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 (CSLP 19-69) discussed a summit eruption at Ebulobo stratovolcano, near the S coast of Central Flores island, that in 1969 had emitted ash and steam as well as "fire" (generally taken as incandescence but also possibly flames). CVGHM (Center for Volcanology and Mitigation of Geologic Disasters), issued a report on Ebulobo on 26 August 2013 informing readers that during August 2013, observers noted one or more hot emissions escaping from the crater. The resulting plume was of sparse consistency, white in color, under weak pressure, and it rose to 5-30 m above the peak. "Smoke" was noted.

The CVGHM report noted that on the night of 21 August 2013, observers on the volcano's N side saw incandescence at the summit area. Observations during the night of 22-23 August revealed points of glowing remained unchanged. The glowing was considered anomalous, having not been seen since 2011. The exact cause of the incandescent regions was not reported No new fissures, lava flows or pyroclastic flows were reported. The glowing later terminated as discussed in an October follow up report.

During June 2013, the system recorded the earthquakes shown in table 1.

Table 1. A summary of seismicity recorded at Ebulobo. Dashes signify cases without reported data. Extracted from the 26 August and 17 October CVGHM reports.

During 1-22 August 2013, the seismic system also recorded tremor with maximum amplitudes in the range of 0.5-15 mm.

Ebulobo (figure 1) has a dedicated observation post and two seismic instruments as discussed further below.

Figure 1. Ebulobo as seen in a photo taken 9 June 2009. Copyrighted photo by Andrzej-Muda.

Glow diminishes and Alert Level drops (to I). During September-October white plumes rose as high as 100 m above the crater. Despite that, the glowing area had remained absent after 27 August. On 17 October CVGHM scaled back the Alert from II to I (Normal, on a scale that reaches IV).

More background. The following was extracted from CVGHM reporting.

"Ebulobo Volcano is located in the district of Nagekeo, province of Nusa Tenggara Timur. Eruptions of Ebulobo generally have consisted of lava streams that quickly formed mounds but have never so far resulted in sudden eruptive outbursts that produced a symmetrically shaped mass to the volcano. Ebulobo's eruptions have occurred between 3 and 58 years. In its historical record, its latest eruptive activity took place in 1941 and consisted of a lava stream.

"Observation of Ebulobo's activity is carried out from its monitoring post in the village of Ekowolo, sub-district of Boa Wae and is done visually and according to tremor events. The monitoring is done by means of a Type VR-60 seismograph and a Type L4C seismometer. The readings are transmitted by a telemetric system."

Geologic Background. Ebulobo, also referred to as Amburombu or Keo Peak, is a steep-sided symmetrical stratovolcano in central Flores Island. The Watu Keli lava flow traveled down the N flank to 4 km from the summit in 1830, the first of only four recorded historical eruptions of the volcano.

Information Contacts: Center for Volcanology and Mitigation of Geologic Disasters (CVGHM), Jalan Diponegoro 57, Bandung 40122, Indonesia (URL: http://www.vsi.esdm.go.id/); and theNational Agency for Disaster Management (BNPB), Gedung Graha 55 Jl. Tanah Abang II No. 57 Postal Code: 10120, Jakarta Pusat, Indonesia (URL: http://www.bnpb.go.id/).

In the first nine months of 2011, Ibu was the scene of frequent avalanches and at least one weak explosion that generated minor white-to-gray plumes (BGVN 36:08). Seismic activity decreased during September 2011, prompting the Center of Volcanology and Geological Hazard Mitigation (CVGHM) to lower the Alert Level to 2 (on a scale of 1-4) on 8 September (the Level rose again later). This report discusses activity from 9 September 2011 through March 2014. The location of Ibu is shown in BGVN 36:08.

According to CVGHM, seismicity increased and volcanic tremor was detected during May through 6 June 2013. The lava dome grew, especially the N part, and by early June had grown taller than the N crater rim. White-to-gray plumes rose 200-450 m above the crater rim. Based on visual and instrumental observations, as well as the hazard potential, CVGHM increased the Alert Level to 3 on 7 June. The public was warned to stay at least 3 km away from the active crater.

CVGHM reported that during 7 June-9 December 2013, the lava dome continued to grow, and incandescent material from the dome filled the river valley in the direction of Duono village, about 5 km NW. The seismicity remained relatively stable. Observers saw occasional weak white-to-gray plumes. On 10 December 2013, the Alert Level was lowered to 2; however, the public was warned to stay at least 2 km away from the active crater, and 3.5 km away from the N part.

Between 1 September 2011 and March 2014, MODVOLC thermal alerts were issued on 70 days, or an average of almost one day every two weeks. Such alerts are consistent with dome growth such as that noted above. (Those alerts are derived from satellite data collected by the MODIS instrument and processed by the Hawai'i Institute of Geophysics and Planetology.) For comparison, between 1 January 2011 and 13 September 2011, these alerts only appeared about once every 2.4 weeks on average.

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

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

A new island emerged on 20 November 2013 out of the ocean as the result of a Surtseyan eruption on the S flank of Nishinoshima, a small volcanic island in the Izu-Bonin arc, ~940 km S of Tokyo (figure 1). The new island, originally called Niijima ('new island') by the Japan Coast Guard (JCG), eventually merged with Nishinoshima on 24 December 2013. We continue to describe the now merged islands under the name 'Nishinoshima.'

Figure 1. Location of Nishinoshima island shown on an annotated topographic map of the Izu-Bonin arc; the insert shows the area of the main map and the larger regional geography. The map highlights the location of Nishinoshima (Nsi). Other features located respectively from N to S are: Os–Oh–shima; Nij–Nii–jima; Myk–Miyake–jima; Mkr–Mikura–jima; Krs–Kurose hole; Hcj–Hachijo–jima; Shc–outh Hachijo caldera; Ags–Aoga–shima; Myn–Myojin knoll; Sms–South Sumisu; Ssc–South Sumisu caldera; Tsm–Torishima; Sfg–Sofugan; G–Getsuyo seamount; Ka–Kayo seamount; S–Suiyo seamount; Kn–Kinyo seamount; D–Doyo seamount; Nsi–Nishinoshima; Kkt–Kaikata seamount; Ktk–Kaitoku seamount; and Kij–Kita Iou-jima. After Kodaira and others (2007).

Niijima emerges. Niijima emerged by 20 November 2013 from the ocean surface at an area ~0.5 km SSE off the coast of Nishinoshima. The latter is a small (700 m²), uninhabited volcanic island that last erupted and expanded in during 1973-74. Additional background information is included at the end of this report.

Based on satellite images, the Tokyo Volcanic Ash Advisory Center (VAAC) reported that at 0717 UTC on 20 November 2013 a plume rose 600 m over a new island which emerged ~500 m S of Nishinoshima (figure 2). At 0630 UTC on 22 November, a plume rose 900 m. MODVOLC satellite thermal alerts were measured almost daily from 1635 UTC on 23 November and continued through the latest alert noted at 0120 UTC on 7 April 2014.

Figure 2. Niijima produces a plume as it emerges from the ocean to form a new island off the coast of Nishinoshima on 20 November 2013. Courtesy of Kurtenbach (2013); image from the JCG.

On 21 November JCG and the Japan Meteorological Agency (JMA) noted that the island formed was by then ~200 m in diameter. A warning of dense black emissions from the eruption was issued by JCG on 20 November, and television footage (Frisk, 2013) showed on 21 November ash and rocks exploding from the crater as steam billowed out of the crater (figure 3). On 24 November, JCG reported lava flows coming from the newly-formed crater. They extended to the coastline of the island, and bombs continued to be ejected.

Figure 3. A photograph of Niijima from 21 November 2013 shortly after it emerged from the ocean.  Note the large airborne rock erupting from the crater. Courtesy of Kurtenbach (2013); picture provided by JCG.

The Advanced Land Imager (ALI) on NASA's Earth Observing-1 (EO-1) satellite captured a natural-color image on 8 December 2013 (figure 4). JMA reported that by early December the area of the new island had grown to 56,000 m², about three times its initial size, and was 20 to 25 m above sea level.

Figure 4. NASA Earth Observatory satellite image acquired on 8 December 2013 from the EO-1 ALI sensor. The discolored water around the island was attributed to material included volcanic minerals, gases, and seafloor sediment stirred up by the ongoing volcanic eruption. The faint white puffs above the center and SW portion of the island are likely steam and other volcanic gases associated with the eruption. Courtesy of NASA Earth Observatory.

Niijima merges with Nishinoshima. NASA's EO-1 ALI satellite again captured a natural-color image of Nishinoshima and Niijima islands on 24 December 2013 and shows only a narrow channel of water appearing to separate the two (figure 5). The water around the islands continued to be discolored by volcanic minerals and gases, as well as by seafloor sediment stirred up by the ongoing eruption. A faint plume, likely steam and other volcanic gases associated with the eruption, drifted SE. Infrared imagery from the same satellite on the same date showed intense heat from the fresh lava, which continued to build the new island. A strip of isolated, discolored (orange) seawater appeared at the junction of the two islands (figure 6).

Figure 5. NASA Earth Observatory satellite image acquired 24 December 2013. Courtesy of NASA Earth Observatory; satellite image by Jesse Allen using EO-1 ALI data from the NASA EO-1 team.

Figure 6. An aerial photograph just prior to the merger of the two islands, taken on 24 December 2013, with Niijima on the right and Nishinoshima on the left. Seawater trapped at the junction has been discolored to orange, attributed to the presence of particulate matter and biochemical activity of organisms in the water. Courtesy of the JCG.

Figure 7 is a drawing by the Japanese Coast Guard (JCG) showing the location of the coastline and the growth of the new island (Niijima) from 20 November 2013 to 26 December 2013. It is striking how much of the island expanded during 13-24 December 2013.

Figure 7. Scale drawing of the merged islands showing the changing coastlines as the new island grew. Colored enclosing lines during the current eruption of Nishinoshima as shown for the following dates: 20, 21, 22, 26, and 30 November 2013, and 1, 4, 7, 13, 24, and 26 December 2013 (note legend translated from Japanese for dates and color of mapped shorelines). Image and interpretation courtesy of JCG.

According to JCG's aerial observation on 20 January 2014, the new part of Nishinoshima island had an area of 0.3 km² (750 m E to W, and 600 m N to S) (figure 8).

Figure 8. An aerial photograph, looking W, of Nishinoshima island taken on 20 January 2014. The newly merged island, Niijima, on the left, continued to expand NW. White and brown plumes rose from vents on the new land, and the water around the SW portion was discolored. Photo courtesy of JCG.

New images from an overflight on 3 February (figure 9) confirmed that the activity on the former new island continued steadily. Over the past weeks, the vent fed several active lava flow fronts that enlarged the land in more or less all directions. In particular, there are two active flows relatively close to the vent which had been traveling E and formed a small, almost closed bay with green-orange discolored water inside. The previous shorelines for 20 January 2014 (yellow enclosing line) and 21 November 2013 (white enclosing line) are superimposed over the image to show the growth of the island.

Figure 9. Aerial photography of the island on 3 February 2014. For comparison, the previous shorelines on 20 January 2014 (yellow enclosing line) and 21 November 2013 (white enclosing line). Photo courtesy of JCG.

According to Pfeiffer (2014), the island continued growing with lava flows traveling in several directions (figure 10). Its highest peak, formed by the most western of the two active vents, was measured at 66 m. The new addition has more than doubled the size of the island by 16 February. A black-sand beach formed on the NE shore of the old part of the island, as a result of lava fragments washed up by currents and waves.

Figure 10. Direction of lava flow from the western side of two active vents is show by vectors superimposed on the image of the island. North is to the top of the photo. The flow arrows were drawn by JCG over an aerial photograph of the island taken 16 February 2014. Photo courtesy of JCG.

In summary, the new addition to Nishinoshima grew ~500 m SSE of the island's S flank, beginning ~20 November 2013, from a depth of ~50 m to a height of ~65 m from an originating time no earlier than 1974, the time of the latest addition to the island. Based on continued emissions and satellite-based thermal alerts, it is apparent as of 13 March 2014 that Niijima was still expanding outward in all directions from the vents, and that Nishinoshima had grown to over three times its original size.

Further background. The new island was located in the Volcano Islands, a group of three Japanese active volcanic islands that lie atop the Izo-Bonin-Mariana arc system (Stern and Bloomer, 1992) that stretches S of Japan and N of the Marianas (figure 1).

According to the Geological Survey of Japan, Nishinoshima was an emerged submarine volcano in 1974 with a height of ~3,000 m from the surrounding ocean floor and ~30 km wide at its base.

For further details on earlier Nishinoshima activity refer to our earlier reports in predecessor publications, CSLP 93-73 (eight cards issued during 1973-1974), SEAN 04:07, and BVE 25. The latter (BVE 25) is a 1985 Smithsonian report called the Bulletin of Volcanic Eruptions noting that aerial observations on 2 December 1985 disclosed pale green water SW from the island.

The Geological Survey of Japan reported that Nishinoshima is of andesite to basaltic-andesite composition; Aoki and others (1983) classified the volcano's rocks as high-alkali tholeiite. Nishinoshima is surrounded on all sides by cones, vents, pillars, and parasitic seamounts, and its local bathymetry from surveys in 1911 and 1992 are shown in figure 11.

Figure 11. Comparison of bathymetric maps (depths in meters) around Nishinoshima before and after 1973 eruption. The emerged island is shown in green. Depths of 0-100 m are in white, 100-400 m in light blue, 400-700 m in medium blue, and 700-1,000 m in darker blue. The map on the right shows a survey conducted in 1992, after the eruption, based on 1:50,000 basic map of "Nishino-shima" by the Japan Coast Guard (1993). The map on the left shows a survey conducted prior to the eruption, based on mapping in 1911 (Ossaka, 1973). The new island of Niijima first appeared above the sea surface ~500 m SSE of the S coast of Nishinoshima island shown in the 1992 map. Courtesy of the Geological Survey of Japan (2013).

From the 1992 bathymetric map seen at right on figure 11, it is apparent that the ocean depth from which Niijima erupted in 2013, was ~50 m. A sketch of the setting showing a cross sectional view (roughly NNW-SSE) appears in figure 12.

Figure 12. A sketch depicting an approximately NNW (to the left) to SSE (to the right) cross-section across Nishinoshima (blue indicates sea water) portraying some historical stages of growth. The label "Current Nishinoshima" refers to the pre-existing island prior to and in the early stages of the 2013 eruption. Other labels indicate (a) "Nishinoshima before 1973" (also see 1911 bathymetric map in figure 11), (b) flanking material added to Nishinoshima as it "Emerged during the 1973-74 eruption" (also see 1992 bathymetric map in figure 11), and (c) Niijima "Emerging during ongoing eruption" (red area emerging from the sea early in the 2013 eruption). Original drawing courtesy of The Asahi Shimbun (2013).

References. Aoki, H., and Tokai University Research Group for Marine Volcano, 1983, Petrochemistry of the Nishinoshima Islands, La mer, v. 22, pp. 248-256.

Earth of Fire: Actualité volcanique, Article de fond sur étude de volcan, tectonique, récits et photos de voyage [Volcano News, Feature Article on study of volcanos, tectonics, travel stories and photos], 2013, Evolution of Nishino-shima's eruption, Earth-of-Fire web site (URL: http://www.earth-of-fire.com/page-8837676.html).

Frisk, A., 2013 (21 November), WATCH: Incredible video, photos show new island forming off Japan after volcanic eruption, Global News (URL: http://globalnews.ca/news/981245/watch-incredible-video-photos-show-new-island-forming-off-japan-after-volcanic-eruption/ ).

Geological Survey of Japan, 2013, Nishinoshima (URL: https://gbank.gsj.jp/volcano/Quat_Vol/volcano_data/G22.html).

Japan Coast Guard, 1993, 1:50,000 basic map of "Nishino-shima."

Kodaira, S., Sato, T., Takahashi, N., Miura, S., Tamura, Y., Tatsumi, Y., and Kaneda, Y., 2007, New seismological constraints on growth of continental crust in the Izu-Bonin intra-oceanic arc, Geology, v. 35, no. 11, pp. 1031-1034 (doi: 10.1130/G23901A.1).

Kurtenbach, E., 2013 (21 November), Volcano raises new island far south of Japan, AP (Associated Press) (URL: http://news.yahoo.com/volcano-raises-island-far-south-japan-054228644.html).

Ossaka, J., 1973, On the submarine eruption of Nishinoshima, Bulletin of the Volcanological Society of Japan, v. 18, no. 2, p. 97-98, 173-174.

Pfeiffer, T., 2014 (21 February), Nishinoshima volcano (Izu Islands, Japan): island has doubled in elevation, Volcano Discovery web site (URL: http://www.volcanodiscovery.com/nishino-shima/news/42781/Nishino-Shima-volcano-Izu-Islands-Japan-island-has-doubled-in-elevation.html).

Shun, N., 2014, Kaitei chikei (bottom topography), Nishinoshima Kazan (in Japanese), Geological Survey of Japan web site (URL: https://gbank.gsj.jp/volcano/Act_Vol/nishinoshima/page3.html).

The Asahi Shimbun, 2013 (22 November), Japan counts on survival of new island to expand territorial waters (URL: https://ajw.asahi.com/article/behind_news/social_affairs/AJ201311220084).

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 Coast Guard (JCG) (URL: http://www.kaiho.mlit.go.jp/); MODVOLC, Hawai'i Institute of Geophysics and Planetology (HIGP), MODVOLC Thermal Alerts System, School of Ocean and Earth Science and Technology (SOEST), Univ. of Hawai'i, 2525 Correa Road, Honolulu, HI 96822, USA (URL: http://modis.higp.hawaii.edu/); NASA Earth Observatory (URL: http://earthobservatory.nasa.gov); ANN (All Nippon News Network) (URL: https://www.youtube.com/user/ANNnewsCH); VolcanoCafe web site (URL: http://volcanocafe.wordpress.com); Earth of Fire web site (URL: http://www.earth-of-fire.com/); Demis web site (URL: http://www.demis.nl/home/pages/Gallery/examples.htm.).

The last Bulletin report (BGVN 35:11) detailed an explosive eruption that began with gas-and-ash explosions in September 2010 and ended in mid-October 2010. Renewed activity began in February 2011 and continued through June 2011. In this report, we highlight the significant ash events from early-to-mid 2011 as well as the continuous monitoring efforts of Servicio Nacional de Geología y Minería (SERNAGEOMIN) during 2011-2013.

During 17 February-27 June 2011, unrest was detected from Planchón-Peteroa and significant meteorological information (SIGMET) notices were distributed by the Buenos Aires Volcanic Ash Advisory Center (VAAC) (table 3). Ash plumes were reported once or twice a month during this time period, although satellite images were not able to detect many of the events. Ash and gas plumes became continuous during late April, and ash plumes rose as high as 5.8 km altitude on 26 April. On 29 April, SERNAGEOMIN raised the Alert Level to 3 (Yellow).

Table 3. Emissions from Planchón-Peteroa during 18 February-27 June 2011. The Observatorio Volcanológico de los Andes del Sur (OVDAS) maintained a web-camera that contributed to numerous direct observations of emissions and is frequently listed as a source. Courtesy of Buenos Aires VAAC.

Seismicity in April 2011 was dominated by volcano-tectonic (VT) events; 405 were detected, and locations were primarily concentrated in an area 25 km NE of the volcanic complex as well as along the N flank, ~6 km from the crater. Earthquakes were M_C less than 2. Some tremor (RD of 3 cm²) and 30 long-period (LP) (RD 4 cm²) events were also detected that month. SERNAGEOMIN frequently reported seismic data in terms of RD, which is the value calculated from reduced displacements.

SERNAGEOMIN reported that ash emissions on 17, 18, and 29 April correlated with episodes of tremor with RD oscillating between 1 and 3 cm². Overflights conducted on 26, 27, and 29 April determined that the active crater had not changed geometry and also appeared structurally stable (figure 7). The observers noted that tephra deposits from the previous explosions were notable SE and SW of the volcano. Deposits from the 29 April explosion were particularly easy to define during the overflight.

Figure 7. This photo of Planchón-Peteroa was taken during one of a series of overflights during 26, 27, and 29 April 2011. A column of ash rose from the active crater and tephra had visibly covered much of the snow immediately SE and SW of the crater. Courtesy of Orlando Rivera, Exploraciones Mineras Andinas S.A.

Buenos Aires VAAC reported a significant ash plume detected by satellite images on 2 May 2011. The plume drifted between 4.9 and 5.5 km altitude toward the NE at ~7.7 m/s. The OVDAS web-camera also captured images of the plume appearing diffuse and ~3.7 km wide. The VAAC noted that the plume rapidly dissipated during 1315-1845 local time. The following day, continuous emissions of ash, steam, and gas were reported by SIGMET and the VAAC, although satellite images were not able to detect any emissions. By 1000, the VAAC reported SIGMET data for a plume that rose to 4.6-5.5 km altitude, moving E. At 1500, satellite images captured a diffuse and ~15 km wide ash plume. The plume drifted E at 5 m/s and had risen to 5.5 km altitude.

Elevated activity during 4-5 May produced ashfall that reached the towns of Minera Río Teno (about 70 km NW) and Las Leñas (in Argentina, 45 km ENE). An overflight conducted by SERNAGEOMIN confirmed continued ash emissions and explosions that occurred approximately every 30 seconds. The explosive activity rarely produced plumes higher than 1,000 m above the crater. Gray ash deposits were visible downwind of the crater; the wind tended to disperse tephra widely and the observers noted that wind directions were frequently directed to the E, NE, NNE, NNE, and NW. During 30 April-8 May, SERNAGEOMIN noted that seismicity included tremor (RD of 2-3 cm²) and VT earthquakes (M_L less than 1.8).

Geologists from SERNAGEOMIN conducted an overflight of Planchón-Peteroa on 13 June 2011. RedMaule interviewed the observers who were on the helicopter which included representatives of SERNAGEOMIN and Oficina Nacional de Emergencia del Ministerio del Interior y Seguridad Pública (OMENI) as well as the mayor of Maule, Chile. The observers noted that persistent degassing continued; a low-level white plume (less than 400 m high), associated with fumarolic activity, was visible rising from the active crater (figure 8). SERNAGEOMIN concluded from the overflight that Alert Level 3 (Yellow) could be reduced to Alert Level 2 (Green/Normal); Alert Level 3 had been in effect since 29 April 2011.

Figure 8. During an overflight of Planchón-Peteroa on 13 June 2011, few bare rocks were visible around the active crater due to snow-cover and ice; a low-level plume of white vapor rose from the crater. These six photos are stillshots taken from a video interview camera; note that the look direction varies in each photo with the approximate direction noted in the upper left corner of each photo. The tall peak of Planchón is visible in the background of the photo looking N. Courtesy of SERNAGEOMIN and RedMaule.

The Buenos Aires VAAC released an ash advisory on 29 October 2011. Satellite images could not detect ash, but a SIGMET was available.

Activity during 2012. An approximate average of 400 earthquakes per month was detected in 2012, and roughly 75% of the events were VT while 25% were cataloged as LP events. The VT events were rarely larger than M_L 3.0 and depths were in range of 4-10 km; these earthquakes were frequently clustered in groups that correlated with local faults. LP earthquakes were typically M_D ≤ 2.0 and RD ≤ 2.9 cm². SERNAGEOMIN reported tremor in April, May, November, and December (table 4). One notable seismic swarm occurred on 5 April. Approximately 123 VT earthquakes were detected during 0230-0730; these events were located ~20 km NE of the crater with depths less than 10 km. The largest earthquake was M_L 1.7.

Table 4. Tremor was detected during four months in 2012. RD is the value calculated from the reduced displacements of seismicity. Courtesy of SERNAGEOMIN.

On 30 October 2012, the Oficina Nacional de Emergencia del Ministerio del Interior y Seguridad Pública (OMENI) released a report highlighting several communities that would be included in the early warning system designed to report flood risks. The towns included Curicó, Romeral, and Teno, in the region Maule, which are especially vulnerable due to proximity to Planchón-Peteroa's major drainages (figure 9).

Figure 9. This Google Earth image includes the location of Planchón-Peteroa (lower right-hand corner), major towns, and primary roads. The background image is a composite of Landsat images from 2014. Note that the yellow line crossing through the volcanic center is the international border for Chile and Argentina. The scale is approximate. Courtesy of Google Earth.

On 6 November 2012, the network of web-cameras captured images of a white plume rising from the crater. At 1620, the persistent plume rose to ~1.3 km and drifted NE. SERNAGEOMIN noted that this activity was related to fumarolic emissions.

Activity during 2013. During 2013, an approximate average of 200 earthquakes was detected per month. Of these events, ~80% were VT and ~20% were LP. Magnitudes and depths of the VT earthquakes were comparable to the previous year, although ML values were sparsely reported. LP seismicity was reported in M_L, instead of M_D and values were in range of 0.3 to 2.0. The reduced displacements (RD) of LP events were frequently reported on a monthly basis with values in range 0.3-8.4.

Tremor was rarely detected in 2013. SERNAGEOMIN reported six episodes of tremor, but these only occurred in January and the calculated RD was 0.5 cm².

Geologic Background. Planchón-Peteroa is an elongated complex volcano along the Chile-Argentina border with several overlapping calderas. Activity began in the Pleistocene with construction of the basaltic andesite to dacitic Volcán Azufre, followed by formation of the basaltic and basaltic andesite Volcán Planchón, 6 km N. About 11,500 years ago much of Azufre and part of Planchón collapsed, forming the massive Río Teno debris avalanche, which traveled 95 km to reach Chile's Central Valley. Subsequently, Volcán Planchón II was formed. The youngest volcano, andesitic and basaltic andesite Volcán Peteroa, consists of scattered vents between Azufre and Planchón, and and contains a small steaming crater lake. Reported eruptions from the complex have been dominantly explosive, although lava flows were emplaced in 1837 and 1937.

Information Contacts: Observatorio Volcanológico de los Andes del Sur-Servicio Nacional de Geologia y Mineria (OVDAS-SERNAGEOMIN), Avda Sta María No. 0104, Santiago, Chile (URL: http://www.sernageomin.cl/); Buenos Aires Volcanic Ash Advisory Center (VAAC) (URL: http://www.smn.gov.ar/vaac/buenosaires/productos.php); and Oficina Nacional de Emergencia del Ministerio del Interior y Seguridad Pública (OMENI) (URL: http://www.onemi.cl/index.html).

A partial dome collapse took place at Soufrière Hills on 11 February 2010 (BGVN 35:03), an event followed by a lack of easily measured dome growth during an interval that continued into at least April 2014. Despite a lack of significant extrusion into the dome, pyroclastic flows continued, as did rockfalls and volcano-tectonic (VT) earthquakes. MVO describes intervals of this nature as extrusive pauses or more simply pauses. Pauses have been diagnosed as a prevalent behavior since they began following an extrusive phase starting in mid-1995. Our last issue (BGVN 36:08) covered part of the still-ongoing pause.

The various phases of activity at Soufrière Hills Volcano (SHV) during 1 January 1992 to 30 April 2013 are summarized in table 72. The table comes from a Montserrat Volcano Observatory (MVO) report providing a synthesis of activity during ~6 months ending in April 2013, and making authoritative and instructive comparisons to the overall eruption (table 72).

Table 72. Inventory of behavioral phases observed at SHV between 1 January 1992 and 30 April 2013. Pause 5 continued into at least April 2014. Taken from the MVO Scientific Report for Volcanic Activity between 13 October 2012 and 30 April 2013.

In brief, table 72 documents that an increase in seismicity occurred from 1992 to 1995, followed by a phreatic eruptive phase starting in mid-1995. That episode was followed by intervals of extrusion, transition, and pause. Extrusive phases included dome growth and frequent pyroclastic flows. During transition phases, dome growth slowed, but the risk to areas near the volcano continued.

As noted above, pauses are characterized by much slower dome growth (if at all), yet residual activity. The current pause is the longest yet recorded since the eruption began in 1995. Pause 5 began on 12 February 2010, and as of March 2014 was over 50 months long.

MVO established three criteria that indicate the potential for future activity. These criteria include low frequency seismic swarms and tremors, daily SO₂ fluxes above 50 tons/day, and significant ground deformation. Most of the data reported in this Bulletin came from MVO Scientific Reports from 1 November 2011 to 30 April 2012, 1 May 2012 to 12 October 2012, and 13 October 2012 to 30 April 2013.

Short, intense swarms of VT earthquakes have occurred at Soufrière Hills since late 2007. The smaller swarms are often described by MVO as strings.

The most notable activity since September 2011 included intense Volcanic Tectonic (VT) earthquake swarms during 22-23 March 2012. Two small strings of VT events occurred in early August 2012, a brief VT string occurred on 24 December 2012, and a few VT strings of earthquakes took place during 4-6 February 2013.

The seismic events of 22-23 March 2012 and August 2012 were followed by ash venting. The venting in March resulted in the formation of two new craters. One developed inside the 11 February 2010 dome collapse scar; the other was outside the collapse scar to the (figure 91).

Figure 91. The craters at Soufrière Hills that formed following the intense VT earthquake swarms during 22-23 March 2012 are labeled in the above aerial photographs, taken by the Montserrat Volcano Observatory (MVO). The upper photo looks S into the 11 February 2010 collapse scar, and the lower photo looks E from above Gage's Mountain. Courtesy of MVO.

On 20 November 2012, images of the S flank of the dome revealed a pervasively fractured area below the S rim of the explosion crater. That area was considered a potential source for large rockfalls or pyroclastic flows.

During the increased fumarole activity on 4-5 February 2013, a new crater was excavated around a gas vent on the floor of the 11 February 2010 collapse scar. This crater was 15 to 20 m across and 5 to 10 m deep.

The Hazard Level remained at 2, indicating daytime (0800 to 1600) access to Zone C and daytime-transit-only in maritime zone W (located W of the volcano; boats may sail through the zone but must not stop). A map of the zones on the island appeared in BGVN (22:05) and is found as figure 22 above.

Activity during 1 November 2011 to 30 April 2012. Throughout the entire reporting period, seismicity remained comparable to previous pauses in lava extrusion. Four strings of VT events, in this case referred to as "spasmodic bursts," occurred in the course of the interval 1 November 2011 to 30 April 2012. In early December 2011, 10 events were recorded in a 3 minute span; the largest in terms of local magnitude (M_L, discussed further below) was 3.2. The 10 events were interpreted as a sequence of triggered events.

Two intense VT swarms occurred on 23 March 2012, with almost 50 VT earthquakes in each swarm. The largest VT earthquake ever recorded at Soufrière Hills, with M_L of 3.9, was recorded during these swarms. The second more intense swarm was followed by mild ash venting, seven hybrid earthquakes, and three long-period (LP) earthquakes. Topics such as ML are discussed in a subsection below on seismicity.

On 30 March 2012, MVO detected unusually low-level VT seismicity sustained over several hours. This was atypical activity, as seismicity at Soufrière Hills is normally characterized by the occasional appearance of short bursts of VT strings.

November-December 2012. Seven lahars were seismically detected in the Belham Valley region during 1 November 2011 to 30 April 2012. Five took place during November-December 2011. They were associated with rainfall above 10 mm/hr.

A pyroclastic flow occurred in Gages Valley on 9 March 2012. The flow originated close to the summit of Chance's Peak and traveled 1.5 km down the W flank into Spring Ghaut. Although direct volume measurements couldn't be made, an empirical relationship between runout and flow volume suggested the pyroclastic flow deposit volume to be 104 m³.

A slight increase in rockfall activity occurred before the VT swarms of 23 March 2012. There were minor rockfalls on the steep N, E, SW and W sectors of the dome, averaging to less than one rockfall per day. The SW side of the dome above Gingoe's Ghaut was unstable with noticeable rockfall activity.

SO₂ flux averaged 420 tons/day, a value below the multi-year eruption's average. Following the March VT swarms, a daily flux of 4,600 tons was observed, the third highest recorded by the optical spectrometer (DOAS) since its installation in 2002. After 2010, SO₂ cycle fluctuations were dominated by variation with timescales on the order of weeks to months.

On 17 February 2012, a fumarole at the E base of the 2006-2007 dome was observed for the first time by MVO staff. An area with yellow and white sulfur deposits was also discovered on this cliff. Around January 2012, this site had temperatures near 60°C, but temperatures in February ranged from 90° to 275°C.

Ground deformation recorded by a GPS network continued to show a trend of ongoing inflation, a behavior similar to previous pauses.

Activity from 1 May 2012 to 12 October 2012. Among 21 bursts of small earthquakes, the most notable occurred on 11 September 2012. Over the course of 13 hours, a low amplitude VT swarm resulted in 17 events, with the maximum M_L around 1.3. Eight rockfalls and two hybrid earthquakes were noted alongside typical seismic activity.

On 13 and 14 October 2012, tropical storm Rafael triggered eight seismically detected lahars in this region. The most noteworthy were those in the Belham Valley. Also, the SO₂ flux was slightly decreased from the previous reporting period, with an average of 280 tons/day.

As of October 2012, the E and W flanks had been determined to be the most unstable areas of the edifice, based on the presence of fresh rockfall deposits and pyroclastic flows. A large pyroclastic flow from the W flank could travel into Plymouth, the former capital destroyed by previous pyroclastic flows.

On 29 August 2012, a large pyroclastic flow originated at the 2006-2007 dome. This has been the largest pyroclastic flow in Tar River since the end of Phase 5 extrusion. Another pyroclastic flow occurred on 19 September 2012 in Gage's Valley. It originated from the steep slope adjacent to Chance's Peak and traveled about 1 kilometer. The sources of these pyroclastic flows can be viewed in figure 92.

Figure 92. Two photographs showing features at Soufrière Hills. The photograph on the left shows the source of the 19 September 2012 pyroclastic flow. The photograph on the right shows the source and flow direction of the 29 August pyroclastic flow. Courtesy of MVO.

A 10-minute exposure photo taken on 6 September 2012 determined no changes in location and number of incandescent areas on the N flank. However, the large fumarole in the floor of the 11 February 2010 collapse scar reached temperatures of ~300°C, and was the source of weak ash venting on 8 August 2012. Thermal IR camera imaging, showed the brightest point of incandescence, which reached temperatures over 400°C, originated from a hole in the rear of the collapse scar.

It should be noted that from August 2012 to November 2012, measurements at three local continuous GPS (cGPS) stations, AIRS, SPRI, and MVO1, had slight shortening of the radial distance between stations and vents, which may indicate short-term reversal of the long term inflation trend. Conclusions remain speculative without testing with more data.

Activity from 13 October 2012 to 30 April 2013. The largest of seven VT strings occurred on 30 November 2012. That swarm had a total of 23 earthquakes, with M_L of 2.1 or less. As mentioned in the introduction, a brief VT swarm occurred on 24 December 2012, but the four swarms of main interest followed on 3-5 February 2013. The most intense, with a total of 36 events in 27 minutes, occurred on 4 February, with a maximum M_L of 2.6. As a result, there was an increase in temperature of fumaroles residing on the 11 February 2010 collapse scar. This escalation continued until later in the evening, and at 1750 loud roaring sounds were heard, accompanied by minor ash venting. Activity and temperature returned to background levels the next day. This activity was noticeably similar to the events of 23 March 2012. Both were preceded by smaller VT strings, about 11 hours earlier, and the most intense phase had a 10-minute duration. There followed a VT string on 5 February associated with minor ash venting from the main gas vent in the floor of the 11 February 2010 collapse scar, as shown in figure 93.

Figure 93. Two thermal images, viewed from MVO and Jack Boy Hill, show the source of the ash venting on 5 February 2013, as well as a newly observed incandescence. Courtesy of MVO.

The next prominent seismic activity occurred on 15 and 19 April 2013. The earthquakes had M_L of 3.0 and 2.9, respectively, and neither were part of a VT string. The last time isolated VT earthquakes occurred was 28 June and 9 October 2011. Beside VT strings, 15 low-frequency earthquakes, which encompassed long-period and hybrid events, were observed during the October 2012 to April 2013 recording period. As of April 2013, 51 VT strings have occurred, and 13 have directly preceded surface activity.

Heavy rainfall on 28 and 30 March 2013 generated large lahars, lasting several hours, in various valleys around Soufrière Hills, including Belham Valley. The average daily SO₂ flux, as of April 2013, was 511 metric tons/day, with a high of 2,381 tons on 6 February 2013. This was the highest value observed since the ash venting of 23 March 2012. The connection between SO₂ flux and VT activity is still not thoroughly understood, but there seems to be an increase of SO₂ a few days before seismic events at Soufrière Hills.

Pyroclastic flow activity had followed the trends of previous pauses. On 28 March 2013, a pyroclastic flow traveled 1.5 km E through Tar River Valley. This pyroclastic flow began at a peeled-away slab of lava on the near-vertical E face of the dome. This was one of the largest pyroclastic flows since the start of Pause 5, and it removed a large portion of the lava slab on the 2006-2007 dome. This flank became heavily fractured as a result of weather and erosion, continued cooling, and contraction of the E flank of the dome above Tar River. Consequently, the Tar River side of the dome will likely be the source of future pyroclastic flow activity. Rockfall activity has been at its lowest since 10 February 2010, consistent with the stabilization of the dome over the past three years.

After 5 February 2013, temperatures in the collapse scar were ~100°C higher than previously recorded. That increase may be due to MVO's use of a new more sensitive IR camera (a FLIR T650sc), replacing their old (Mikron) camera. The new camera records temperatures that are corrected for atmospheric conditions.

Figure 94 emphasizes the difference in sensitivity between the two cameras. However, the distance at which these images were captured, about 5.7 km from the dome, results in unreliable temperature readings. This is because infrared light is absorbed, scattered, and refracted by dust, air, and water (in solid, liquid, or gaseous states). Variables such as solar reflection, heat from direct sunlight, condensates, and high concentrations of SO₂ in the atmosphere can also result in errors in image readings.

Figure 94. For Soufrière Hills, a juxtaposition of thermal images to highlight the difference in resolution and displays between the old infrared-detecting (IR) camera (left) and the more sensitive and accurate new one (right). Although there are temperature scales to the right of each image (22.4-32.4 on the scale at right), they are not applicable in this instance owing to multiple factors (see text). Even at this distance, IR images give scientists greater clarity on dome behavior. Despite the loss of the temperature scale, the images serve as an important tool for monitoring the state of the dome. Both IR photos taken during early 2013. Courtesy of MVO.

According to Adam J. Stinton, a volcanologist at MVO, the new camera produces images twice the size of the older camera due to a larger internal sensor, and therefore the right-hand image was scaled down to a comparable size. Thermal imaging technology works by recording the intensity of radiation in the infrared part of the electromagnetic spectrum and converting it to a radiometric image, with every pixel in the image conveying a temperature measurement.

Using the FLIR camera, a strong fumarole on the summit of the 2006-2007 dome was recorded on 15 March 2013, the first time this fumarole was ever imaged. Its temperature was between 250 and 260°C. No other new thermal features or incandescence had been recorded during this period.

As of April 2013, the trend of long-term edifice inflation continued. This suggested that the magmatic system is still actively deforming surficial areas. MVO observed similar deformation signals during previous pauses in extrusion.

Activity during April 2013 to March 2014. On 14 January 2014, a helicopter assessment of several groups of fumaroles revealed temperatures of 140-340°C within the summit crater. These fumaroles were observed for the first time since 2011. Aside from this detection, there has been a low level of activity at Soufrière Hills, including occasional rockfalls and seismic activity.

Background on seismicity. According to Druitt and Kokelaar (2002), hybrid earthquakes are long-period earthquakes located at (shallow) depths of less than 2 km. LP earthquakes, on the other hand, are widely interpreted as earthquakes associated with the movement of pressurized fluids (eg., BGVN 20:08).

According to MVO, using M_L offers possible advantages when calculating cumulative VT energy. The Gutenberg-Richter magnitude-energy relationship portrays an earthquake's size based on the amplitude of the resulting waves recorded on a seismogram. The concept is that the wave amplitude portrays the earthquake's size once the amplitudes are corrected for the decrease in magnitude with distance owing to geometric spreading and attenuation (Stein and Wysession, 2003). Local magnitude (often also termed Richter magnitude or the Richter scale). MVO employs the following (base 10) logarithmic equation, which associates ML to cumulative VT energy, E, as follows: Log E = 1.5 × ML + 11.8

MVO notes that this equation is a reliable calculation of cumulative energy, as opposed to amplitude measurements at a single station. Amplitude measurement data are easily affected by variables such as data gaps. As further background, magnitudes can be negative for very small displacements (eg. a small rockfall). Stein and Wysession (2003, p. 263) make the point that seismic magnitude scales are logarithmic, ". . . so an increase from magnitude "5" to "6," indicates a ten-fold increase in seismic wave amplitude. Measured displacements range more than 10 units because the displacements measured by seismometers span more than a factor of 1010." In practice, the amplitude is measured in microns of displacement after the effects of the seismometer are removed. Different magnitude scales (eg., M_L, mb, M_s, M_w, etc.) yield different values (Stein and Wysession, 2003).

References: Cole, P., Bass, V., Christopher, T., Melander, S., Pascal, K., Smith, P., Stewart, R., Stinton, A., and Syers, R., undated, MVO Scientific Report for Volcanic Activity Between 1 May 2012 and 12 October 2012, Open File Report OFR 12-02; Montserrat Volcano Observatory, 47 pp. (URL: http://www.mvo.ms/pub/Open_File_Reports/MVO_OFR_12_02-MVO_Scientific_Report.pdf)

Cole, P., Bass, V., Christopher, Odhert, H., Smith, P., Stewart, R., Stinton, A., Syers, R., and Williams, P., undated, MVO Scientific Report for Volcanic Activity Between 1 November 2011 and 30 April 2012. Montserrat Volcano Observatory, (URL: http://www.mvo.ms/pub/Open_File_Reports/MVO_OFR_12_01-MVO_Scientific_Report.pdf)

Druitt, T. and Kokelaar, B., 2002, The Eruption of Soufriere Hills Volcano, Montserrat, form 1995 to 1999, Issue 21. Geological Society Memoir No. 21. UK: The Geological Society Publishing House, 2002.

Stein, S. and Wysession, M., 2003, An Introduction to Seismology, Earthquakes and Earth Structure, 2003, Blackwell Publishing, Oxford, 498 pp. [ISBN 0-86542- 078-5]

Stewart, R., Bass, V., Christopher, T., Cole, P., Dondin, F., Higgins, M., Joseph, E., Pascal, K., Smith, P., Stinton, A., Syers, R., and Williams, P., (27 May) 2013, MVO Scientific Report for Volcanic Activity Between 13 October 2012 and 30 April 2013, Open File Report, OFR 13-06. Montserrat Volcano Observatory. (URL: http://www.mvo.ms/pub/Open_File_Reports/MVO_OFR_13_06-Six_monthly_report.pdf )

Geologic Background. The complex, dominantly andesitic Soufrière Hills volcano occupies the southern half of the island of Montserrat. The summit area consists primarily of a series of lava domes emplaced along an ESE-trending zone. The volcano is flanked by Pleistocene complexes to the north and south. English's Crater, a 1-km-wide crater breached widely to the east by edifice collapse, was formed about 2000 years ago as a result of the youngest of several collapse events producing submarine debris-avalanche deposits. Block-and-ash flow and surge deposits associated with dome growth predominate in flank deposits, including those from an eruption that likely preceded the 1632 CE settlement of the island, allowing cultivation on recently devegetated land to near the summit. Non-eruptive seismic swarms occurred at 30-year intervals in the 20th century, but no historical eruptions were recorded until 1995. Long-term small-to-moderate ash eruptions beginning in that year were later accompanied by lava-dome growth and pyroclastic flows that forced evacuation of the southern half of the island and ultimately destroyed the capital city of Plymouth, causing major social and economic disruption.

Information Contacts: Montserrat Volcano Observatory (MVO), Fleming, Montserrat, West Indies (URL: http://www.mvo.ms/); Washington Volcanic Ash Advisory Center (VAAC); and Adam Stinton, MVO.

Our previous report from May 2013 (BGVN 38:05) noted Strombolian activity, including volcanic bombs in July 2012 and ashfall and volcanic bombs in April and May 2013. The Vanuatu Geohazards Observatory (VGO) bulletin from 28 May 2013 noted that Yasur's explosive activity had increased slightly, compared to the recent past. The activity included Strombolian explosions (figure 43) and ash and steam plumes. This report discusses activity from June 2013 through February 2014, along with photographs taken in May 2013. A map of Vanuatu and nearby countries was provided in BGVN 35:06.

Figure 43. Strombolian activity from Yasur recorded during May 2013. Courtesy of Volcano Discovery (Dietmar Berendes).

Observations and seismic data from early to mid-August 2013 suggested that explosive activity of the volcano had decreased slightly during that time. Explosions were weaker and less frequent. Therefore, on 29 August 2013, the VGO decreased the Alert Level from 2, where it had been since early April 2013, to 1. Level 1 (on a scale of 0-4) indicates "increased activity [but] danger near crater only". From 29 August 2013 until at least February 2014, the Alert Level has remained at 1.

Hazard zones at Yasur are indicated in figure 44. VGO has warned visitors that ejected volcanic bombs could hit the summit area, the tourist walk, and parking area.

Figure 44. This danger map ('Denja Map') of Tanna Island containing Yasur volcano shows Red, Yellow, and Green zones to warn visitors and civilians of ashfall and other hazards. Yasur volcano is near the eastern end of the red, highest-risk zone. Map key and title are in a language with phonetic similarities to English that evolved with contact from traders (a lingua franca) but many other languages also remain in use in Vanuatu. Ash could likely fall well W of Yasur due to trade winds from the ESE. This image is of low to moderate resolution and some symbols are illegible. Courtesy of Vanuatu Geohazards Observatory.

Observations and seismic data from early to mid-August 2013 suggested that explosive activity of the volcano had decreased slightly during that time. Explosions were weaker and less frequent. Therefore, on 29 August 2013, the VGO decreased the Alert Level from 2, where it had been since early April 2013, to 1. Level 1 (on a scale of 0-4) indicates "increased activity [but] danger near crater only". From 29 August 2013 until at least February 2014, the Alert Level has remained at 1.

According to John Search, who has led tours of the volcano since 1998, activity increased beginning October 2013. A large ash emission caused widespread damage to vegetation on Tanna Island, and ashfall was reported on Erromango Island, 150 km N of Yasur. On the evening of 3 November 2013, Search witnessed large Strombolian explosions. These explosions ejected volcanic bombs, up to 4 m in diameter, 250 m from the vent, putting visitors at risk. According to Search, the explosions were some of the largest at Yasur since 1995.

On 19 November 2013, VGO reported that a new phase of ash emissions began on 3 November. The explosive intensity remained low.

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

Information Contacts: Vanuatu Geohazards Observatory, Department of Geology, Mines and Water Resources of Vanuatu (URL: http://www.geohazards.gov.vu); John Seach, Volcanolive.com (URL: Volcanolive.com/Yasur.html); and Volcano Discovery (www.volcanodiscovery.com).