was noted in Kozyrevsk (45 km WNW). At 0820 on 20 October an ash plume was identified in satellite images drifting 100 km ENE at altitudes of 4-4.5 km.

Figure 57. Sentinel-2 satellite images of Bezymianny from 1159 on 17 October 2023 (2359 on 16 October UTC) showing a snow-free S and SE flank along with thermal anomalies in the crater and down the SE flank. Left image is in false color (bands 8, 4, 3); right image is thermal infrared (bands 12, 11, 8A). Courtesy of Copernicus Browser.

Lava flows and hot avalanches from the dome down the SE flank continued over the next few days, including 23 October when clear conditions allowed good observations (figures 58 and 59). A large thermal anomaly was observed over the volcano through 24 October, and in the summit crater on 30 October (figure 60). Strong fumarolic activity continued, with numerous avalanches and occasional incandescence. By the last week of October, volcanic activity had decreased to a level consistent with that earlier in the reporting period.

Figure 58. Daytime photo of Bezymianny under clear conditions on 23 October 2023 showing a lava flow and avalanches descending the SE flank, incandescence from the summit crater, and a small ash plume. Photo by Yu. Demyanchuk, courtesy of IVS FEB RAS, KVERT.

Figure 59. Night photo of Bezymianny under cloudy conditions on 23 October 2023 showing an incandescent lava flow and avalanches descending the SE flank. Photo by Yu. Demyanchuk, courtesy of IVS FEB RAS, KVERT.

Figure 60. Sentinel-2 satellite images of Bezymianny from 1159 on 30 October 2023 (2359 on 29 October UTC) showing a plume drifting SE and thermal anomalies in the summit crater and down multiple flanks. Left image is in true color (bands 4, 3, 2); right image is thermal infrared (bands 12, 11, 8A). Courtesy of Copernicus Browser.

Aviation warnings were frequently updated during 17-20 October. KVERT issued a Volcano Observatory Notice for Aviation (VONA) on 17 October at 1419 and 1727 (0219 and 0527 UTC) raising the Aviation Color Code (ACC) from Yellow to Orange (second highest level). The next day, KVERT issued a VONA at 1705 (0505 UTC) raising the ACC to Red (highest level) but lowered it back to Orange at 2117 (0917 UTC). After another decrease to Yellow and back to Orange, the ACC was reduced to Yellow on 20 October at 1204 (0004 UTC). In addition, the Tokyo VAAC issued a series of Volcanic Ash Advisories beginning on 16 October and continuing through 30 October.

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/); Tokyo Volcanic Ash Advisory Center (VAAC), 1-3-4 Otemachi, Chiyoda-ku, Tokyo 100-8122, Japan (URL: http://ds.data.jma.go.jp/svd/vaac/data/); Hawai'i Institute of Geophysics and Planetology (HIGP) - MODVOLC Thermal Alerts System, School of Ocean and Earth Science and Technology (SOEST), Univ. of Hawai'i, 2525 Correa Road, Honolulu, HI 96822, USA (URL: http://modis.higp.hawaii.edu/); 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/).chr

Kīlauea is the southeastern-most volcano in Hawaii and overlaps the E flank of the Mauna Loa volcano. Its East Rift Zone (ERZ) has been intermittently active for at least 2,000 years. An extended eruption period began in January 1983 and was characterized by open lava lakes and lava flows from the summit caldera and the East Rift Zone. During May 2018 magma migrated into the Lower East Rift Zone (LERZ) and opened 24 fissures along a 6-km-long NE-trending fracture zone that produced lava flows traveling in multiple directions. As lava emerged from the fissures, the lava lake at Halema'uma'u drained and explosions sent ash plumes to several kilometers altitude (BGVN 43:10).

The current eruption period started during September 2021 and has recently been characterized by lava effusions, spatter, and sulfur dioxide emissions in the active Halema’uma’u lava lake (BGVN 47:08). Lava effusions, some spatter, and sulfur dioxide emissions have continued during this reporting period of July through December 2022 using daily reports, volcanic activity notices, and abundant photo, map, and video data from the US Geological Survey's (USGS) Hawaiian Volcano Observatory (HVO).

Summary of activity during July-December 2022. Low-level effusions have continued at the western vent of the Halema’uma’u crater during July through early December 2022. Occasional weak ooze-outs (also called lava break outs) would occur along the margins of the crater floor. The overall level of the active lava lake throughout the reporting period gradually increased due to infilling, however it stagnated in mid-September (table 13). During September through November, activity began to decline, though lava effusions persisted at the western vent. By 9 December, the active part of the lava lake had completely crusted over, and incandescence was no longer visible.

Table 13. Summary of measurements taken during overflights at Kīlauea that show a gradual increase in the active lava lake level and the volume of lava effused since 29 September 2021. Lower activity was reported during September-October. Data collected during July-December 2022. Courtesy of HVO.

Activity during July 2022. Lava effusions were reported from the western vent in the Halema’uma’u crater, along with occasional weak ooze-outs along the margins of the crater floor. The height of the lava lake was variable due to deflation-inflation tilt events; for example, the lake level dropped approximately 3-4 m during a summit deflation-inflation event reported on 1 July. Webcam images taken during the night of 6-12 July showed intermittent low-level spattering at the western vent that rose less than 10 m above the vent (figure 519). Measurements made during an overflight on 7 July indicated that the crater floor was infilled about 130 m and that 95 million cubic meters of lava had been effused since 29 September 2021. A single, relatively small lava ooze-out was active to the S of the lava lake. Around midnight on 8 July there were two brief periods of lava overflow onto the lake margins. On 9 July lava ooze-outs were reported near the SE and NE edges of the crater floor and during 10-11 July they occurred near the E, NE, and NW edges. On 16 July crater incandescence was reported, though the ooze-outs and spattering were not visible. On 18 July overnight webcam images showed incandescence in the western vent complex and two ooze-outs were reported around 0000 and 0200 on 19 July. By 0900 there were active ooze-outs along the SW edge of the crater floor. Measurements made from an overflight on 19 July indicated that the crater floor was infilled about 133 m and 98 million cubic meters of lava had erupted since 29 September 2021 (figure 520). On 20 July around 1600 active ooze-outs were visible along the N edge of the crater, which continued through the next day. Extensive ooze-outs occurred along the W margin during 24 July until 1900; on 26 July minor ooze-outs were noted along the N margin. Minor spattering was visible on 29 July along the E margin of the lake. The sulfur dioxide emission rates ranged 650-2,800 tons per day (t/d), the higher of which was measured on 8 July (figure 519).

Figure 519. Minor spattering rising less than 10 m was visible at the E end of the lava lake within Halema‘uma‘u, at the summit of Kīlauea on 8 July 2022. Sulfur dioxide is visible rising from the lake surface (bluish-colored fume). A sulfur dioxide emission rate of approximately 2,800 t/d was measured on 8 July. Courtesy of K. Mulliken, USGS.

Figure 520. A helicopter overflight on 19 July 2022 allowed for aerial visible and thermal imagery to be taken of the Halema’uma’u crater at Kīlauea’s summit crater. The active part of the lava lake is confined to the western part of the crater. The scale of the thermal map ranges from blue to red, with blue colors indicative of cooler temperatures and red colors indicative of warmer temperatures. Courtesy of USGS, HVO.

Activity during August 2022. The eruption continued in the Halema’uma’u crater at the western vent. According to HVO the lava in the active lake remained at the level of the bounding levees. Occasional minor ooze-outs were observed along the margins of the crater floor. Strong nighttime crater incandescence was visible after midnight on 6 August over the western vent cone. During 6-7 August scattered small lava lobes were active along the crater floor and incandescence persisted above the western vent through 9 August. During 7-9 August HVO reported a single lava effusion source was active along the NW margin of the crater floor. Measurements from an overflight on 4 August indicated that the crater floor was infilled about 136 m total and that 102 million cubic meters of lava had been erupted since the start of the eruption. Lava breakouts were reported along the N, NE, E, S, and W margins of the crater during 10-16 August. Another overflight survey conducted on 16 August indicated that the crater floor infilled about 137 m and 104 million cubic meters of lava had been erupted since September 2021. Measured sulfur dioxide emissions rates ranged 1,150-2,450 t/d, the higher of which occurred on 8 August.

Activity during September 2022. During September, lava effusion continued from the western vent into the active lava lake and onto the crater floor. Intermittent minor ooze-outs were reported through the month. A small ooze-out was visible on the W crater floor margin at 0220 on 2 September, which showed decreasing surface activity throughout the day, but remained active through 3 September. On 3 September around 1900 a lava outbreak occurred along the NW margin of the crater floor but had stopped by the evening of 4 September. Field crews monitoring the summit lava lake on 9 September observed spattering on the NE margin of the lake that rose no higher than 10 m, before falling back onto the lava lake crust (figure 521). Overflight measurements on 12 September indicated that the crater floor was infilled a total of 143 m and 111 million cubic meters of lava had been erupted since September 2021. Extensive breakouts in the W and N part of the crater floor were reported at 1600 on 20 September and continued into 26 September. The active part of the lava lake dropped by 10 m while other parts of the crater floor dropped by several meters. Summit tiltmeters recorded a summit seismic swarm of more than 80 earthquakes during 1500-1800 on 21 September, which occurred about 1.5 km below Halema’uma’u; a majority of these were less than Mw 2. By 22 September the active part of the lava lake was infilled about 2 m. On 23 September the western vent areas exhibited several small spatter cones with incandescent openings, along with weak, sporadic spattering (figure 522). The sulfur dioxide emission rate ranged from 930 t/d to 2,000 t/d, the higher of which was measured on 6 September.

Figure 521. Photo of spattering occurring at Kīlauea's Halema’uma’u crater during the morning of 9 September 2022 on the NE margin of the active lava lake. The spatter material rose 10 m into the air before being deposited back on the lava lake crust. Courtesy of C. Parcheta, USGS.

Figure 522.The active western vent area at Kīlauea's Halema’uma’u crater consisted of several small spatter cones with incandescent openings and weak, sporadic spattering. Courtesy of M. Patrick, USGS.

Activity during October 2022. Activity during October declined slightly compared to previous months, though lava effusions persisted from the western vent into the active lava lake and onto the crater floor during October (figure 523). Slight variations in the lava lake were noted throughout the month. HVO reported that around 0600 on 3 October the level of the lava lake has lowered slightly. Overflight measurements taken on 5 October indicated that the crater floor was infilled a total of about 143 m and that 111 million cubic meters of lava had been effused since September 2021. During 6-7 October the lake gradually rose 0.5 m. Sulfur dioxide measurements made on 22 October had an emission rate of 700 t/d. Another overflight taken on 28 October showed that there was little to no change in the elevation of the crater floor: the crater floor was infilled a total of 143 m and 111 million cubic meters of lava had erupted since the start of the eruption.

Figure 523. Photo of the Halema’uma’u crater at Kīlauea looking east from the crater rim showing the active lava lake, with active lava ponds to the SE (top) and west (bottom middle) taken on 5 October 2022. The western vent complex is visible through the gas at the bottom center of the photo. Courtesy of N. Deligne, USGS.

Activity during November 2022. Activity remained low during November, though HVO reported that lava from the western vent continued to effuse into the active lava lake and onto the crater floor throughout the month. The rate of sulfur dioxide emissions during November ranged from 300-600 t/d, the higher amount of which occurred on 9 November.

Activity during December 2022. Similar low activity was reported during December, with lava effusing from the western vent into the active lava lake and onto the crater floor. During 4-5 December the active part of the lava lake was slightly variable in elevation and fluctuated within 1 m. On 9 December HVO reported that lava was no longer erupting from the western vent in the Halema’uma’u crater and that sulfur dioxide emissions had returned to near pre-eruption background levels; during 10-11 December, the lava lake had completely crusted over, and no incandescence was visible (figure 524). Time lapse camera images covering the 4-10 December showed that the crater floor showed weak deflation and no inflation. Some passive events of crustal overturning were reported during 14-15 December, which brought fresh incandescent lava to the lake surface. The sulfur dioxide emission rate was approximately 200 t/d on 14 December. A smaller overturn event on 17 December and another that occurred around 0000 and into the morning of 20 December were also detected. A small seismic swarm was later detected on 30 December.

Figure 524. Photo of Halema’uma’u crater at Kīlauea showing a mostly solidified lake surface during the early morning of 10 December 2022. Courtesy of J. Bard, USGS.

Geologic Background. Kilauea overlaps the E flank of the massive Mauna Loa shield volcano in the island of Hawaii. Eruptions are prominent in Polynesian legends; written documentation since 1820 records frequent summit and flank lava flow eruptions interspersed with periods of long-term lava lake activity at Halemaumau crater in the summit caldera until 1924. The 3 x 5 km caldera was formed in several stages about 1,500 years ago and during the 18th century; eruptions have also originated from the lengthy East and Southwest rift zones, which extend to the ocean in both directions. About 90% of the surface of the basaltic shield volcano is formed of lava flows less than about 1,100 years old; 70% of the surface is younger than 600 years. The long-term eruption from the East rift zone between 1983 and 2018 produced lava flows covering more than 100 km2, destroyed hundreds of houses, and added new coastline.

Information Contacts: Hawaiian Volcano Observatory (HVO), U.S. Geological Survey, PO Box 51, Hawai'i National Park, HI 96718, USA (URL: http://hvo.wr.usgs.gov/).

Nyamulagira (also known as Nyamuragira) is a shield volcano in the Democratic Republic of Congo with the summit truncated by a small 2 x 2.3 km caldera with walls up to about 100 m high. Documented eruptions have occurred within the summit caldera, as well as from numerous flank fissures and cinder cones. The current eruption period began in April 2018 and has more recently been characterized by summit crater lava flows and thermal activity (BGVN 48:05). This report describes lava flows and variable thermal activity during May through October 2023, based on information from the Observatoire Volcanologique de Goma (OVG) and various satellite data.

Lava lake activity continued during May. The MIROVA (Middle InfraRed Observation of Volcanic Activity) system recorded moderate-to-strong thermal activity throughout the reporting period; activity was more intense during May and October and relatively weaker from June through September (figure 95). The MODVOLC thermal algorithm, detected a total of 209 thermal alerts. There were 143 hotspots detected during May, eight during June, nine during September, and 49 during October. This activity was also reflected in infrared satellite images, where a lava flow was visible in the NW part of the crater on 7 May and strong activity was seen in the center of the crater on 4 October (figure 96). Another infrared satellite image taken on 12 May showed still active lava flows along the NW margin of the crater. According to OVG lava effusions were active during 7-29 May and moved to the N and NW parts of the crater beginning on 9 May. Strong summit crater incandescence was visible from Goma (27 km S) during the nights of 17, 19, and 20 May (figure 97). On 17 May there was an increase in eruptive activity, which peaked at 0100 on 20 May. Notable sulfur dioxide plumes drifted NW and W during 19-20 May (figure 98). Drone footage acquired in partnership with the USGS (United States Geological Survey) on 20 May captured images of narrow lava flows that traveled about 100 m down the W flank (figure 99). Data from the Rumangabo seismic station indicated a decreasing trend in activity during 17-21 May. Although weather clouds prevented clear views of the summit, a strong thermal signature on the NW flank was visible in an infrared satellite image on 22 May, based on an infrared satellite image. On 28 May the lava flows on the upper W flank began to cool and solidify. By 29 May seismicity returned to levels similar to those recorded before the 17 May increase. Lava effusion continued but was confined to the summit crater; periodic crater incandescence was observed.

Figure 95. Moderate-to-strong thermal anomalies were detected at Nyamulagira during May through October 2023, as shown on this MIROVA graph (Log Radiative Power). During late May, the intensity of the anomalies gradually decreased and remained at relatively lower levels during mid-June through mid-September. During mid-September, the power of the anomalies gradually increased again. The stronger activity is reflective of active lava effusions. Courtesy of MIROVA.

Figure 96. Infrared (bands B12, B11, B4) satellite images showing a constant thermal anomaly of variable intensities in the summit crater of Nyamulagira on 7 May 2023 (top left), 21 June 2023 (top right), 21 July 2023 (bottom left), and 4 October 2023 (bottom right). Although much of the crater was obscured by weather clouds on 7 May, a possible lava flow was visible in the NW part of the crater. Courtesy of Copernicus Browser.

Figure 97. Photo of intense nighttime crater incandescence at Nyamulagira as seen from Goma (27 km S) on the evening of 19 May 2023. Courtesy of Charles Balagizi, OVG.

Figure 98. Two strong sulfur dioxide plumes were detected at Nyamulagira and drifted W on 19 (left) and 20 (right) May 2023. Courtesy of NASA Global Sulfur Dioxide Monitoring Page.

Figure 99. A map (top) showing the active vents (yellow pins) and direction of active lava flows (W) at Nyamulagira at Virunga National Park on 20 May 2023. Drone footage (bottom) also shows the fresh lava flows traveling downslope to the W on 20 May 2023. Courtesy of USGS via OVG.

Low-level activity was noted during June through October. On 1 June OVG reported that seismicity remained at lower levels and that crater incandescence had been absent for three days, though infrared satellite imagery showed continued lava effusion in the summit crater. The lava flows on the flanks covered an estimated 0.6 km². Satellite imagery continued to show thermal activity confined to the lava lake through October (figure 96), although no lava flows or significant sulfur dioxide emissions were reported.

Geologic Background. Africa's most active volcano, Nyamulagira (also known as Nyamuragira), is a massive high-potassium basaltic shield about 25 km N of Lake Kivu and 13 km NNW of the steep-sided Nyiragongo volcano. The summit is truncated by a small 2 x 2.3 km caldera that has walls up to about 100 m high. Documented eruptions have occurred within the summit caldera, as well as from the numerous flank fissures and cinder cones. A lava lake in the summit crater, active since at least 1921, drained in 1938, at the time of a major flank eruption. Recent lava flows extend down the flanks more than 30 km from the summit as far as Lake Kivu; extensive lava flows from this volcano have covered 1,500 km2 of the western branch of the East African Rift.

Information Contacts: Observatoire Volcanologique de Goma (OVG), Departement de Geophysique, Centre de Recherche en Sciences Naturelles, Lwiro, D.S. Bukavu, DR Congo; Hawai'i Institute of Geophysics and Planetology (HIGP) - MODVOLC Thermal Alerts System, School of Ocean and Earth Science and Technology (SOEST), Univ. of Hawai'i, 2525 Correa Road, Honolulu, HI 96822, USA (URL: http://modis.higp.hawaii.edu/); MIROVA (Middle InfraRed Observation of Volcanic Activity), a collaborative project between the Universities of Turin and Florence (Italy) supported by the Centre for Volcanic Risk of the Italian Civil Protection Department (URL: http://www.mirovaweb.it/); NASA Global Sulfur Dioxide Monitoring Page, Atmospheric Chemistry and Dynamics Laboratory, NASA Goddard Space Flight Center (NASA/GSFC), 8800 Greenbelt Road, Goddard, Maryland, USA (URL: https://so2.gsfc.nasa.gov/); Copernicus Browser, Copernicus Data Space Ecosystem, European Space Agency (URL: https://dataspace.copernicus.eu/browser/); Charles Balagizi, Goma Volcano Observatory, Departement de Geophysique, Centre de Recherche en Sciences Naturelles, Lwiro, D.S. Bukavu, DR Congo.

The remote volcano of Bagana is located in central Bougainville Island, Papua New Guinea. Recorded eruptions date back to 1842 and activity has consisted of effusive activity that has built a small lava dome in the summit crater and occasional explosions that produced pyroclastic flows. The most recent eruption has been ongoing since February 2000 and has produced occasional explosions, ash plumes, and lava flows. More recently, activity has been characterized by ongoing effusive activity and ash emissions (BGVN 48:04). This report updates activity from April through September 2023 that has consisted of explosions, ash plumes, ashfall, and lava flows, using information from the Darwin Volcanic Ash Advisory Center (VAAC) and satellite data.

An explosive eruption was reported on 7 July that generated a large gas-and-ash plume to high altitudes and caused significant ashfall in local communities; the eruption plume had reached upper tropospheric (16-18 km altitude) altitudes by 2200, according to satellite images. Sulfur dioxide plumes were detected in satellite images on 8 July and indicated that the plume was likely a mixture of gas, ice, and ash. A report issued by the Autonomous Bougainville Government (ABG) (Torokina District, Education Section) on 10 July noted that significant ash began falling during 2000-2100 on 7 July and covered most areas in the Vuakovi, Gotana (9 km SW), Koromaketo, Laruma (25 km W) and Atsilima (27 km NW) villages. Pyroclastic flows also occurred, according to ground-based reports; small deposits confined to one drainage were inspected by RVO during an overflight on 17 July and were confirmed to be from the 7 July event. Ashfall continued until 10 July and covered vegetation, which destroyed bushes and gardens and contaminated rivers and streams.

RVO reported another eruption on 14 July. The Darwin VAAC stated that an explosive event started around 0830 on 15 July and produced an ash plume that rose to 16.5 km altitude by 1000 and drifted N, according to satellite images. The plume continued to drift N and remained visible through 1900, and by 2150 it had dissipated.

Ashfall likely from both the 7 and 15 July events impacted about 8,111 people in Torokina (20 km SW), including Tsito/Vuakovi, Gotana, Koromaketo, Kenaia, Longkogari, Kenbaki, Piva (13 km SW), and Atsinima, and in the Tsitovi district, according to ABG. Significant ashfall was also reported in Ruruvu (22 km N) in the Wakunai District of Central Bougainville, though the thickness of these deposits could not be confirmed. An evacuation was called for the villages in Wakunai, where heavy ashfall had contaminated water sources; the communities of Ruruvu, Togarau, Kakarapaia, Karauturi, Atao, and Kuritaturi were asked to evacuate to a disaster center at the Wakunai District Station, and communities in Torokina were asked to evacuate to the Piva District station. According to a news article, more than 7,000 people needed temporary accommodations, with about 1,000 people in evacuation shelters. Ashfall had deposited over a broad area, contaminating water supplies, affecting crops, and collapsing some roofs and houses in rural areas. Schools were temporarily shut down. Intermittent ash emissions continued through the end of July and drifted NNW, NW, and SW. Fine ashfall was reported on the coast of Torokina, and ash plumes also drifted toward Laruma and Atsilima.

A small explosive eruption occurred at 2130 on 28 July that ejected material from the crater vents, according to reports from Torokina, in addition to a lava flow that contained two lobes. A second explosion was detected at 2157. Incandescence from the lava flow was visible from Piva as it descended the W flank around 2000 on 29 July (figure 47). The Darwin VAAC reported that a strong thermal anomaly was visible in satellite images during 30-31 July and that ash emissions rose to 2.4 km altitude and drifted WSW on 30 July. A ground report from RVO described localized emissions at 0900 on 31 July.

Figure 47. Infrared (bands B12, B11, B4) satellite images showed weak thermal anomalies at the summit crater of Bagana on 12 April 2023 (top left), 27 May 2023 (top right), 31 July 2023 (bottom left), and 19 September 2023 (bottom right). A strong thermal anomaly was detected through weather clouds on 31 July and extended W from the summit crater. Courtesy of Copernicus Browser.

The Darwin VAAC reported that ash plumes were identified in satellite imagery at 0800 and 1220 on 12 August and rose to 2.1 km and 3 km altitude and drifted NW and W, respectively. A news report stated that aid was sent to more than 6,300 people that were adversely affected by the eruption. Photos taken during 17-19 August showed ash emissions rising no higher than 1 km above the summit and drifting SE. A small explosion generated an ash plume during the morning of 19 August. Deposits from small pyroclastic flows were also captured in the photos. Satellite images captured lava flows and pyroclastic flow deposits. Two temporary seismic stations were installed near Bagana on 17 August at distances of 7 km WSW (Vakovi station) and 11 km SW (Kepox station). The Kepox station immediately started to record continuous, low-frequency background seismicity.

Satellite data. Little to no thermal activity was detected during April through mid-July 2023; only one anomaly was recorded during early April and one during early June, according to MIROVA (Middle InfraRed Observation of Volcanic Activity) data (figure 48). Thermal activity increased in both power and frequency during mid-July through September, although there were still some short gaps in detected activity. MODVOLC also detected increased thermal activity during August; thermal hotspots were detected a total of five times on 19, 20, and 27 August. Weak thermal anomalies were also captured in infrared satellite images on clear weather days throughout the reporting period on 7, 12, and 17 April, 27 May, 1, 6, 16, and 31 July, and 19 September (figure 48); a strong thermal anomaly was visible on 31 July. Distinct sulfur dioxide plumes that drifted generally NW were intermittently captured by the TROPOMI instrument on the Sentinel-5P satellite and sometimes exceeded two Dobson Units (DUs) (figure 49).

Figure 48. Low thermal activity was detected at Bagana during April through mid-July 2023, as shown on this MIROVA graph. In mid-July, activity began to increase in both frequency and power, which continued through September. There were still some pauses in activity during late July, early August, and late September, but a cluster of thermal activity was detected during late August. Courtesy of MIROVA.

Figure 49. Distinct sulfur dioxide plumes rising from Bagana on 15 July 2023 (top left), 16 July 2023 (top right), 17 July 2023 (bottom left), and 17 August 2023 (bottom right). These plumes all generally drifted NW; a particularly notable plume exceeded 2 Dobson Units (DUs) on 15 July. Data is from the TROPOMI instrument on the Sentinel-5P satellite. Courtesy of NASA Global Sulfur Dioxide Monitoring Page.0

Geologic Background. Bagana volcano, in a remote portion of central Bougainville Island, is frequently active. This massive symmetrical cone was largely constructed by an accumulation of viscous andesitic lava flows. The entire edifice could have been constructed in about 300 years at its present rate of lava production. Eruptive activity is characterized by non-explosive effusion of viscous lava that maintains a small lava dome in the summit crater, although occasional explosive activity produces pyroclastic flows. Lava flows with tongue-shaped lobes up to 50 m thick and prominent levees descend the flanks on all sides.

Information Contacts: Rabaul Volcano Observatory (RVO), Geohazards Management Division, Department of Mineral Policy and Geohazards Management (DMPGM), PO Box 3386, Kokopo, East New Britain Province, Papua New Guinea; Darwin Volcanic Ash Advisory Centre (VAAC), Bureau of Meteorology, Northern Territory Regional Office, PO Box 40050, Casuarina, NT 0811, Australia (URL: http://www.bom.gov.au/info/vaac/); MIROVA (Middle InfraRed Observation of Volcanic Activity), a collaborative project between the Universities of Turin and Florence (Italy) supported by the Centre for Volcanic Risk of the Italian Civil Protection Department (URL: http://www.mirovaweb.it/); Hawai'i Institute of Geophysics and Planetology (HIGP) - MODVOLC Thermal Alerts System, School of Ocean and Earth Science and Technology (SOEST), Univ. of Hawai'i, 2525 Correa Road, Honolulu, HI 96822, USA (URL: http://modis.higp.hawaii.edu/); NASA Global Sulfur Dioxide Monitoring Page, Atmospheric Chemistry and Dynamics Laboratory, NASA Goddard Space Flight Center (NASA/GSFC), 8800 Greenbelt Road, Goddard, Maryland, USA (URL: https://so2.gsfc.nasa.gov/); Copernicus Browser, Copernicus Data Space Ecosystem, European Space Agency (URL: https://dataspace.copernicus.eu/browser/); Autonomous Bougainville Government, P.O Box 322, Buka, AROB, PNG (URL: https://abg.gov.pg/); Andrew Tupper (Twitter: @andrewcraigtupp); 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); Radio NZ (URL: https://www.rnz.co.nz/news/pacific/494464/more-than-7-000-people-in-bougainville-need-temporary-accommodation-after-eruption); USAID, 1300 Pennsylvania Ave, NW, Washington DC 20004, USA (URL: https://www.usaid.gov/pacific-islands/press-releases/aug-08-2023-united-states-provides-immediate-emergency-assistance-support-communities-affected-mount-bagana-volcanic-eruptions).

Mayon is located in the Philippines and has steep upper slopes capped by a small summit crater. Historical eruptions date back to 1616 CE that have been characterized by Strombolian eruptions, lava flows, pyroclastic flows, and mudflows. Eruptions mostly originated from a central conduit. Pyroclastic flows and mudflows have commonly descended many of the approximately 40 drainages that surround the volcano. The most recent eruption occurred during June through October 2022 and consisted of lava dome growth and gas-and-steam emissions (BGVN 47:12). A new eruption was reported during late April 2023 and has included lava flows, pyroclastic density currents, ash emissions, and seismicity. This report covers activity during April through September 2023 based on daily bulletins from the Philippine Institute of Volcanology and Seismology (PHIVOLCS).

During April through September 2023, PHIVOLCS reported near-daily rockfall events, frequent volcanic earthquakes, and sulfur dioxide measurements. Gas-and-steam emissions rose 100-900 m above the crater and drifted in different directions. Nighttime crater incandescence was often visible during clear weather and was accompanied by incandescent avalanches of material. Activity notably increased during June when lava flows were reported on the S, SE, and E flanks (figure 52). The MIROVA graph (Middle InfraRed Observation of Volcanic Activity) showed strong thermal activity coincident with these lava flows, which remained active through September (figure 53). According to the MODVOLC thermal algorithm, a total of 110 thermal alerts were detected during the reporting period: 17 during June, 40 during July, 27 during August, and 26 during September. During early June, pyroclastic density currents (PDCs) started to occur more frequently.

Figure 52. Infrared (bands B12, B11, B4) satellite images show strong lava flows descending the S, SE, and E flanks of Mayon on 13 June 2023 (top left), 23 June 2023 (top right), 8 July 2023 (bottom left), and 7 August 2023 (bottom right). Courtesy of Copernicus Browser.

Figure 53. Strong thermal activity was detected at Mayon during early June through September, according to this MIROVA graph (Log Radiative Power) due to the presence of active lava flows on the SE, S, and E flanks. Courtesy of MIROVA.

Low activity was reported during much of April and May; gas-and-steam emissions rose 100-900 m above the crater and generally drifted in different directions. A total of 52 rockfall events and 18 volcanic earthquakes were detected during April and 147 rockfall events and 13 volcanic events during May. Sulfur dioxide flux measurements ranged between 400-576 tons per day (t/d) during April, the latter of which was measured on 29 April and between 162-343 t/d during May, the latter of which was measured on 13 May.

Activity during June increased, characterized by lava flows, pyroclastic density currents (PDCs), crater incandescence and incandescent rockfall events, gas-and-steam emissions, and continued seismicity. Weather clouds often prevented clear views of the summit, but during clear days, moderate gas-and-steam emissions rose 100-2,500 m above the crater and drifted in multiple directions. A total of 6,237 rockfall events and 288 volcanic earthquakes were detected. The rockfall events often deposited material on the S and SE flanks within 700-1,500 m of the summit crater and ash from the events drifted SW, S, SE, NE, and E. Sulfur dioxide emissions ranged between 149-1,205 t/d, the latter of which was measured on 10 June. Short-term observations from EDM and electronic tiltmeter monitoring indicated that the upper slopes were inflating since February 2023. Longer-term ground deformation parameters based on EDM, precise leveling, continuous GPS, and electronic tilt monitoring indicated that the volcano remained inflated, especially on the NW and SE flanks. At 1000 on 5 June the Volcano Alert Level (VAL) was raised to 2 (on a 0-5 scale). PHIVOLCS noted that although low-level volcanic earthquakes, ground deformation, and volcanic gas emissions indicated unrest, the steep increase in rockfall frequency may indicate increased dome activity.

A total of 151 dome-collapse PDCs occurred during 8-9 and 11-30 June, traveled 500-2,000 m, and deposited material on the S flank within 2 km of the summit crater. During 8-9 June the VAL was raised to 3. At approximately 1947 on 11 June lava flow activity was reported; two lobes traveled within 500 m from the crater and deposited material on the S (Mi-isi), SE (Bonga), and E (Basud) flanks. Weak seismicity accompanied the lava flow and slight inflation on the upper flanks. This lava flow remained active through 30 June, moving down the S and SE flank as far as 2.5 km and 1.8 km, respectively and depositing material up to 3.3 km from the crater. During 15-16 June traces of ashfall from the PDCs were reported in Sitio Buga, Nabonton, City of Ligao and Purok, and San Francisco, Municipality of Guinobatan. During 28-29 June there were two PDCs generated by the collapse of the lava flow front, which generated a light-brown ash plume 1 km high. Satellite monitors detected significant concentrations of sulfur dioxide beginning on 29 June. On 30 June PDCs primarily affected the Basud Gully on the E flank, the largest of which occurred at 1301 and lasted eight minutes, based on the seismic record. Four PDCs generated between 1800 and 2000 that lasted approximately four minutes each traveled 3-4 km on the E flank and generated an ash plume that rose 1 km above the crater and drifted N and NW. Ashfall was recorded in Tabaco City.

Similar strong activity continued during July; slow lava effusion remained active on the S and SE flanks and traveled as far as 2.8 km and 2.8 km, respectively and material was deposited as far as 4 km from the crater. There was a total of 6,983 rockfall events and 189 PDCs that affected the S, SE, and E flanks. The volcano network detected a total of 2,124 volcanic earthquakes. Continuous gas-and-steam emissions rose 200-2,000 m above the crater and drifted in multiple directions. Sulfur dioxide emissions averaged 792-4,113 t/d, the latter of which was measured on 28 July. During 2-4 July three PDCs were generated from the collapse of the lava flow and resulting light brown plumes rose 200-300 m above the crater. Continuous tremor pulses were reported beginning at 1547 on 3 July through 7 July at 1200, at 2300 on 8 July and going through 0300 on 10 July, and at 2300 on 16 July, as recorded by the seismic network. During 6-9 July there were 10 lava flow-collapse-related PDCs that generated light brown plumes 300-500 m above the crater. During 10-11 July light ashfall was reported in some areas of Mabinit, Legazpi City, Budiao and Salvacion, Daraga, and Camalig, Albay. By 18 July the lava flow advanced 600 m on the E flank as well.

During 1733 on 18 July and 0434 on 19 July PHIVOLCS reported 30 “ashing” events, which are degassing events accompanied by audible thunder-like sounds and entrained ash at the crater, which produced short, dark plumes that drifted SW. These events each lasted 20-40 seconds, and plume heights ranged from 150-300 m above the crater, as recorded by seismic, infrasound, visual, and thermal monitors. Three more ashing events occurred during 19-20 July. Short-term observations from electronic tilt and GPS monitoring indicate deflation on the E lower flanks in early July and inflation on the NW middle flanks during the third week of July. Longer-term ground deformation parameters from EDM, precise leveling, continuous GPS, and electronic tilt monitoring indicated that the volcano was still generally inflated relative to baseline levels. A short-lived lava pulse lasted 28 seconds at 1956 on 21 July, which was accompanied by seismic and infrasound signals. By 22 July, the only lava flow that remained active was on the SE flank, and continued to extend 3.4 km, while those on the S and E flanks weakened markedly. One ashing event was detected during 30-31 July, whereas there were 57 detected during 31 July-1 August; according to PHIVOLCS beginning at approximately 1800 on 31 July eruptive activity was dominated by phases of intermittent ashing, as well as increased in the apparent rates of lava effusion from the summit crater. The ashing phases consisted of discrete events recorded as low-frequency volcanic earthquakes (LFVQ) typically 30 seconds in duration, based on seismic and infrasound signals. Gray ash plume rose 100 m above the crater and generally drifted NE. Shortly after these ashing events began, new lava began to effuse rapidly from the crater, feeding the established flowed on the SE, E, and E flanks and generating frequent rockfall events.

Intensified unrest persisted during August. There was a total of 4,141 rockfall events, 2,881 volcanic earthquakes, which included volcanic tremor events, 32 ashing events, and 101 PDCs detected throughout the month. On clear weather days, gas-and-steam emissions rose 300-1,500 m above the crater and drifted in different directions (figure 54). Sulfur dioxide emissions averaged 735-4,756 t/d, the higher value of which was measured on 16 August. During 1-2 August the rate of lava effusion decreased, but continued to feed the flows on the SE, S, and E flanks, maintaining their advances to 3.4 km, 2.8 km, and 1.1 km from the crater, respectively (figure 55). Rockfall and PDCs generated by collapses at the lava flow margins and from the summit dome deposited material within 4 km of the crater. During 3-4 August there were 10 tremor events detected that lasted 1-4 minutes. Short-lived lava pulse lasted 35 seconds and was accompanied by seismic and infrasound signals at 0442 on 6 August. Seven collapses were recorded at the front of the lava flow during 12-14 August.

Figure 54. Photo of Mayon showing a white gas-and-steam plume rising 800-1,500 m above the crater at 0645 on 25 August. Courtesy of William Rogers.

Figure 55. Photo of Mayon facing N showing incandescent lava flows and summit crater incandescence taken at 1830 on 25 August 2023. Courtesy of William Rogers.

During September, similar activity of slow lava effusion, PDCs, gas-and-steam emissions, and seismicity continued. There was a total of 4,452 rockfall events, 329 volcanic earthquakes, which included volcanic tremor events, two ashing events, and 85 PDCs recorded throughout the month. On clear weather days, gas-and-steam emissions rose 100-1,500 m above the crater and drifted in multiple directions. Sulfur dioxide emissions averaged 609-2,252 t/d, the higher average of which was measured on 6 September. Slow lava effusion continued advancing on the SE, S, and E flanks, maintaining lengths of 3.4 km, 2.8 km, and 1.1 km, respectively. Rockfall and PDC events generated by collapses along the lava flow margins and at the summit dome deposited material within 4 km of the crater.

Geologic Background. Symmetrical Mayon, which rises above the Albay Gulf NW of Legazpi City, is the most active volcano of the Philippines. The steep upper slopes are capped by a small summit crater. Recorded eruptions since 1616 CE range from Strombolian to basaltic Plinian, with cyclical activity beginning with basaltic eruptions, followed by longer periods of andesitic lava flows. Eruptions occur predominately from the central conduit and have also produced lava flows that travel far down the flanks. Pyroclastic density currents and mudflows have commonly swept down many of the approximately 40 ravines that radiate from the summit and have often damaged populated lowland areas. A violent eruption in 1814 killed more than 1,200 people and devastated several towns.

Information Contacts: Philippine Institute of Volcanology and Seismology (PHIVOLCS), Department of Science and Technology, University of the Philippines Campus, Diliman, Quezon City, Philippines (URL: http://www.phivolcs.dost.gov.ph/); MIROVA (Middle InfraRed Observation of Volcanic Activity), a collaborative project between the Universities of Turin and Florence (Italy) supported by the Centre for Volcanic Risk of the Italian Civil Protection Department (URL: http://www.mirovaweb.it/); Hawai'i Institute of Geophysics and Planetology (HIGP) - MODVOLC Thermal Alerts System, School of Ocean and Earth Science and Technology (SOEST), Univ. of Hawai'i, 2525 Correa Road, Honolulu, HI 96822, USA (URL: http://modis.higp.hawaii.edu/); Copernicus Browser, Copernicus Data Space Ecosystem, European Space Agency (URL: https://dataspace.copernicus.eu/browser/); William Rogers, Legazpi City, Albay Province, Philippines.

Nishinoshima, located about 1,000 km S of Tokyo, is a small island in the Ogasawara Arc in Japan. The island is the summit of a massive submarine volcano that has prominent submarine peaks to the S, W, and NE. Eruptions date back to 1973 and the current eruption period began in October 2022. Recent activity has consisted of small ash plumes and fumarolic activity (BGVN 48:07). This report covers activity during May through August 2023, using information from monthly reports of the Japan Meteorological Agency (JMA) monthly reports and satellite data.

Activity during May through June was relatively low. The Japan Coast Guard (JCG) did overflights on 14 and 22 June and reported white gas-and-steam emissions rising 600 m and 1,200 m from the central crater of the pyroclastic cone, respectively (figure 125). In addition, multiple white gas-and-steam emissions rose from the inner rim of the W side of the crater and from the SE flank of the pyroclastic cone. Discolored brown-to-green water was observed around almost the entire perimeter of the island; on 22 June light green discolored water was observed off the S coast of the island.

Figure 125. A white gas-and-steam plume rising 600 m above the crater of Nishinoshima at 1404 on 14 June 2023 (left) and 1,200 m above the crater at 1249 on 22 June 2023 (right). Courtesy of JCG via JMA (monthly reports of activity at Nishinoshima, June, 2023).

Observations from the Himawari meteorological satellite confirmed an eruption on 9 and 10 July. An eruption plume rose 1.6 km above the crater and drifted N around 1300 on 9 July. Satellite images acquired at 1420 and 2020 on 9 July and at 0220 on 10 July showed continuing emissions that rose 1.3-1.6 km above the crater and drifted NE and N. The Tokyo VAAC reported that an ash plume seen by a pilot and identified in a satellite image at 0630 on 21 July rose to 3 km altitude and drifted S.

Aerial observations conducted by JCG on 8 August showed a white-and-gray plume rising from the central crater of the pyroclastic cone, and multiple white gas-and-steam emissions were rising from the inner edge of the western crater and along the NW-SE flanks of the island (figure 126). Brown-to-green discolored water was also noted around the perimeter of the island.

Figure 126. Aerial photo of Nishinoshima showing a white-and-gray plume rising from the central crater taken at 1350 on 8 August 2023.

Intermittent low-to-moderate power thermal anomalies were recorded in the MIROVA graph (Middle InfraRed Observation of Volcanic Activity), showing an increase in both frequency and power beginning in July (figure 127). This increase in activity coincides with eruptive activity on 9 and 10 July, characterized by eruption plumes. According to the MODVOLC thermal alert algorithm, one thermal hotspot was recorded on 20 July. Weak thermal anomalies were also detected in infrared satellite imagery, accompanied by strong gas-and-steam plumes (figure 128).

Figure 127. Low-to-moderate power thermal anomalies were detected at Nishinoshima during May through August 2023, showing an increase in both frequency and power in July, according to this MIROVA graph (Log Radiative Power). Courtesy of MIROVA.

Figure 128. Infrared (bands B12, B11, B4) satellite images showing a small thermal anomaly at the crater of Nishinoshima on 30 June 2023 (top left), 3 July 2023 (top right), 7 August 2023 (bottom left), and 27 August 2023 (bottom right). Strong gas-and-steam plumes accompanied this activity, extending NW, NE, and SW. Courtesy of Copernicus Browser.

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

Information Contacts: Japan Meteorological Agency (JMA), 1-3-4 Otemachi, Chiyoda-ku, Tokyo 100-8122, Japan (URL: http://www.jma.go.jp/jma/indexe.html); Tokyo Volcanic Ash Advisory Center (VAAC), 1-3-4 Otemachi, Chiyoda-ku, Tokyo 100-8122, Japan (URL: http://ds.data.jma.go.jp/svd/vaac/data/); 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/).

Krakatau is located in the Sunda Strait between Java and Sumatra, Indonesia. Caldera collapse during the catastrophic 1883 eruption destroyed Danan and Perbuwatan cones and left only a remnant of Rakata. The post-collapse cone of Anak Krakatau (Child of Krakatau) was constructed within the 1883 caldera at a point between the former Danan and Perbuwatan cones; it has been the site of frequent eruptions since 1927. The current eruption period began in May 2021 and has recently consisted of Strombolian eruptions and ash plumes (BGVN 48:07). This report describes lower levels of activity consisting of ash and white gas-and-steam plumes during May through August 2023, based on information provided by the Indonesian Center for Volcanology and Geological Hazard Mitigation, referred to as Pusat Vulkanologi dan Mitigasi Bencana Geologi (PVMBG), MAGMA Indonesia, and satellite data.

Activity was relatively low during May and June. Daily white gas-and-steam emissions rose 25-200 m above the crater and drifted in different directions. Five ash plumes were detected at 0519 on 10 May, 1241 on 11 May, 0920 on 12 May, 2320 on 12 May, and at 0710 on 13 May, and rose 1-2.5 km above the crater and drifted SW. A webcam image taken on 12 May showed ejection of incandescent material above the vent. A total of nine ash plumes were detected during 6-11 June: at 1434 and 00220 on 6 and 7 June the ash plumes rose 500 m above the crater and drifted NW, at 1537 on 8 June the ash plume rose 1 km above the crater and drifted SW, at 0746 and at 0846 on 9 June the ash plumes rose 800 m and 3 km above the crater and drifted SW, respectively, at 0423, 1431, and 1750 on 10 June the ash plumes rose 2 km, 1.5 km, and 3.5 km above the crater and drifted NW, respectively, and at 0030 on 11 June an ash plume rose 2 km above the crater and drifted NW. Webcam images taken on 10 and 11 June at 0455 and 0102, respectively, showed incandescent material ejected above the vent. On 19 June an ash plume at 0822 rose 1.5 km above the crater and drifted SE.

Similar low activity of white gas-and-steam emissions and few ash plumes were reported during July and August. Daily white gas-and-steam emissions rose 25-300 m above the crater and drifted in multiple directions. Three ash plumes were reported at 0843, 0851, and 0852 on 20 July that rose 500-2,000 m above the crater and drifted NW.

The MIROVA (Middle InfraRed Observation of Volcanic Activity) graph of MODIS thermal anomaly data showed intermittent low-to-moderate power thermal anomalies during May through August 2023 (figure 140). Although activity was often obscured by weather clouds, a thermal anomaly was visible in an infrared satellite image of the crater on 12 May, accompanied by an eruption plume that drifted SW (figure 141).

Figure 140. Intermittent low-to-moderate power thermal anomalies were detected at Krakatau during May through August 2023, based on this MIROVA graph (Log Radiative Power). Courtesy of MIROVA.

Figure 141. A single thermal anomaly (bright yellow-orange) was visible at Krakatau in this infrared (bands B12, B11, B4) satellite image taken on 12 May 2023. An eruption plume accompanied the thermal anomaly and drifted SW. Courtesy of Copernicus Browser.

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

Information Contacts: Pusat Vulkanologi dan Mitigasi Bencana Geologi (PVMBG, also known as Indonesian Center for Volcanology and Geological Hazard Mitigation, CVGHM), Jalan Diponegoro 57, Bandung 40122, Indonesia (URL: http://www.vsi.esdm.go.id/); MAGMA Indonesia, Kementerian Energi dan Sumber Daya Mineral (URL: https://magma.esdm.go.id/v1); 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/).

Villarrica, in central Chile, consists of a 2-km-wide caldera that formed about 3,500 years ago and is located at the base of the presently active cone at the NW margin of a 6-km-wide caldera. Historical eruptions 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 nighttime crater incandescence, ash emissions, and seismicity (BGVN 48:04). This report covers activity during April through September 2023 and describes occasional Strombolian activity, gas-and-ash emissions, and nighttime 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 April consisted of long period (LP) events and tremor (TRE); a total of 9,413 LP-type events and 759 TR-type events were detected throughout the month. Nighttime crater incandescence persisted and was visible in the degassing column. Sulfur dioxide data was obtained using Differential Absorption Optical Spectroscopy Equipment (DOAS) that showed an average value of 1,450 ± 198 tons per day (t/d) during 1-15 April and 1,129 ± 201 t/d during 16-30 April, with a maximum daily value of 2,784 t/d on 9 April. Gas-and-steam emissions of variable intensities rose above the active crater as high as 1.3 km above the crater on 13 April. Strombolian explosions were not observed and there was a slight decrease in the lava lake level.

There were 14,123 LP-type events and 727 TR-type events detected during May. According to sulfur dioxide measurements taken with DOAS equipment, the active crater emitted an average value of 1,826 ± 482 t/d during 1-15 May and 912 ± 41 t/d during 16-30 May, with a daily maximum value of 5,155 t/d on 13 May. Surveillance cameras showed continuous white gas-and-steam emissions that rose as high as 430 m above the crater on 27 May. Nighttime incandescence illuminated the gas column less than 300 m above the crater rim was and no pyroclastic emissions were reported. A landslide was identified on 13 May on the E flank of the volcano 50 m from the crater rim and extending 300 m away; SERNAGEOMIN noted that this event may have occurred on 12 May. During the morning of 27 and 28 May minor Strombolian explosions characterized by incandescent ejecta were recorded at the crater rim; the last reported Strombolian explosions had occurred at the end of March.

Seismic activity during June consisted of five volcano-tectonic (VT)-type events, 21,606 LP-type events, and 2,085 TR-type events. The average value of sulfur dioxide flux obtained by DOAS equipment was 1,420 ± 217 t/d during 1-15 June and 2,562 ± 804 t/d, with a maximum daily value of 4,810 t/d on 17 June. White gas-and-steam emissions rose less than 480 m above the crater; frequent nighttime crater incandescence was reflected in the degassing plume. On 12 June an emission rose 100 m above the crater and drifted NNW. On 15 June one or several emissions resulted in ashfall to the NE as far as 5.5 km from the crater, based on a Skysat satellite image. Several Strombolian explosions occurred within the crater; activity on 15 June was higher energy and ejected blocks 200-300 m on the NE slope. Surveillance cameras showed white gas-and-steam emissions rising 480 m above the crater on 16 June. On 19 and 24 June low-intensity Strombolian activity was observed, ejecting material as far as 200 m from the center of the crater to the E.

During July, seismicity included 29,319 LP-type events, 3,736 TR-type events, and two VT-type events. DOAS equipment recorded two days of sulfur dioxide emissions of 4,220 t/d and 1,009 t/d on 1 and 13 July, respectively. Constant nighttime incandescence was also recorded and was particularly noticeable when accompanied by eruptive columns on 12 and 16 July. Minor explosive events were detected in the crater. According to Skysat satellite images taken on 12, 13, and 16 July, ashfall deposits were identified 155 m S of the crater. According to POVI, incandescence was visible from two vents on the crater floor around 0336 on 12 July. Gas-and-ash emissions rose as high as 1.2 km above the crater on 13 July and drifted E and NW. A series of gas-and-steam pulses containing some ash deposited material on the upper E flank around 1551 on 13 July. During 16-31 July, average sulfur dioxide emissions of 1,679 ± 406 t/d were recorded, with a maximum daily value of 2,343 t/d on 28 July. Fine ash emissions were also reported on 16, 17, and 23 July.

Seismicity persisted during August, characterized by 27,011 LP-type events, 3,323 TR-type events, and three VT-type events. The average value of sulfur dioxide measurements taken during 1-15 August was 1,642 ± 270 t/d and 2,207 ± 4,549 t/d during 16-31 August, with a maximum daily value of 3,294 t/d on 27 August. Nighttime crater incandescence remained visible in degassing columns. White gas-and-steam emissions rose 480 m above the crater on 6 August. According to a Skysat satellite image from 6 August, ash accumulation was observed proximal to the crater and was mainly distributed toward the E slope. White gas-and-steam emissions rose 320 m above the crater on 26 August. Nighttime incandescence and Strombolian activity that generated ash emissions were reported on 27 August.

Seismicity during September was characterized by five VT-type events, 12,057 LP-type events, and 2,058 TR-type events. Nighttime incandescence persisted. On 2 September an ash emission rose 180 m above the crater and drifted SE at 1643 (figure 125) and a white gas-and-steam plume rose 320 m above the crater. According to the Buenos Aires VAAC, periods of continuous gas-and-ash emissions were visible in webcam images from 1830 on 2 September to 0110 on 3 September. Strombolian activity was observed on 2 September and during the early morning of 3 September, the latter event of which generated an ash emission that rose 60 m above the crater and drifted 100 m from the center of the crater to the NE and SW. Ashfall was reported to the SE and S as far as 750 m from the crater. The lava lake was active during 3-4 September and lava fountaining was visible for the first time since 26 March 2023, according to POVI. Fountains captured in webcam images at 2133 on 3 September and at 0054 on 4 September rose as high as 60 m above the crater rim and ejected material onto the upper W flank. Sulfur dioxide flux of 1,730 t/d and 1,281 t/d was measured on 3 and 4 September, respectively, according to data obtained by DOAS equipment.

Figure 125. Webcam image of a gray ash emission rising above Villarrica on 2 September 2023 at 1643 (local time) that rose 180 m above the crater and drifted SE. Courtesy of SERNAGEOMIN (Reporte Especial de Actividad Volcanica (REAV), Region De La Araucania y Los Rios, Volcan Villarrica, 02 de septiembre de 2023, 17:05 Hora local).

Strong Strombolian activity and larger gas-and-ash plumes were reported during 18-20 September. On 18 September activity was also associated with energetic LP-type events and notable sulfur dioxide fluxes (as high as 4,277 t/d). On 19 September Strombolian activity and incandescence were observed. On 20 September at 0914 ash emissions rose 50 m above the crater and drifted SSE, accompanied by Strombolian activity that ejected material less than 100 m SSE, causing fall deposits on that respective flank. SERNAGEOMIN reported that a Planet Scope satellite image taken on 20 September showed the lava lake in the crater, measuring 32 m x 35 m and an area of 0.001 km². Several ash emissions were recorded at 0841, 0910, 1251, 1306, 1312, 1315, and 1324 on 23 September and rose less than 150 m above the crater. The sulfur dioxide flux value was 698 t/d on 23 September and 1,097 t/d on 24 September. On 24 September the Volcanic Alert Level (VAL) was raised to Orange (the third level on a four-color scale). SENAPRED maintained the Alert Level at Yellow (the middle level on a three-color scale) for the communities of Villarrica, Pucón (16 km N), Curarrehue, and Panguipulli.

During 24-25 September there was an increase in seismic energy (observed at TR-events) and acoustic signals, characterized by 1 VT-type event, 213 LP-type events, and 124 TR-type events. Mainly white gas-and-steam emissions, in addition to occasional fine ash emissions were recorded. During the early morning of 25 September Strombolian explosions were reported and ejected material 250 m in all directions, though dominantly toward the NW. On 25 September the average value of sulfur dioxide flux was 760 t/d. Seismicity during 25-30 September consisted of five VT-type events, 1,937 LP-type events, and 456 TR-type events.

During 25-29 September moderate Strombolian activity was observed and ejected material as far as the crater rim. In addition, ash pulses lasting roughly 50 minutes were observed around 0700 and dispersed ENE. During 26-27 September a TR episode lasted 6.5 hours and was accompanied by discrete acoustic signals. Satellite images from 26 September showed a spatter cone on the crater floor with one vent that measured 10 x 14 m and a smaller vent about 35 m NE of the cone. SERNAGEOMIN reported an abundant number of bomb-sized blocks up to 150 m from the crater, as well as impact marks on the snow, which indicated explosive activity. A low-altitude ash emission was observed drifting NW around 1140 on 28 September, based on webcam images. Between 0620 and 0850 on 29 September an ash emission rose 60 m above the crater and drifted NW. During an overflight taken around 1000 on 29 September scientists observed molten material in the vent, a large accumulation of pyroclasts inside the crater, and energetic degassing, some of which contained a small amount of ash. Block-sized pyroclasts were deposited on the internal walls and near the crater, and a distal ash deposit was also visible. The average sulfur dioxide flux measured on 28 September was 344 t/d. Satellite images taken on 29 September ashfall was deposited roughly 3 km WNW from the crater and nighttime crater incandescence remained visible. The average sulfur dioxide flux value from 29 September was 199 t/d. On 30 September at 0740 a pulsating ash emission rose 1.1 km above the crater and drifted NNW (figure 126). Deposits on the S flank extended as far as 4.5 km from the crater rim, based on satellite images from 30 September.

Figure 126. Webcam image of a gray ash plume rising 1.1 km above the crater of Villarrica at 0740 (local time) on 30 September 2023. Courtesy of SERNAGEOMIN (Reporte Especial de Actividad Volcanica (REAV), Region De La Araucania y Los Rios, Volcan Villarrica, 30 de septiembre de 2023, 09:30 Hora local).

Infrared MODIS satellite data processed by MIROVA (Middle InfraRed Observation of Volcanic Activity) showed intermittent thermal activity during April through September, with slightly stronger activity detected during late September (figure 127). Small clusters of thermal activity were detected during mid-June, early July, early August, and late September. According to the MODVOLC thermal alert system, a total of four thermal hotspots were detected on 7 July and 3 and 23 September. This activity was also intermittently captured in infrared satellite imagery on clear weather days (figure 128).

Figure 127. Low-to-moderate power thermal anomalies were detected at Villarrica during April through September 2023, according to this MIROVA graph (Log Radiative Power). Activity was relatively low during April through mid-June. Small clusters of activity occurred during mid-June, early July, early August, and late September. Courtesy of MIROVA.

Figure 128. Consistent bright thermal anomalies (bright yellow-orange) were visible at the summit crater of Villarrica in infrared (bands B12, B11, B4) satellite images, as shown on 17 June 2023 (top left), 17 July 2023 (top right), 6 August 2023 (bottom left), and 20 September 2023 (bottom right). Courtesy of Copernicus Browser.

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/); Sistema y Servicio Nacional de Prevención y Repuesta Ante Desastres (SENAPRED), Av. Beauchef 1671, Santiago, Chile (URL: https://web.senapred.cl/); 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/); Copernicus Browser, Copernicus Data Space Ecosystem, European Space Agency (URL: https://dataspace.copernicus.eu/browser/).

Merapi, located just north of the major city of Yogyakarta in central Java, Indonesia, has had activity within the last 20 years characterized by pyroclastic flows and lahars accompanying growth and collapse of the steep-sided active summit lava dome. The current eruption period began in late December 2020 and has more recently consisted of ash plumes, intermittent incandescent avalanches of material, and pyroclastic flows (BGVN 48:04). This report covers activity during April through September 2023, based on information from Balai Penyelidikan dan Pengembangan Teknologi Kebencanaan Geologi (BPPTKG), the Center for Research and Development of Geological Disaster Technology, a branch of PVMBG which specifically monitors Merapi. Additional information comes from the Pusat Vulkanologi dan Mitigasi Bencana Geologi (PVMBG, also known as Indonesian Center for Volcanology and Geological Hazard Mitigation, CVGHM), MAGMA Indonesia, the Darwin Volcanic Ash Advisory Centre (VAAC), and various satellite data.

Activity during April through September 2023 primarily consisted of incandescent avalanches of material that mainly affected the SW and W flanks and traveled as far as 2.3 km from the summit (table 25) and white gas-and-steam emissions that rose 10-1,000 m above the crater.

Table 25. Monthly summary of avalanches and avalanche distances recorded at Merapi during April through September 2023. The number of reported avalanches does not include instances where possible avalanches were heard but could not be visually confirmed as a result of inclement weather. Data courtesy of BPPTKG (April-September 2023 daily reports).

BPPTKG reported that during April and May white gas-and-steam emissions rose 10-750 m above the crater, incandescent avalanches descended 500-2,000 m on the SW and W flanks (figure 135). Cloudy weather often prevented clear views of the summit, and sometimes avalanches could not be confirmed. According to a webcam image, a pyroclastic flow was visible on 17 April at 0531. During the week of 28 April and 4 May a pyroclastic flow was reported on the SW flank, traveling up to 2.5 km. According to a drone overflight taken on 17 May the SW lava dome volume was an estimated 2,372,800 cubic meters and the dome in the main crater was an estimated 2,337,300 cubic meters.

Figure 135. Photo showing an incandescent avalanche affecting the flank of Merapi on 8 April 2023. Courtesy of Øystein Lund Andersen.

During June and July similar activity persisted with white gas-and-steam emissions rising 10-350 m above the crater and frequent incandescent avalanches that traveled 300-2,000 m down the SW, W, and S flanks (figure 136). Based on an analysis of aerial photos taken on 24 June the volume of the SW lava dome was approximately 2.5 million cubic meters. A pyroclastic flow was observed on 5 July that traveled 2.7 km on the SW flank. According to the Darwin VAAC multiple minor ash plumes were identified in satellite images on 19 July that rose to 3.7 km altitude and drifted S and SW. During 22, 25, and 26 July a total of 17 avalanches descended as far as 1.8 km on the S flank.

Figure 136. Photo showing an incandescent avalanche descending the flank of Merapi on 23 July 2023. Courtesy of Øystein Lund Andersen.

Frequent white gas-and-steam emissions continued during August and September, rising 10-450 m above the crater. Incandescent avalanches mainly affected the SW and W flanks and traveled 400-2,300 m from the vent (figure 137). An aerial survey conducted on 10 August was analyzed and reported that estimates of the SW dome volume was 2,764,300 cubic meters and the dome in the main crater was 2,369,800 cubic meters.

Figure 137. Photo showing a strong incandescent avalanche descending the flank of Merapi on 23 September 2023. Courtesy of Øystein Lund Andersen.

Frequent and moderate-power thermal activity continued throughout the reporting period, according to a MIROVA (Middle InfraRed Observation of Volcanic Activity) analysis of MODIS satellite data (figure 138). There was an increase in the number of detected anomalies during mid-May. The MODVOLC thermal algorithm recorded a total of 47 thermal hotspots: six during April, nine during May, eight during June, 15 during July, four during August, and five during September. Some of this activity was captured in infrared satellite imagery on clear weather days, sometimes accompanied by incandescent material on the SW flank (figure 139).

Figure 138. Frequent and moderate-power thermal anomalies were detected at Merapi during April through September 2023, as shown on this MIROVA plot (Log Radiative Power). There was an increase in the number of anomalies recorded during mid-May. Courtesy of MIROVA.

Figure 139. Infrared (bands B12, B11, B4) satellite images showed a consistent thermal anomaly (bright yellow-orange) at the summit crater of Merapi on 8 April 2023 (top left), 18 May 2023 (top right), 17 June 2023 (middle left), 17 July 2023 (middle right), 11 August 2023 (bottom left), and 20 September 2023 (bottom right). Incandescent material was occasionally visible descending the SW flank, as shown in each of these images. Courtesy of Copernicus Browser.

Geologic Background. Merapi, one of Indonesia's most active volcanoes, lies in one of the world's most densely populated areas and dominates the landscape immediately north of the major city of Yogyakarta. It is the youngest and southernmost of a volcanic chain extending NNW to Ungaran volcano. Growth of Old Merapi during the Pleistocene ended with major edifice collapse perhaps about 2,000 years ago, leaving a large arcuate scarp cutting the eroded older Batulawang volcano. Subsequent growth of the steep-sided Young Merapi edifice, its upper part unvegetated due to frequent activity, began SW of the earlier collapse scarp. Pyroclastic flows and lahars accompanying growth and collapse of the steep-sided active summit lava dome have devastated cultivated lands on the western-to-southern flanks and caused many fatalities.

Information Contacts: Balai Penyelidikan dan Pengembangan Teknologi Kebencanaan Geologi (BPPTKG), Center for Research and Development of Geological Disaster Technology (URL: http://merapi.bgl.esdm.go.id/, Twitter: @BPPTKG); MAGMA Indonesia, Kementerian Energi dan Sumber Daya Mineral (URL: https://magma.esdm.go.id/v1); Pusat Vulkanologi dan Mitigasi Bencana Geologi (PVMBG, also known as Indonesian Center for Volcanology and Geological Hazard Mitigation, CVGHM), Jalan Diponegoro 57, Bandung 40122, Indonesia (URL: http://www.vsi.esdm.go.id/); Darwin Volcanic Ash Advisory Centre (VAAC), Bureau of Meteorology, Northern Territory Regional Office, PO Box 40050, Casuarina, NT 0811, Australia (URL: http://www.bom.gov.au/info/vaac/); MIROVA (Middle InfraRed Observation of Volcanic Activity), a collaborative project between the Universities of Turin and Florence (Italy) supported by the Centre for Volcanic Risk of the Italian Civil Protection Department (URL: http://www.mirovaweb.it/); Hawai'i Institute of Geophysics and Planetology (HIGP) - MODVOLC Thermal Alerts System, School of Ocean and Earth Science and Technology (SOEST), Univ. of Hawai'i, 2525 Correa Road, Honolulu, HI 96822, USA (URL: http://modis.higp.hawaii.edu/); Copernicus Browser, Copernicus Data Space Ecosystem, European Space Agency (URL: https://dataspace.copernicus.eu/browser/); Øystein Lund Andersen (URL: https://www.oysteinlundandersen.com/, https://twitter.com/oysteinvolcano).

Ebeko, located on the N end of Paramushir Island in Russia’s Kuril Islands just S of the Kamchatka Peninsula, consists of three summit craters along a SSW-NNE line at the northern end of a complex of five volcanic cones. Observed eruptions date back to the late 18th century and have been characterized as small-to-moderate explosions from the summit crater, accompanied by intense fumarolic activity. The current eruptive period began in June 2022, consisting of frequent explosions, ash plumes, and thermal activity (BGVN 47:10, 48:06). This report covers similar activity during June-November 2023, based on information from the Kamchatka Volcanic Eruptions Response Team (KVERT) and satellite data.

Moderate explosive activity continued during June-November 2023 (figures 50 and 51). According to visual data from Severo-Kurilsk, explosions sent ash 2-3.5 km above the summit (3-4.5 km altitude) during most days during June through mid-September. Activity after mid-September was slightly weaker, with ash usually reaching less than 2 km above the summit. According to KVERT the volcano in October and November was, with a few exceptions, either quiet or obscured by clouds that prevented satellite observations. KVERT issued Volcano Observatory Notices for Aviation (VONA) on 8 and 12 June, 13 and 22 July, 3 and 21 August, and 31 October warning of potential aviation hazards from ash plumes drifting 3-15 km from the volcano. Based on satellite data, KVERT reported a persistent thermal anomaly whenever weather clouds permitted viewing.

Figure 50. Ash explosion from the active summit crater of Ebeko on 18 July 2023; view is approximately towards the W. Photo provided by I. Bolshakov and M.V. Lomonosov MGU; courtesy of KVERT.

Figure 51. Ash explosion from the active summit crater of Ebeko on 23 July 2023 with lightning visible in the lower part of the plume. Photo provided by I. Bolshakov and M.V. Lomonosov MGU; courtesy of KVERT.

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

Information Contacts: Kamchatka Volcanic Eruptions Response Team (KVERT), Far Eastern Branch, Russian Academy of Sciences, 9 Piip Blvd., Petropavlovsk-Kamchatsky, 683006, Russia (URL: http://www.kscnet.ru/ivs/kvert/).

Our last report covered the explosive eruptions of 2-3 October 2009 from two of Sakura-jima's active vents: Minami-dake and Showa (BGVN 34:08) (figure 33). Minami-dake was last active on 22 February 2009. This report covers Sakura-jima's activity from October 2009 through October 2011; datasets may have various termination dates due to availability.

Figure 33. Location of Sakura-jima; surrounded by Kagoshima Bay and connected to the mainland of Kyushu, Japan by lava flows from 1914 AD (SW side of the island). Satellite image courtesy of Japan Aerospace Exploration Agency (JAXA) and index map from MapsOf.net.

The ash plumes of October 2009 to October 2011 reported by the Tokyo Volcanic Ash Advisory Center (VAAC) were disclosed in pilot's reports and satellite observations. Plume heights had a maximum altitude range of 1.2 to 4.9 km. VAAC released regular advisories during this time period, often more than once each week.

For the next 11 months following the explosive 2-3 October 2009 events, the Japan Meteorological Agency (JMA) maintained Alert Level 3 status due to intense eruptions from Showa crater (figure 34). The five-tier alert system used by JMA assigns red alert to Level 5; a Level 3 status forbids anyone to approach the volcano. Activity was occasionally Strombolian and Vulcanian during this time period. Lava fountaining on 8 February 2010 reached 1,000 m above the crater; this activity was visible at night and lightning was observed within the ash plume.

Figure 34. Plume heights and documented explosions for Sakura-jima's primary eruptive vents: Minami-dake (top) and Showa (bottom). Data is plotted for January 2009 through July 2011. Courtesy of JMA.

On 30 May 2010 an ash plume rose 2.8 km from Showa crater. A small pyroclastic flow was documented on the E flank (figure 35). A camera located at the Ohsumi National Office of Rivers and Highways recorded the vertical plume and pyroclastic flow with both visible and thermal images. The pyroclastic flow traveled ~ 700 m and had temperatures up to 500°C above the background levels.

Figure 35. An ash plume rose up to an altitude of 2.8 km from Sakura-jima's Showa crater and a pyroclastic flow traveled down the E flank. The eruption occurred at 1140 on 30 May 2010 and was captured by visual photography and a thermal camera. Courtesy of JMA.

Explosions were numerous in 2010 and according to JMA, by 20 June a new record had been reached; 550 explosions had already occurred at Sakura-jima. The Japan Times reported that the previous record high in a single year was 548 in 2009. By September 2010, this activity was less vigorous; the plumes from Showa crater were frequently less than 1 km high and no additional activity was reported from Minami-dake. On 30 September, JMA reduced the Alert Level but maintained warnings that no one should approach the summit craters. Earthquakes and tremor had become rare and constant deflation was recorded by tiltmeter and GPS. By June 2010, the long trend of inflation recorded by the water-tube tiltmeter at Arimura station peaked and in early July, abruptly began measuring deflation (figure 36).

Figure 36. Tilt change at Sakura-jima observed by the water-tube tiltmeter at Arimura station from January 2009 to September 2011. Tidal response was corrected and inflation at the summit corresponds to positive tilt. In the bottom panel, the red bars denote monthly frequencies of explosions from Showa crater. Courtesy of JMA.

From 7 to 20 October 2010, explosive eruptions became more frequent and exceeded background levels from the previous month. A large explosion on 13 October produced ejecta that reached ~ 1.3 km from Showa crater. Earthquake activity was consistently low, but elevated levels of tremor were recorded prompting JMA to raise the Alert Level to 3. During the subsequent months, explosive, ash-rich plumes became more frequent, increasing from 59 in November, and 62 in December, to 102 in January.

Activity was concentrated within the Showa crater until February 2011 when renewed activity began simultaneously at Minami-dake. Last active on 3 October 2009, the summit crater of Minami-dake released two ash-rich plumes on 7 February 2011. Volcanic bombs from Showa crater landed 0.8-1.3 km from the crater. At 1908 on 19 February, a pyroclastic flow extended ~ 500 m down the SE flank. JMA recorded 144 explosions that month, 110 of these events produced ash.

Incandescence and pyroclastic flows from Showa crater. Explosive eruptions continued at a lower rate during the following months; observers however, noted incandescence from Sakura-jima's summit from March through September 2011. An explosive eruption at 2242 on 30 April was recorded from Showa crater and was accompanied by a pyroclastic flow that extended 600 m from the crater on the E flank. Smaller pyroclastic flows 200-400 m in length occurred on 5 June, 12 July, and 1 and 12 September. These events traveled E and SE from the Showa crater and were recorded by thermal cameras and observers.

Aerial surveillance. Aerial observations of Showa crater were made on 31 May 2011 by JMA in cooperation with the Japan Maritime Self Defense Force (JMSDF). Fresh lava was discovered covering part of the crater floor with a diameter of 50-60 m (figure 37). Thermal results determined that the hottest area was in the center of the lava with temperatures up to 500°C above the measured background.

Figure 37. Sakura-jima's Showa crater on 31 May 2011. Aerial observations (A) and thermal imaging (B) determined the presence of new lava (appears black in plain light but has a high thermal output). Courtesy of JMA-JMSDF.

During the 31 May overflight, two ponds of water were identified within the Minami-dake vent. Both craters, A and B, contained water (figure 38) that persisted through 11 July, and by August the volume of water appeared to have increased in crater A. Observations from an aerial survey on 30 August found the ponds differed in color: Crater A appeared light blue, and Crater B was red-brown. There was no apparent change in the amount of degassing from these craters.

Figure 38. Sakura-jima's Minami-dake vent on 31 May and 11 July 2011. Aerial observations determined that water was collecting in craters A and B. Activity had not been recorded from this site since 7 February 2011. Courtesy of JMA-JMSDF.

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

Information Contacts: Tokyo Volcanic Ash Advisory Center (VAAC), Tokyo, Japan (URL: http://ds.data.jma.go.jp/svd/vaac/data/); Japan Meteorological Agency (JMA), Otemachi, 1-3-4, Chiyoda-ku Tokyo 100-8122, Japan (URL: http://www.jma.go.jp/); JAXA (URL: http://www.eorc.jaxa.jp/en/earthview/2011/tp110223.html); MapsOf.Net (URL: http://mapsof.net/).

Volcanic activity at Concepción Volcano from 2007 through 2009 was characterized by intermittent, explosive eruptions of ash. Our last report, BGVN 34:11, highlighted the extent of ashfall from these eruptions and the declining frequency of explosions from 9 February through 11 December 2009. New activity reported below begins with a sequence of ash eruptions from January 2010 through early April 2010. Recent mitigation efforts are also discussed that include evacuation drills in January 2010, an international conference held in Managua with site visits to Ometepe Island in November 2010, and a new GPS network (called CONCEPTEPE).

Seismicity for the past five years from Concepción Volcano has been summarized by the Instituto Nicarag?ense de Estudios Territoriales (INETER). Low tremor (around 0.5 Hz) was frequently recorded during this time period and sporadic volcano-tectonic (VT) events occurred every 4-5 months. They also noted that intermittent summit explosions followed the same 4-5 month pattern.

Escalation and summit eruption. Volcanic unrest at Concepción Volcano from January through February 2010 was marked by few direct observations and isolated seismic events. On 27 January a small summit explosion was observed although there was no associated seismic signal; ash was not detected by weather satellites and no VAAC notices were released. Banded tremor was detected by INETER stations (2 installations are on Ometepe Island) on 11 February lasting for about 5 minutes, but there were no signs of degassing or explosions. Banded tremor is a term describing a pattern of regular increase and decrease in tremor appearing on a seismic drum (McNutt 1992), also known as intermittent volcanic tremor (IVT) (Gresta and others, 1996).

A series of explosions from Concepción's summit occurred suddenly on 7 March 2010. Low-level tremor appeared in the afternoon on 8 March and, in total, 14 ash-and-gas explosions were recorded that day (figure 5). Observers on Ometepe reported regular plume heights of ~ 1 km above the crater, and ash fell >10 km across the SW sector of the island reaching the communities Moyogalpa, Los Angeles, Esquipulas, and San José del Sur (ABC Digital). The Washington Volcanic Ash Advisory Center (VAAC) reported a 2.1 km-high plume drifting W.

Figure 5. The number of daily explosions plotted over time for Concepción volcano. This time period covers the height of activity from 8-17 March 2010. Courtesy of INETER.

By 9 March, episodes of banded tremor prevailed for over 5 minutes and the number of small explosions doubled.

On 11 March, tremor increased by 180 RSAM units (Real-time Seismic-Amplitude Measurement) and explosions were often recorded as impulsive with RSAM values of 300 (figure 6). The highest RSAM value occurred at 1440 reaching ~ 1,100. Throughout the day there were small gas-and-ash explosions and banded tremor increased slightly.

Figure 6. RSAM plot from Concepción volcano for 8-17 March 2010. X-axis is reported as Days/Hours/Minutes. Courtesy of INETER.

At 0759 on 12 March an M 4.6 earthquake occurred along the coast of San Juan del Sur, ~ 100 km W of the volcano. Forty minutes after this regional earthquake, INETER reported one of the strongest ash explosions from Concepción. Residents of La Sabana, Altagracia, and neighboring communities reported ashfall at 1940 that day (noticias.com). The resulting plume was detected by weather satellites and reported in a VAAC advisory. Ash reached an altitude of ~ 3 km and drifted SE. Tremor continued to be recorded during the day by INETER instruments.

In the March 2010 report, INETER highlighted seismic events and noted that, during the first 10 days of activity, no VT events were recorded. The last VT event in this region had occurred on 25 January 2010, an M 2.8 earthquake located near Ometepe Island.

Explosive activity from Concepción's summit had dropped after 17 March, and by 25 March, gas and ash emissions were no longer reported. Two ash explosions were recorded in April and seismic events were rare. INETER reported quiescence at the volcano through the end of the year except for occasional VT events in July and one M 3.4 earthquake on 6 August 2010. Heavy rain caused signal outages on Ometepe Island in September and resulted in data gaps.

Gas measurements. During the height of Concepción's explosive activity in March 2010, teams of scientists from INETER were deployed with mobile Mini-DOAS to measure SO₂ flux. One team traversed the Ometepe circular road system and measured emissions on 10, 13, and 14 March at the base of the plumes, finding values of 83 to 1,057 tons/day over this time period. A second team collected data on 9, 13, 14, and 15 March and calculated average daily values as high as 507 tons/day (figure 7).

Figure 7. SO2 flux measured from Concepción with Mini-DOAS for four days in March as well as data from 1997, 2002, and 2005. Courtesy of INETER, Dirección de Geofísica.

On 23 March a scientific team from Spain (Instituto Tecnológico de Energía Renovable) joined INETER to they investigate reports of thermal vents previously identified by local residents in the SW part of the island. Near the town of Pull in the Altagracia municipality, diffuse CO₂ emissions were measured from small (sub-meter), rocky crevices that also had low thermal outputs (figure 8).

Figure 8. Field reconnaissance at a previously unexplored fumarole on Concepción's SW flank. Photo by INETER.

Various reports in March from residents on the S and SE side of Concepción described new openings along the upper flanks; these features are described as fumaroles in the reports. Photos and observations were collected by INETER and included reports from several communities and Civil Defense (figure 9). In places, these cavities are on the order of several of meters wide, some appearing in one location where a fresh-water spring broke to the surface in 2005 following summit eruptions. No additional information was available to explain the cause or characteristics of these features.

Figure 9. A sample of one of the various cave-like features that opened during the volcanic crisis of March 2010. The right-hand photo is a close-up of a new feature located just below a recently fractured surface. INETER did not report size estimates of these features. Photos were taken in March but dates were not specified. Photo courtesy of David Chavarría, INETER.

Evacuation drills on 27 January 2010. INETER and the Sistema Nacional para la Prevención, Mitigación y Atención de Desastres (SINAPRED) held evacuation drills on 27 January on Ometepe Island. More than 3,000 residents participated from Moyogalpa and Altagracia, the island's municipalities. Representatives from Civil Defense, Red Cross, and local government officials helped with search-and-rescue training. The event was planned with and supported by Nicaragua's national agencies as well as CARE International and the Swiss Agency for Development and Cooperation. Formal discussions regarding hazard maps, risk assessment, and analysis of precursory activity (seismicity in particular) were held between INETER, SINAPRED, and CARE officials. Evacuation routes and representative maps were discussed with local residents. The drills measured the response capabilities and exercised decision-making on the part of the residents and local emergency management officials.

GPS network. INETER's July 2010 report described the status of a long-term, collaborative program with the Universidad de Cádiz, Spain and the Consejo Superior de Investigación Científica de Madrid (CSIC). This program ("Metodologías de vigilancia desarrolladas en España, en el sistema de vigilancia de Nicaragua") focused on implementing new monitoring systems in Nicaragua with a strong focus on Ometepe Island. After assessments and field visits in February 2010, participants designed CONCEPTEPE, an island-wide GPS network. Installation of the network began in June and continued through July 2010 and included nine permanent stations across the island and one onshore at Rivas, a town just SW of the Pan-American Highway roughly 6 km from the shoreline of Lake Nicaragua (figure 10). Additional fieldwork and equipment testing were required before this system would be fully operational. This project expanded the long-term monitoring efforts on Ometepe Island that have included meteorological stations, a seismic network, and web cameras.

Figure 10. Locations of new GPS stations on Ometepe Island and one location in the town of Rivas (station RIVA) ~6 km W of the Lake Nicaragua shoreline. Courtesy of INETER (using a Google Earth base map); index map courtesy of MapsOf.net.

International conference and Ometepe site visits. A professional meeting of geoscientists was held in Managua on 23-30 November 2010 to discuss ash, lahar, and landslide modeling techniques: "Primera Taller de la Red Iberoamericana para el Monitoreo y Modelizacion de Cenizas y Aerosoles Volcanicos y Uso de TITAN2D para Modelizacion de Lahares y Deslizamientos" (First workshop of the Iberian-Latino-American network for monitoring and modeling volcanic ash and aerosols and the use of TITAN2D for modeling lahars and landslides). Presentations focused on numerical modeling programs TITAN 2D and FALL 3D, programs that investigate mass-flow behavior and forecasting based on geotechnical parameters. Representatives from Spain, Italy, Mexico, Colombia, and Central American countries discussed new techniques for hazards assessments as well as current mitigation efforts applied at different volcanic settings.

From 26-27 November participants from this international workshop visited Ometepe Island. Field activities included sampling of recent lahars as well as mapping in order to improve maps for lahar and landslide hazard mitigation. Participants of the workshop were also invited to speak at community meetings, addressing citizens of Moyogalpa and Altagracia municipalities. The themes of these meetings centered on local risk assessment and new techniques for volcanic hazard forecasting.

References. Gresta, S., Privitera, E., Leotta, A., Gasperini, P., 1996. Analysis of the intermittent volcanic tremor observed at Mount Etna (Sicily), 1987. Ann. Geofis. 39, 421-428.

McNutt, S.R., 1992. Volcanic tremor. In: Encyclopedia of Earth System Science, vol. 4. Academic Press, pp. 417-425.

Geologic Background. Volcán Concepción is one of Nicaragua's highest and most active volcanoes. The symmetrical basaltic-to-dacitic stratovolcano forms the NW half of the dumbbell-shaped island of Ometepe in Lake Nicaragua and is connected to neighboring Madera volcano by a narrow isthmus. A steep-walled summit crater is 250 m deep and has a higher western rim. N-S-trending fractures on the flanks have produced chains of spatter cones, cinder cones, lava domes, and maars located on the NW, NE, SE, and southern sides extending in some cases down to Lake Nicaragua. Concepción was constructed above a basement of lake sediments, and the modern cone grew above a largely buried caldera, a small remnant of which forms a break in slope about halfway up the N flank. Frequent explosive eruptions during the past half century have increased the height of the summit significantly above that shown on current topographic maps and have kept the upper part of the volcano unvegetated.

Information Contacts: Instituto Nicaraguense de Estudios Territoriales (INETER), Volcanology and Geophysics Departments (URL: http://www.ineter.gob.ni/); Washington Volcanic Ash Advisory Center (VAAC) (URL: http://www.ospo.noaa.gov/Products/atmosphere/vaac/); ABC Digital: Paraguay y El Mundo (URL: http://www.abc.com.py/); Noticias.com: Noticias de Guatemala (URL: http://noticias.com.gt/internacionales/); MapsOf.net (URL: http://mapsof.net/).

A submarine eruption at Hierro volcano, Canary Islands, Spain, represents the first documented historical activity, although a flank eruption may have occurred in 1793. A satellite photo shows El Hierro island and the sea surface expression of the submarine eruption on 26 October 2011 (figure 1). For clarification, the name "Hierro" refers to the volcano (as listed in the GVP database), while the name "El Hierro" refers to the island constructed by the volcano; this naming convention will be followed in this report. Unless otherwise noted, all data concerning the pre-eruptive and eruptive activity at Hierro was reported by Instituto Geográfico Nacional (IGN).

Figure 1. Annotated satellite photograph of El Hierro island on 26 October 2011 highlighting the emission area (discolored brown water, circled) and volcanic material transported by ocean currents, appearing light blue-green; settlement names are underlined. (Inset) Geographic location of El Hierro island, in the Canary Islands, off the W coast of Africa. Satellite image courtesy of RapidEye; index map modified from Mapsof.net.

Pre-eruptive activity. Increased seismicity at El Hierro beginning 16 July 2011 marked the onset of pre-eruptive activity. More than 6,000 seismic events had occurred by the beginning of September; seismic events were less than M 3, and hypocenters were located at ~10 km depth beneath the area of the now-collapsed El Golfo volcano (El Golfo Bay, on the N side of the island; figure 1). The increased seismicity was accompanied by 2 cm of ground inflation and increased CO₂ flux over the same time period. Following a significant increase in both seismic energy release rates (figure 2) and ground deformation rates, the Canarian Autonomous Government raised the Alert Level to Yellow on 23 September (on a 3 color scale; Green, Yellow, and Red).

Figure 2. Cumulative energy (units of joules) registered by a seismometer monitoring El Hierro. a) Seismicity during 18 July-27 September 2011 highlighting pre-eruptive activity; yellow line indicates the beginning of Yellow Alert Level on 23 September. Slope increase around 20 September indicates increased seismicity. b) Seismicity during 18 July-18 November congruent with eruptive activity; yellow and red lines indicate the beginning of Yellow alert (23 September) and Red alert (11 October); dashed black line indicates the onset of volcanic tremor. Note the change in scale on the y-axis, from 1010 (a) to 1012 (b). Courtesy of Instituto Geográfico Nacional (IGN).

In the first week of October, seismic hypocenters were located offshore SW of El Hierro island. The next week, an M 4.3 earthquake occurred on 8 October, 1.5 km offshore to the SW, at ~ 14 km depth. This was the largest magnitude precursory seismic event. During 8-9 October, following the 8 October earthquake, ground deformation trends changed, suggesting deflation. Coinciding low magnitude earthquakes occurred at 2 km depth to the SW of the island, and tremor commenced at about 0515 on 10 October, with the highest amplitudes measured at the S-most seismic station. IGN said, "data suggested a submarine eruption."

Red alert due to submarine eruption. At 0700 on 11 October, the amplitude of tremor increased; the same day, the Government of the Canary Islands raised the Alert Level to Red for La Restinga village (figure 1), and residents were evacuated. A maritime exclusion zone was extended to ~4 nautical miles from the coast on the S end of the island.

Within the next week, visual evidence of the eruption was observed. On 12 October, a large area of the ocean to the S of La Restinga village was discolored, and a small, intensely discolored area was identified as the emission area. On 15 October, viewers in a helicopter observed steaming lava fragments floating in the emission area (figures 3 and 4). Further emission episodes occurred as large, turbulent rings of gas or foam reached the sea surface. Contemporaneously, tremor amplitude and deformation decreased, but in the N part of the island, significant inflation-deflation episodes ensued. Seismic activity at the N of the island continued, highlighting a NNW-SSE trend extending ~13 km from the center of the island at 20-25 km depth.

Figure 3. Steaming blocks of vesicular lava floating in the ocean after eruption at Hierro on 15 October. The water is discolored from the eruption. Courtesy of Instituto Geográfico Nacional (IGN).

Figure 4. Sample of erupted material collected floating on the sea on 18 October 2011; coin for scale. According to Gobierno de Canarias, Plan de Protección Civil por Riesgo Volcánico (PEVOLCA) the pyroclasts were predominantly basalt (black) with lesser amounts of trachyte (white). Courtesy of Instituto Geográfico Nacional (IGN).

Further emission episodes occurred during early November, with turbulent water, foam rings, and volcanic material again reaching the sea surface (figure 5). On 5 and 8 November, especially large bubbles rose to the surface, and they ejected sea water and volcanic material a few meters above the surface; video footage of this phenomenon was captured by Radio Televisión Canaria (RTVC) on 8 November and other dates.

Figure 5. Photographs of large gas bubbles and foam reaching the sea surface at Hierro. a) Photograph taken on 8 November 2011, highlighting the proximity of the emission area (bubbles breaching the sea surface in foreground) to the village of La Restinga (background). b) Detail of a breaching gas bubble on 5 November 2011; upper peripheral parts of the image show intensely discolored seawater as compared with relatively uncontaminated seawater seen in the bottom peripheral parts of the image. Both photographs taken from helicopter flights. Courtesy of Instituto Geográfico Nacional (IGN).

Increasing seismicity included an M 4.4 earthquake on 5 November (the eruptive episode's largest as of 8 November). The "Plan de Protección Civil por Riesgo Volcánico" (PEVOLCA) required the evacuation of 51 residents from the settlement Frontera (figure 1) due to landslide risks, and the evacuation of about 200 residents from La Restinga. On 14 November, authorities allowed residents of La Restinga to return to their homes, but children were to attend school in another town, El Pinar. Two buses remained in La Restinga for re-evacuation use, if necessary.

Lava composition, eruption rate, sea-water acidity and gas flux; fish kills. The lava erupted by Hierro was reported by Gobierna de Canarias (analyzed by PEVOLCA) to be predominantly basalt with lesser amounts of trachyte (an approximate basalt-to-trachyte ratio of 10:1; figure 4). They reported that the pyroclasts formed from magma mixing at the time of the eruption. They inferred that the lavas were physical mixtures.

According to Gobierno de Canarias, researchers for the Instituto Español de Oceanografia (IEO) acquired underwater Digital Terrain Maps (DTM; figure 6) during 24-28 October, and estimated that, in that short time, the volcano erupted nearly 5.5 x 10⁶ m³ of material. IEO also measured a decrease in seawater pH from 7.97 to 5.45 within 5 m of the sea surface in the area of the eruption. Furthermore, Gobierno de Canarias reported that Instituto Tecnológico y de Energías Renovables (ITER) estimated the release of CO₂ and H₂S into the atmosphere at up to 54 and 36 tons/day, respectively.

Figure 6. Underwater Digital Terrain Maps (DTM) a) acquired in 1998 and b) 24 October 2011, collectively highlighting morphologic changes in the submarine vent area offshore of El Hierro island. Further DTMs acquired through 28 October 2011 allowed the Instituto Español de Oceanografia (IEO) to estimate the mass eruption rate to be nearly 5.5 million m3 of material during 24-28 October. Courtesy of IEO.

RTVC reported the death of fish that could not escape the eruption. IGN stated that "Preliminary reports of analyses... suggest that the cause of fish kills is related to the ongoing volcanic processes."

Editor's note: As this issue went to press, the Instituto Volcanologico de Canarias (INVOLCAN) announced a new video channel (Youtube, 2011).

Reference: Instituto Volcanologico de Canarias (INVOLCAN), 2011, Submarine eruption at El Hierro, Canary Islands (Spain), YouTube Video Channel (URL: http://www.youtube.com/user/INVOLCAN).

Geologic Background. The triangular island of Hierro is the SW-most and least studied of the Canary Islands. The massive shield volcano is truncated by a large NW-facing escarpment formed as a result of gravitational collapse of El Golfo volcano about 130,000 years ago. The steep-sided scarp towers above a low lava platform bordering 12-km-wide El Golfo Bay, and three other large submarine landslide deposits occur to the SW and SE. Three prominent rifts oriented NW, NE, and S form prominent topographic ridges. The subaerial portion of the volcano consists of flat-lying Quaternary basaltic and trachybasaltic lava flows and tuffs capped by numerous young cinder cones and lava flows. Holocene cones and flows are found both on the outer flanks and in the El Golfo depression. Hierro contains the greatest concentration of young vents in the Canary Islands. Uncertainty surrounds the report of an eruption in 1793. A submarine eruption took place about 2 km SSW off the southern point of the island during 2011-12.

Information Contacts: Instituto Geográfico Nacional (IGN), C/ General Ibáñez de Ibero, 3. 28003, Madrid, España (URL: http://www. ign.es/); RapidEye, RapidEye AG, Molkenmarkt 30, 14776 Brandenburg an der Havel, Germany (URL: http://www.rapideye.de/); Mapsof.net (URL: http://mapsof.net/); Radio Televisión Canaria (URL: http://rtvc.es/); Gobierno de Canarias (URL: http://www.gobiernodecanarias.org/); Instituto Español de Oceanografia (IEO) (URL: http://www.ieo.es/).

This report covers behavior at Kizimen (figure 9) during February-September 2011, an interval where the volcano emitted substantial ash plumes (often blowing towards major air traffic routes, in four cases with plumes 300-475 km long). Viscous block lava flows extended over 2 km from the vent. The progression of this eruption can be divided into three stages: increased seismicity, which began 1.5 years before the eruption (BGVN 35:02); gas-and-steam emissions starting on 11 November 2010, and the eruption, which began on 9 December 2010 (BGVN 36:01). The eruption continued through at least September 2011.

Figure 9. (upper left) Regional location of Kizimen on Kamchatka Peninsula, Russia; red square indicates area of enlarged map. (lower right) Local setting of Kizimen among neighboring volcanoes. Regional map was found on the internet, authorship unknown. Local map was provided by Droznin Valery (Institute of Volcanology and Seismology, Russian Academy of Sciences, Far Eastern Branch).

During February to September 2011, scientists continued to observe seismicity that consisted of a large number of weak, local surface earthquakes (sometimes accompanied by significant seismic noise) and weak volcanic tremor. The Kamchatka Branch of the Geophysical Service of the Russian Academy of Sciences (KB GS RAS) reported a substantial increase in the number of recorded earthquakes during August-September 2011 (figure 10a). KB GS RAS observers also noted a nearly continuous thermal anomaly (figure 10b) coupled with volcanic activity consisting of both pyroclastic flows and a steady stream of gas-and-ash plumes that drifted 20 to 475 km from the volcano (table 1).

Figure 10. For Kizimen, a) the number of earthquakes per day and b) number of thermal anomaly pixels per day during February-September 2011. Data from Kamchatka Branch of the Geophysical Service of the Russian Academy of Sciences (KB GS RAS).

Table 1. Summary of selected significant volcanic ash plumes during February-August 2011. This table records four days with plume lengths of greater than 300 km. One plume, on 2 April, extended 475 km SE. Data from KB GS RAS.

A rose diagram created from the data in table 1 showed that plumes predominantly drifted SE (13 cases, figure 11). The longest plume (475 km on 2 April) also extended to the SE.

Figure 11. A rose diagram created from table 1; each point plotted represents the direction and distance traveled by an individual Kizimen plume. Based on data from KB GS RAS.

Ash dispersal from Kizimen has strong implications for aviation, as the routes of major aircraft lie to the E of the volcano and many of the plumes traveled in directions between NE and SE. Many plumes, most notably the farthest reaching plumes, drifted SE. Eastward components (between SE and NE) make up 25 cases, over half of the 40 total cases shown in table 1.

Several events occurred during April: explosive emissions ejected ash and rock, and effusive lava flows on the upper flanks originated from summit crater vents. On 16 April, lava flows appear to have melted snow, and meltwater drained into Lake Kronotskoe. On 26 July, lava on E slope flowed 1 km from a summit vent.

September 2011 fieldwork. During fieldwork to Kizimen in September 2011, volcanologists observed lava flow and pyroclastic-flow deposits (figure 12). According to Natalia Malik (2011), on 14 September 2011, the volcano erupted constantly, and earthquakes were felt. The lava flow front on the E slope reached 1,300 m elevation, extending ~ 2.3 km from the vent area. The thickness of the flow, based on a visual estimate, was ~ 50 m. The bottom of the flow produced hot avalanches that were incandescent at night.

Figure 12. a) View of Kizimen's N side from a helicopter with a fresh lava flow (dark area at left) descending the E slope. Note the thick steam plume from the summit. b) Fresh lava flow front on the E flank; person at left for scale. c) Pyroclastic-flow deposit in Poperechny Creek, on the NE side of the volcano; for scale, the dog is ~0.5 m tall. Photos taken by Natalia Malik in September 2011.

In the valley of Poperechny Creek on the NE flank of the volcano, observers documented fresh, hot pyroclastic-flow deposits, which locally emitted steam and other gases (figure 12c). Surface water caused erosion of the pyroclastic flow deposit's surface (figure 12c). The thickness of the pyroclastic-flow deposits was estimated to be on the order of 3 m. During emplacement of the pyroclastic flows, trees and vegetation on the valley's lower slopes suffered extensive damage.

Several satellite images also helped to depict Kizimen's recent activity (figure 13). Notice the striking differences between the images from 6 September 2009 and 5 September 2011.

Figure 13. a) Kizimen false-color satellite image acquired on 6 September 2009, showing the pre-eruptive state of the volcano. b) False-color satellite image acquired on 5 September 2011, showing the enormous change over large areas of the volcano, particularly on the E side. A prominent lava flow is present on the E flank. Freshly erupted material, such as tephra and lahars, blocked drainages, and formed a new lake. Freshly erupted material appears brown and vegetation appears red. These images were acquired by the Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER) aboard the Terra satellite. Courtesy of NASA Earth Observatory.

According to NASA Earth Observatory, the new volcanic deposits (appearing brown in figure 13b) have covered much of the vegetation (red) on the slopes of the volcano, especially to the E. Likewise, volcanic material has filled rivers and streams around the volcano. The same photograph shows a modest volcanic plume rising from Kizimen's summit, accompanied by a smaller plume from a fumarole to the NW. These images illustrate the growth of a stratovolcano: lava flows interbedded with layers of volcanic ash, cinders, blocks, and bombs. The lava flow on Kizimen is a viscous block lava (that forms the steep-sided flows seen in figure 12b). As the flow slowly advanced down the E side of the volcano, the surface collapsed, sending boulders, ash, and other material into the valley below.

Reference: Malik, Natalia, 2011, Current activity of Kizimen, September 2011 (in Russian): Institute of Volcanology and Seismology, Russian Academy of Sciences (http://www.kscnet.ru/ivs/volcanoes/inform_messages/2011/Kizimen_092011/Kizimen_092011.html).

Geologic Background. Kizimen is an isolated, conical stratovolcano that is morphologically similar to St. Helens prior to its 1980 eruption. The summit consists of overlapping lava domes, and blocky lava flows descend the flanks of the volcano, which is the westernmost of a volcanic chain north of Kronotsky volcano. The 2334-m-high edifice was formed during four eruptive cycles beginning about 12,000 years ago and lasting 2000-3500 years. The largest eruptions took place about 10,000 and 8300-8400 years ago, and three periods of long-term lava dome growth have occurred. The latest eruptive cycle began about 3000 years ago with a large explosion and was followed by intermittent lava dome growth lasting about 1000 years. An explosive eruption about 1100 years ago produced a lateral blast and created a 1.0 x 0.7 km wide crater breached to the NE, inside which a small lava dome (the fourth at Kizimen) has grown. Prior to 2010, only a single explosive eruption, during 1927-28, had been recorded in historical time.

Information Contacts: Kamchatka Branch of the Geophysical Service of the Russian Academy of Sciences (KB GS RAS), Piip Ave. 9, Petropavlovsk-Kamchatsky, 683006, Russia; Kamchatka Volcanic Eruptions Response Team (KVERT), Institute of Volcanology and Seismology, Russian Academy of Sciences, Far East Division, 9 Piip Blvd., Petropavlovsk-Kamchatsky 683006, Russia (URL: http://www.kscnet.ru/ivs/); Sergey Senukov, Kamchatka Branch of the Geophysical Service, Russian Academy of Sciences (KB GS RAS), (URL: http://www.emsd.ru/); Valery Droznin and Natalia Malik, Institute of Volcanology and Seismology Russian Academy of Sciences, Far Eastern Branch, 9 Piip Blvd., Petropavlovsk-Kamchatsky 683006, Russia; NASA Earth Observatory (URL: http://earthobservatory.nasa.gov/).

This report examines the tectonic setting of Batu Tara, Indonesia, and volcanic activity between February 2010 and October 2011. A map details the tectonics of portions of the Indonesian and Australian plates in the region (Elburg, 2005). Batu Tara lies along some critical air routes that link Asia to Australia. Sonnabend (2007) discussed alternate routes to avoid plumes from Batu Tara at a conference on volcanic ash in 2007. Satellite imagery from the NASA Earth Observing System (EOS) in 201 showed the islands volcanic features and complex plume dispersion.

The Darwin Volcano Ash Advisory Centre (VAAC) produced more than 40 ash plume advisories. The majority of the Darwin VAAC advisories stemmed from plume detection by the Japan Meteorological Agency's MTSAT-1 and two satellites. Lastly, during 17-19 August 2011, Thorsten Boeckel and others witnessed Batu Tara in eruption; they collected photos, videos and recorded the event.

Batu Tara (figure 6) lies 55 km from Timor, the nearest large island. Maumere, the largest town in the region (pop. 70,000; United Nations Department of Humanitarian Affairs, 1992), resides on the N coast of Flores Island, Indonesia, 175 km WSW from Batu Tara. Batu Tara sits 947 km NE of Darwin, Australia, 1,860 km W of Jakarta and 2,410 km SW of the Republic of Singapore.

Figure 6. Batu Tara volcano (red triangle) in the Indonesian Archipelago. Revised from Google and Tele Atlas.

Geologic setting and plate tectonics. Volcanism in Indonesia, as shown in figure 7, is characterized by the northward subduction of the Australian plate beneath the Indonesian plate. According to Elburg (2011), volcanoes in the area to the S of the Weber thrust (consisting of the islands Alor, Atauro, Wetar, and Romang) became extinct 3.5-1.8 million years ago. This tectonic region delineates a complex of thrusting, trough, trench, basin, ridge, crust, plateau and continental plate features forming a constellation of volcanoes. The principal geologic features relevant to Batu Tara are its proximity to the subduction zone and the local distribution of active volcanism. It has erupted potassic leucite-bearing basanitic and tephritic rocks intermittently since 1 July 2006, following a dormancy dating back to 1847-1852. Starting in January 2007, observers issued reports of ash plumes from explosive activity. Darwin VAAC recorded 7 to 10 months of plume descriptions per year during 2008 through October 2011.

Figure 7. Map delineating inferred regional-scale tectonics surrounding Batu Tara. Revised from Elburg (2011).

Darwin VAAC Advisories. The Darwin VAAC advisories for this reporting period began on 8 March 2010 (table 4). From 8 March 2010 through 30 Oct 2011, 41 advisories were released. The reports specified ash plume altitude and dispersal direction. No reports were filed for February, November and December of 2010. After a pause in late October 2010, advisories began again in March 2011and continued through 30 October, the end of the reporting period. The most frequent and highest plumes occurred during approximately the same times of both years.

Table 4. Representative Darwin VAAC Advisories listing Batu Tara ash plumes during 2010-2011. Many plumes drifted N to SW, corresponding to the trade winds.

Batu Tara plume heights ranged from ~ 1 to 3 km altitude, the majority of which were near 2 km in height. Plumes dispersed mostly in westerly directions.

Commercial airline routes. Sonnabend (2007) discussed avoiding ash plumes from Batu Tara on the airline routes between Jakarta and Sidney. He reported "When the pilot smells the sulfur it is too late to escape. Therefore it is essential that, with respect to a safe flight, the information about a volcanic eruption will be passed immediately to the airlines and pilots in flight. Standardized products of describing volcanic ash events in text or graphical form are used by flight crews, dispatchers and also automated systems in order to support the decision making process in view of a safe and economic flight operation."

An example (figure 8) shows the normal route (blue, in the middle) and two alternate ones (black to the E, red to the W).

Figure 8. Alternate flight advisory routes due to Batu Tara plumes (red and black) between Sidney and Jakarta. The central route (blue) is the normal route. Revised from Sonnabend (2007).

Table 5 compares time, fuel, and cost resources of the nominal route with the two alternates. The alternate routes cost 3-5 minutes of additional flight time, 1353-1690 kg of fuel, and up to ~ $60 USD per minute. When confronted with the immediacies of ash advisories, this example typifies the decision-making process by a commercial airline confronted with eruptive plumes where changing the flight path adds costs. This is especially true when there are many flights per day or when other routes overlap the same region. The consequences of even minor route deviations could improve safety but add cost and flight time weighed against the possibility of damage from ash.

Table 5. Comparisons of the normal Jakarta-Sidney air route compared to nearby alternate routes that avoid passing over Batu Tara (see figure 8). From Sonnabend, 2007.

NASA EOS Images. The Moderate Resolution Imaging Spectroradiometer (MODIS) sensor aboard the AQUA satellite acquired an image (figure 9) on 15 March 2010. The plume dispersed S, then immediately split, drifting SE and SW. Other areas to the E and W appear to be residual plumes, but their origin was not mentioned in the EOS report. Notice the bottom of the E plume reversed direction, arcing W. An earlier plume near the crater in the NE sector of the image moved NE along an arc.

Figure 9. Wind driven ash plumes from a Batu Tara eruption on 15 March 2010. Courtesy of Jeff Schmaltz, NASA Earth Observatory.

Another NASA EOS image (figure 10), acquired on 6 August 2010, showed material extending from the E shore. The N-S diameter of the island is ~ 3 km; the E scarp of the crater extends ~ 700 m to the sea. A large-scale view from a different satellite instrument (MODIS) on the same day showed that the plume extended W from Batu Tara before it disappeared under a bank of weather clouds.

Figure 10. A NASA EO-1 ALI sensor image of Batu Tara erupting on 6 August 2010. The scarp on the E side of the island is referred to as the "Sciara del Fuoco" in Thorsten Boeckel's narrative. Revised from NASA Earth Observatory, Robert Simmon.

Summer trade winds. Winds aloft play a significant role in three sections of this report: advisories, air routes, and plume-satellite images (e.g. figure 9). The winds at Batu Tara area are often described as trade winds (figure 11). The trades, the most consistent of the Earth's wind systems, with an average altitude of ~ 0.9-1.5 km, are characterized by direction and, to a lesser degree, speed (Glickman, 2000).

Figure 11. A highly simplified depiction of the Earth's wind system showing the trade winds near the equator in light red. At Batu Tara they would be expected to blow to the W and many of the plume dispersal noted in table 4 have a westerly component. From NOAA National Ocean Service Education.

The trades (figure 11) vary seasonally and have other complexities. They meet at the Intertropical Convergence Zone (ITCZ), which norminally lies near the equator. However, the ITCZ shifts to the N and S of the equatorial median, typically ranging from ~ 1,500 km S in January to ~ 3,300 km N above the Indonesian Archipelago in July (figure 12; Lutgens and Tarbuck, 2001).

Figure 12. Northern shift of the ITCZ in July above Indonesia; Batu Tara in red. From Lutgens and Tarbuck (2001).

In July, just N of the equator, below the displaced ITCZ, the winds move counter to those below the equator, pushing E instead of W. These two sources, the nominal trade wind and the NW wind located S of the shifted July ITCZ near Batu Tara, disrupt the normal trade wind pattern. This system of multiple winds (more complex than the cartoon shown in figure 11), along with the shifts in winds with altitude, and other factors (such as sea surface conditions) play roles in dispersal of Batu Tara ash plumes.

Eye-witness observations. Thorsten Boeckel and others recorded videos and photos, and noted impressions of Batu Tara's eruptions during 17-19 August 2011. Boeckel's group landed on the island in the morning of 17 August and continuously documented during the day and night. More details of their adventure can be found on the internet (see Information Contacts); several of Boeckel's photos appear in figures 13 and 14.

Figure 13. Four photos of Batu Tara taken during 17-19 August 2011. a) The scarp from offshore looking N. b) A daytime photograph of a Strombolian eruption, with top edge of the crater almost out of view (except for a trace of the sky at top center and left). c) Near the summit looking WNW, just left of the crater, with a plume rising on the right. d) An enlargement (~400%) of c) showing incandescent spatter ejected from the vent. Courtesy of Thorsten Boeckel.

Figure 14. Photographs of night-time eruptions of Batu Tara during 17-19 August 2011. a) A view near the summit shows lava funneling down a chute just beyond the margin of the slope (out of view) with a secondary flow facing the viewer. b) Incandescent lava bombs ejected from the summit; lava to the left of the crater is traveling downslope in the scarp. Courtesy of Thorsten Boeckel.

In Boeckel's words, "The local maps fail to locate Batu Tara. In Larantuka in East-Flores, where the adventurers sighted volcanic plumes on Batu Tara they booked passage on a tuna vessel for the 7 hour trip ignoring gossip from local fishermen that the island is enchanted. After about 5 hours we could recognize the Batu Tara Island. From a distance of 15 km we could see ash clouds over the island.

"During the approach we noticed increasingly that this volcano is a true stone block in the sea. Hence, would we be able to land? That evening, we reached the backside [ E side] of the island and saw the 'Sciara del Fuoco'. And really, this volcano must be the twin volcano of Stromboli. Even the summit, the Pizzo and the fire chute turned away from the mainland resemble Stromboli. The crater is approximately two-thirds the height, surrounded by a powerful steep crater funnel.

"The next morning a landing site was chosen. About 100 m beside the Sciara a narrow landing strip appeared. A skillful native fisherman whom we had onboard ferried our equipment onto the strip. [Ascending] the very steep area would take an immense expenditure of time. After landing, the equipment was set up near the summit recording the ongoing Strombolian eruption.

"The active Strombolian activity was most vigorous. At intervals of 15 minutes we noted many smaller eruptions. Larger outbreaks, 300-400 m high also occurred at 30-45 minute intervals. Those on the boat viewed lava ejecting far over crater edge. Often the forest was bombarded ~ 200 meters below the crater.

"The night began, and in addition to the fascinating lava show [figure 14], the eruption noise was a highlight. Even ~ 700 meters away, the ground tremored during stronger outbreaks.... The fire chute appears impressive, large plastic lava constantly flowed from the crater. At night bouncing rocks from the lava-flow entering the water created loud explosions."

The eruptions continued as the ship traveled E that night. A photograph, taken from the ship after a day spent on the island, shows the slope angle of the scarp (figure 15). The shot was taken too far away to show lava bombs hitting and skipping along the water's surface, however, such behavior was observed.

Figure 15. A long exposure, evening, shipboard photograph of lava blocks rolling down Batu Tara's scarp. Courtesy of Thorsten Boeckel.

References. Boeckel T., Rietze, M., Szeglat M., and Weber, C., 2011, Indonesia 2011: Batu Tara, URL: http://www.tboeckel.de/EFSF/efsf_wv/indonesia_11/Batu Tara/Batu Tara 2011_e.hth; Posted 03 August 2011; accessed 23 November 2011.

Elburg, M., 2005, Indonesian Magmatism (URL: http://users.ugent.be/~melburg/Indonesia/IndonesiaElburg.html) Updated 10 August 2005; accessed 23 November 2011.

Glickman, T.S., 2000, Glossary of Meteorology, American Meteorology Society, 2nd ed., 850 p.

Lutgens, F.K. and Tarbuck, E.J., 2001, The Atmosphere, An Introduction to the Atmosphere, Prentice Hall, 8th Ed., 484 pp., Figure 7.9.

Sonnabend, H.R., 2007, Airlines, Aircrafts and Volcanic Ash, World Meterological Association (WMO) Fourth International Workshop on Volcanic Ash, Rotorua, New Zealand, 26-30 March 2007, report number VAWS/4 WP/07-04.

United Nations, Department of Humanitarian Affairs, 1992, Indonesia-Earthquake, DHA-UNDRO Information Report No. 2, 13 December, 1992; DHA-UNDRO 92/0817.

Geologic Background. The small isolated island of Batu Tara in the Flores Sea ~50 km N of Lembata (fomerly Lomblen) Island and the main volcanic arc. A scarp on the eastern side reaches the sea, and vegetation covers the other flanks to within 50 m of the summit. This volcano is noted for its potassic leucite-bearing basanitic and tephritic rocks. The first recorded eruption, during 1847-52, produced explosions and a lava flow.

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/); NASA Earth Observatory, NASA Goddard Space Flight Center (URL: http://earthobservatory.nasa.gov/); Thorsten Boeckel (URL: http://www.tboeckel.de).