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/).

This report extends our recent coverage of Bardarbunga (BGVN 39:10) by discussing activity between 7 January 2015 and 1 May 2015, although the eruption ceased on 28 February 2015. Most of the information below is based on reports from the Icelandic Met Office (IMO), with ancillary information from other agencies as noted. For sources other than the IMO reports shown in the reference list, see the websites provided in the "Information contacts" section at the end of this report. In general, the information sources there closely coincides with the date range of interest. The eruption began at Holuhraun on 31 August 2014 (BGVN 39:10).

IMO reports for January 2015 noted that activity at Bárdarbunga's Holuhraun lava field grew slightly along its N and NE margins. The lava field covered 84.1 km²on 10 January, 84.3 km² on 15 January, and 84.7 km² on 22 January. Seismicity remained strong, for example, an earthquake swarm occurred on 29 January 2015. (Specific numbers of earthquakes appear in some IMO reporting, although no plot has emerged with graphical depiction of earthquakes in this reporting interval such as figure 5 in BGVN 39:10.) Local air pollution from gas emissions persisted. GPS measurements showed that subsidence continued. As measured on the ice surface, total subsidence of the Bárdarbunga surface between mid-August 2014 and the end of January 2015 was 61 m. During this period, IMO maintained an Aviation Colour Code of Orange (the second highest on a five-color scale).

IMO noted that on 21 January, "Handheld meters, carried by scientist near the eruptive site . . . showed SO₂ concentrations of 29 ppm and 14 ppm. This is in concordance with the sulphur veils apparent from the aircraft and is reminiscent of the circumstances in SE Iceland [on] 28 October 2014. Since 1 ppm is about 3000 μg/m³ [micrograms per cubic meter ] this refers to concentrations of 87,000 μg/m³ and 42,000 μg/m³ respectively. For comparison, see values in the table compiled by the Environment Agency of Iceland and the Directorate of Health."

According to the Environmental Agency of Iceland, an SO₂ concentration above 14,000 μg/m³ is the most hazardous of six health hazard categories; the Agency advises that serious respiratory symptoms are to be expected. More specifically, the Agency states that when SO₂ concentrations exceed 14,000 μg/m³, residents should remain indoors, close the windows, and shut down air conditioning.

The Institute of Earth Sciences (IES) at the University of Iceland provided a map prepared on 21 January showing that the lava field was thickening and not spreading significantly; the volume of erupted lava was an estimated 1.4 km³ (15% uncertainty)(figure 11). An IMO report on 27 January stated that the average rate of lava emission during the previous three weeks had been just less than 100 m³ per second, taken by the report authors as a sign that the eruption intensity was slowly decreasing. On 27 January, a plume rose to an estimated height of 1.3 km above the plain.

Figure 11. Map of the new lava from Bardarbunga, prepared on 21 January 2015. During January, the lava thickened, without extending much further. Numbers indicate the thickness (m) which is also color-coded (legend on right). Courtesy of Institute of Earth Sciences (IES), University of Iceland.

On 6 February, IMO issued a statement that eruptive activity had decreased visibly during the previous two weeks, although seismicity was still strong. Lower seismicity continued during 11-19 February with many days of over a dozen earthquakes and seismic activity ranging up to M 4.3. On 14 February, the lava field covered 85 km²; measurements of the lava field's size on 4 and 12 February found no significant change.

An IES report issued on 20 February 2015 for 17-19 February 2015 noted "There is only one active vent inside the crater and the surface of the molten lava continues to sink. The lava channel has crusted over, except the 200-300 m nearest to the vent. The eruption column reaches no more than 1000 m above ground. The photos below show breakouts 15–16 km ENE of the vent, fed by the closed lava pathway which is inflating the lava field."

According to the IMO, a lava tube continued to feed the N and NE parts of Holuhraun, inflating the lava field. They also noted a reduced rate of effusion no longer sustained active breakouts in an area 17-18 km ENE from the vent.

A 24 February report noted that the rate of subsidence at Bardarbunga caldera was less than 2 cm per day. (IMO cautioned that care was needed with the interpretation of these data, given that GPS measurements are affected by ice flowing slowly into the caldera.) The eruption rate decreased substantially, and seismic activity continued to decrease although it was still considered strong.

IMO reported that a 27 February 2015 evening overflight found no visible incandescence at Holuhraun. According to FLIR thermal measurements, the radiant heat was greatest from the crater's rim, and lesser from the crater's depths. A gas detector in flight showed a maximum concentration of 0.5 ppm SO₂, and a maximum concentration of 0.4 ppm when tested on the ground at the SW edge of the lava field. Glowing areas were observed in the NE part of the lava field; the maximum temperature detected was 560°C (compared to 1,200°C earlier). Radar measurements showed that the extent of the lava field had not increased since mid-February. (Data from SENTINEL-1 radar image 0741 UTC 27 February 2015 and helicopter flight, 1515 UTC 27 February 2015). According to IMO, experience with other lava-bearing eruptions suggested that the Holuhraun lava field would continue to emit gas for a long time. Without buoyant rise, driven by thermal emission from an active vent, the gases would remain low (near the ground surface). Therefore, IMO expected even greater concentrations of gas than residents had previously seen.

IMO reported that the eruption at the fissure of Bárdarbunga's Holuhraun, which began on 31 August 2014 ended on 28 February 2015. The Aviation Colour Code was lowered to Yellow.

IMO scientists conducted a field study on 3-4 March 2015, and found no signs of activity, other than a diffuse bluish haze at ground level across the lava field (figure 12). The IMO scientists reported that the crater rim had several cracks at the very edge, and while standing close to the crater rim it was possible to hear rumbling due to movements of rocks/solidified lava inside the crater.

Figure 12. Photo of IMO geologists inside the Baugur crater on 4 March 2015. From the photo it appears that the vent discharging the lava is in the distance at the far end of the crater (area with white plume). According to the IMO caption, the photo was taken from the central part of Baugur crater as viewed looking along it to the N. The encrusted surface of the lava lake has collapsed, its remains seen as coarse, black rubble at the crater floor. On the crater floor, observers saw small vents sporadically discharging bluish gas. Part of the crater rim seen on the right side had broken, providing an outlet onto the lava field beyond. The resulting lava channel was about 50 m wide and 40 m deep. Courtesy of IMO (Ármann Höskuldsson; taken from IMO's March-April 2015 report).

In early March maximum CO (carbon monoxide) and SO₂ concentrations, measured with personal sensors near and at the crater rim, were 3 ppm and 2.5 ppm, respectively. A multiGAS instrument at the crater rim measured concentrations of SO₂, CO₂, H₂S, and H₂ for about 30 minutes, and provided ratios of CO₂/SO₂, H₂O/SO₂, and H₂O/CO₂ of 17, 101, and 6, respectively. The scientists noted that comparing the CO₂/SO₂ ratio with previous measurements showed a clear increase, consistent with the end of an eruption. The maximum concentrations measured with the MultiGAS instrument were at the level of 30 ppm for SO₂ (the concentration at which the instrument saturates). For CO₂ and H₂S, the respective measurements were 700 ppm and 5 ppm. The level of SO₂ was measured with an automatic gas detector, as reported by the Science Advisory Board of the Icelandic Civil Protection and disseminated by the Icelandic Commissioner of the Icelandic Police, as 500 µg/m³ (~0.5 ppm). Blönduós is a town and municipality in the North of Iceland situated on Route 1 at the mouth of the glacial river, Blanda. The report of the Police contained a links to a Gas Forecast and a Gas Model and involved scientists from the IMO and the IES along with representatives from the Icelandic Civil Protection, the Environmental Agency of Iceland and the Directorate of Health. The area to the SW and S of Blönduós was reported as possibly affected on the day following the measurement.

On 26 April, IMO lowered the Aviation Color Code to Green (the second lowest level), stating that no further signs of unrest had been noted since the end of the eruption on 28 February. Seismicity both within the caldera and the associated dyke intrusion continued to decline.

References.IMO, 2015 (January), Bárðarbunga 2015-January events, Seismic and volcanic events, 1-31 January, Icelandic Meteorological Office Accessed on 31 March 2015 (URL: http://en.vedur.is/earthquakes-and-volcanism/articles/nr/3071 ) (accessed May 2015).

IMO, 2015 (February), Bárðarbunga 2015-February events, Seismic and volcanic events, 1-28 February, Icelandic Meteorological Office Accessed on 31 March 2015 (URL: http://en.vedur.is/earthquakes-and-volcanism/articles/nr/3087 ) (accessed May 2015).

Geologic Background. The large central volcano of Bárðarbunga lies beneath the NW part of the Vatnajökull icecap, NW of Grímsvötn volcano, and contains a subglacial 700-m-deep caldera. Related fissure systems include the Veidivötn and Trollagigar fissures, which extend about 100 km SW to near Torfajökull volcano and 50 km NE to near Askja volcano, respectively. Voluminous fissure eruptions, including one at Thjorsarhraun, which produced the largest known Holocene lava flow on Earth with a volume of more than 21 km3, have occurred throughout the Holocene into historical time from the Veidivötn fissure system. The last major eruption of Veidivötn, in 1477, also produced a large tephra deposit. The subglacial Loki-Fögrufjöll volcanic system to the SW is also part of the Bárðarbunga volcanic system and contains two subglacial ridges extending from the largely subglacial Hamarinn central volcano; the Loki ridge trends to the NE and the Fögrufjöll ridge to the SW. Jökulhlaups (glacier-outburst floods) from eruptions at Bárðarbunga potentially affect drainages in all directions.

Information Contacts: Icelandic Met Office (IMO) (URL: http://en.vedur.is/); Institute of Earth Sciences (IES), University of Iceland (URL: http://earthice.hi.is); National Commissioner of Police, Department of Civil Protection and Emergency Management (URL: http://avd.is/en/); and The Environmental Agency of Iceland (URL: http://www.ust.is/the-environment-agency-of-iceland).

A submarine eruption began here by 19 December 2014 and ended by 28 January 2015. Hunga Tonga and Hunga Ha'apai are small islands situated on the rim of a submarine caldera known by the names of the two islands (Hunga Tonga and Hunga Ha'apai) (figure 12). The 2014-2015 surtseyan eruption added a circular area of land over 100 m in elevation at a spot S of and about midway along Hunga Ha'apai island's length. The new island initially grew as an isolated third new island, but subsequently connected and joined with Hunga Ha'apai. The area of new land surface eventually reached about 1.5 to 2 km in diameter. The new island also grew to come as close a few hundred meters from Hunga Tonga island. The eruption issued dense ash plumes that generally rose less than about a kilometer in altitude but preliminary estimates on the associated higher, ash poor steam plumes rose to 7-10 km altitude.

Figure 12.(Inset) A map showing a large scale view of the South Pacific with the Kingdom of Tonga highlighted in purple. (Main map) Hunga Tonga and Hunga Ha'apai lie on the rim of a submarine caldera located 65 km N of a wharf in the harbor at Nuku'alofa, Tongatapu island (the main island of the archipelago). Nuku'alofa is a deep-water port, the nation's capital, and Tonga's economic hub. Tongatapu island also hosts an international airport, which sits to the S of the capital. (The word "Ha'apai" is also used as the name of a region of islands and reefs well N of Hunga Tonga-Hunga Ha'apai.) The volcano also lies ~70 km SW of Normuka island. Courtesy of USGS.

This 2014-2015 eruption followed 5 years of quiescence, the previous eruption having occurred in 2009 (BGVN 34:03). That 2009 eruption formed new land above water and deposits destroyed vegetation on neighboring Hunga Tonga and Hunga Ha'apai islands (BGVN 34:03). The 2009 eruption added land at the S end of Hunga Ha'apai island. New research has been published discussing the 2009 eruption since our earlier report (BGVN 34:03). For example, Allen and Riebeek (2009) issued a 28 March 2009 Earth Observatory picture of the day that featured Hunga Tonga-Hunga Ha'apai images depicting the island morphology before and after the eruption. For another example, Vaughan and Webley (2010) discussed satellite observations associated with the 2009 eruption. Bohnenstiehl and others (2013) also discussed marine acoustic signatures from the 2009 eruption.

A key source used to create this report on the 2014-2015 eruption consists of four reports created by the Tongan Ministry of Information and Communications (MIC) and released during 14-28 January 2015. Those four MIC Advisories (numbers 3, 4, 5, and 6) are hereafter referred to as MIC (2015 a, b, c, and d). MIC 3 (2015a) was issued 14 January looking back in time at key aspects of the eruption. Discussions included the location and behavior of the first seen early observations on 20 December 2014, a site visit by the Tongan Navy on 6 January, and a pilot report on 13 January 2015. MIC 4 (2015b) was issued on 19 January describing a visit made on 14 January. This was the first report of the existence of a new island. By this time the new island had attached to Hunga Ha'apai island, roughly doubling the size of that island. MIC 5 (2015c) was also issued on 19 January. It described observations made from a visit aboard a ship (the VOEA Neiafu) on 17 January. MIC 6 (2015b) issued on 28 January describing for a visit on 24 January 2015. The report noted a lack of ash, gas, or steam coming from the vent that formed the new island. The authors concluded that the eruption "appears to be over." They provided a sketch map of the new island.

There were no new MIC reports during February-March 2015. The visits and reporting drew on support that included the Tonga Meteorological Services, NZ-Meteorological Services, the Tongan Navy, National Emergency Management Office, Tonga Broadcasting Commission, the New Zealand High Commission, and Ministry of Lands and Natural Resources, Tonga Airport Limited, Tonga Meteorological Services, GNS-NZ, NZ-Meteorological Services, and possibly others.

Eruption, December 2014. The online newspaper Matangi Tonga on 30 December noted that fishermen observed an eruption near Hunga Tonga-Hunga Ha'apai on 19 December 2014 (Matangi Tonga, 2014). An editor from that publication, Mary Lyn Fonua, notified GVP of the eruption. The same publication issued over 10 reports during 30 December 2014 through at least 9 March 2015 (Matangi Tonga, 2014, 2015a, b, c).

MIC (2015a) was released at 0943 on 14 January; it reported the position of the vent that was active on 20 December. Figure 13 is a later version of their figure, made at higher resolution. MIC (2015a) described this particular area as venting steam and sulfurous-gas at the sea surface. Emissions here did not persist during the later stages of the eruption.

Figure 13. A map (N to top) showing the location of steaming at Hunga Tonga-Hunga Ha'apai volcano (orange icon) on 20 December 2014. Each of the two islands are about 2 km long and lie on margins or rim of the mostly submarine caldera, with Hunga Tonga island to the N, and Hunga Ha'apai island to the W of the caldera's center. The area circled in red is the approximate location of the vent that later formed a new rapidly growing island. Taken from Culture Volcan (2015).

Klemetti (2014) showed an image from a MODIS instrument aboard the Aqua satellite that captured of the area of the eruption on 29 December 2014 (figure 14). A small white plume was in evidence at the volcano in the image. He commented that the area of discolored water stretching to the S could be due to the eruption.

Figure 14. The eruption plume from Hunga Tonga-Hung Ha'apai seen on 29 December 2014 by Aqua's MODIS Imager. Image by NASA with annotations by Erik Klemetti (Klemetti, 2014).

According to Metangi Tonga (2014) on 30 December 2014, "A continuing eruption from Tonga's active undersea volcano, Hunga Ha'apai, was clearly visible on the horizon northwest of Tongatapu today."

Activity during January 2015. During the 6 January visit (MIC, 2015a), observers nearing the volcano saw vigorous venting at a new location. MIC (2015a) did not disclose whether a new island had yet emerged but later reporting mentioned below did clearly document an island. The sea (or perhaps a very low island) discharged vigorous emissions of black ash and white billowing clouds. The new location was situated farther N, much closer to the preexisting islands, than the vent indicated in figure 13. That submarine vent to the S lacked further indications of steam emission during the course of the eruption. Neither of the preexisting islands appeared to contain active vents.

MIC (2015a) contained 11 captioned photos, but most are somewhat hazy and with limited contrast, conditions explained later (MIC, 2015b) as due to rain. Plumes on the 6th rose up to 2 km, but almost all the plumes in the photos were under 1.3 km altitude. At least one photo appeared to capture two low, vertical and parallel plumes. The photos documented some highly non-vertical black plumes, some peculiar low white plumes that seem to rise suddenly at distance, black plumes that appear to contain abundant clasts in their leading edge, low billowing clouds that encircle the darker ones and hug the water surface. In one case (figure 9 of MIC, 2015a) they reported that a white plume with its basal portion hugging the sea surface extended E over 3 km. The captions to their figures 10 and 11 indicated pulsing phenomena..

On 12 January 2015, Wellington VAAC reported ash from Hunga Tonga-Hunga Ha'apai reached an altitude of 6 km. They reported that fallout from the plume turned the sea surface red. Brief discussion of red colored sea surface is again mentioned below, both associated with observations on 14 January 2015 and briefly in a quote in an article by Field (2015).

The Wellington VAAC issued graphics to illustrate observed plume location and possible plume dispersal (figures 15 and 16). On figure 15 they labeled the altitude of the plume as SFC/FL200 (20,000 feet, ~6 km). The label "10/0500Z OBS" refers to the coordinated universal time (UTC) when the plume was observed. The next three cartoons represent movement of the ash plume at 6-hour intervals. The VAA graphic in figure 16 is based on the ash advisory mapping shows the recommended area of avoidance and several flight routes in the area.

Figure 15. Wellington VAAC Ash Advisory maps produced to describe the Hunga Tonga-Hunga Ha'apai plume and its trajectory. Times and dates are UTC (e.g., "10/0500Z" corresponds to 10 January 2015 at 0500 UTC). (Upper left) This is the observed ("OBS") ash plume's margin, which was traced onto this map from satellite image. This is the starting point for the subsequent forecasts. (Upper right) The forecast ("FCST") plume after 6 hours. (Lower left) The forecast plume after 12 hours. (Lower right) The forecast plume after 18 hours. Courtesy of the Wellington VAAC. [Maps extracted from NZ Met Service website (OBS-Observed; FCST, Forecasted) (http://vaac.metservice.com/vag/243040-2015_19)].

Figure 16.Wellington VAAC graphic showing the Hunga Tonga-Hunga Ha'apai ash plume boundararies for 12-13 January 2015 as an area enclosed in a blue polygon. The curved black lines in the center and at right are flight paths. Taken from the Wellington VAAC graphic for 12-13 January 2015.

MIC (2015a) noted that all international flights on 13 January 2015 were cancelled, though the domestic airline was operational. A Tongan government daily media release on 13 January described the ongoing eruption and cancellation of flights: "Activity continues at the Hunga Ha'apai-Hunga Tonga region and the emission of ash is reported to have escalated. Volcanic ash is forecasted to reach 870 km in 80 km wide toward the ESE from the Hunga Ha'apai-Hunga Tonga Region. By 11 January 2015, Real Tonga Airlines cancelled their flights for the day." Similar discussions of flight cancellation occurred around this time in Matangi Tonga, in their reports for 9, 13, 14 January.

On 13 January 2015 the Australian Aviation blog reported numerous flight cancellations, including Air New Zealand, Fiji Airways, and Virgin Australia. They also reported resumed service on 14 January 2015. According to Matangi Tonga (2015a) flights resumed on 15 January.

MIC (2015b, one of two reports issued on 19 January) discussed a site inspection on 14 January using a Tongan Navy vessel. The 14 January observations conveyed in MIC (2015b) noted that continuous volcanic eruptions had created a new island (figure 17). On 14 January the volcano was erupting about every five minutes. Ash and rock were ejected to a height of about 400 m above the sea surface. Wet ash was deposited close to the vent, building up the new island. Hazardous surges of ash and steam spread out horizontally during eruptions, and extended more than 1 km from the erupting vent (figure 18). Ash and acid rain fell in an area of ~10 km surrounding the eruption.

Figure 17. Sketch map of Hunga Tonga-Tonga Ha'apai as seen during a 14 January 2015 site inspection. The arrow points to the initial vent seen on 20 December 2014. The red circle indicates the location of the later vent that erupted for about a month, constructing an island with above water extent on 14 January 2015 in the area within the yellow circle. The circle is roughly 2 km in longest dimension. On the basis of this map, the minimum distance between Hunga Tonga island and the new land scales to ~300 m. Modified from MIC (2015b).

Figure 18. The new island amid eruption on 14 January 2015. The view is looking NE and the steep high area is Hunga Ha'apai island, which resides in behind the new island. The plume was made up of discrete white and dark components. From this perspective the vent appears to sit in the midst of the new low island. Photo taken on 14 January 2015 from the Tongan naval vessel ~300 m offshore (MIC, 2015b).

MIC (2015b) noted that on 14 January steam rose over 1 km and was noted by pilots. The eruption continued to emit ash but in recent days the presence of ash has been limited to low elevations. An early summary section in the report also include the following.

"The new island is more than 1 km wide, ~2 km long and about 100 m high. During our observations the volcano was erupting about every 5 minutes. Dense ash was being erupted to a height of about 400 m, accompanied by some large rocks. Higher we observed mostly steam, but with some ash. Above about 1000 m, the eruption plume was almost exclusively steam. As the ash is very wet, most is being deposited close to the vent, building up the new island.

"Hazardous surges of ash and steam were seen to spread out horizontally during eruptions, and these extended more than 1 km from the erupting vent.

"Ash fall and acidic rain was observed within 10 km of the eruption. Leaves on trees on Hunga Tonga and Hunga Ha'apai have died, probably caused by volcanic ash and gases.

"No large rafts of pumice or other floating volcanic debris were observed. Strong smells of volcanic gases were noticed on a few occasions.

"This eruption is similar to that at Hunga Ha'apai in 2009, but only producing larger volume of materials resulting in the size of the island.

"It is unclear at this stage if there is any relationship between the eruption and a red algal bloom observed in seawaters around Tonga recently."

Field (2015) contained an image from the 14 January site inspection (figure 19).

Figure 19. Hunga Tonga-Hunga Ha'apai eruption viewed from a Tongan naval vessel N of the island on 14 January 2015. Taken from Field (2015) with photo credit there given to the New Zealand High Commission in Tonga.

On 14 January Matangi Tonga (2015b) reported more details on the algal bloom mentioned above (the cause of which remains uncertain). Matangi Tonga (2015b) also reported unusual optical effects seen on the E facing side at the NE end of Tongatapu island (Kanokupolu beach) around that time. The article said the bloom "...turned the seas frothy white, chocolate and red..." and "...the sun shone through a champagne sky." The article contained photos by Shane Egan documenting these effects. Algal blooms can in some cases be detected and tracked by remote sensing as exemplified by Mantas and others (2011), who discuss remote sensing of algal communities as a possible cause of discolored water associated with the Home Reef eruption of 2006.

MIC (2015c) discussed a site visit conducted aboard a naval vessel on 17 January 2015. The authors noted that the eruption still continued at the new island during the visit. MIC (2015c) further stated the following. "During most of our time near the island, strong emission of steam to heights of 7–10 km was observed, but with only limited amounts of ash. Later, some eruptions that threw dense, wet ash, and small rocks 200-300 m into the air, accompanied by further strong emissions of steam. Hunga Tonga and Hunga Ha'apai islands were covered by ash from the eruption over the last month. The eruptions observed today were too small to deposit ash on those islands, suggesting that the eruptions a week or two ago were probably substantially stronger than those observed [on the 17 January site visit]. No trace of rafts of pumice or other floating volcanic debris was observed. No strong smells of volcanic gases were noticed within 3.7 km of the site, it was noticed however 27-47 km on the way to the site. The style of this eruption is similar to that at Hunga Ha'apai in 2009, but the volume of material erupted this time is much greater. International and domestic flights have operated without interruption in the last few days."

On 19 January 2015, the Pléiades satellite captured the Hunga Tonga-Hunga Ha'apai eruption. France's Centre National d'Etudes Spatiales (CNES) issued the resulting 50 m resolution images of the new land created by Hunga Tonga-Hunga Ha'apai's latest eruptions (figure 20). Hunga Tonga island in on the upper right; and Hunga Ha'apai, center left. In the center of the image is a nearly circular, gray colored area, which is the newly created land attached to Hunga Ha'apai island. The vent area on the new island was filled with water (green). Ash from the eruption covered extensive areas of the vegetation on both islands. This and other Images were featured in the article Airbus Defense and Space (2015).

Figure 20. CNES Pléiades satellite image (50-m resolution, optical band) taken on 19 January 2015. Ejecta from the new crater connects it to the E side of Hunga Ha'apai (island at left). Taken Airbus Defense and Space (2015) with data acquisition credit to CNES.

MIC (2015d) was issued on 28 January 2015 summarizing a 24 January site visit, which found the eruption over by this time. Figure 21 shows where the new land surface joins the preexisting Hunga Ha'apai island. Rough seas prevented landing and limited the trip to observations from the naval vessel. The scientists stated, "The eruption from the new island that started growing over a month ago appears to be over. There were no sign of any emissions of ash, gas or steam observed coming out from the vent of the newly formed island."

Figure 21. The point where new land adjoins the older island as seen in January 2015 after the Hunga Tonga Hunga Ha'apai eruption was over. The steep sea cliff forming the old margin of Hunga Ha'apai island is on the left. In the center and right parts of the image lie a low area of gently sloping gray material, which is an outer portion of the newly created land. Besides creating the new land, ash from the eruption covered vegetation over extensive areas on both the older islands. Taken from MIC (2015d).

On 13 March 2015, Luntz (2015) reported that on 6 March 2015 GP Orbassano and two other residents of Tonga landed on one of the new land's three beaches. With his son, he climbed to the highest point of the island's crater, which was ~250 m high. According to Luntz (2015), Tonga's lands and Natural Resources Ministry said the newly formed island was 1.3 km long and 800 m wide.

Orbasano smelled sulfurous and other chemical odors. The vent had filled with opaque green water (figure 22). Matangi Tonga (2015c) also reported on this same topic and featured numerous photos.

Figure 22. The crater lake in the vent area located in the central area of new land as seen on 6 March 2015. Courtesy of Luntz (2015) with photo credit to GP Orbassano.

Luntz (2015) quoted Orbassano as saying "the ash and rock surface was difficult to walk on due to the channels cut in it" (figure 23).

Figure 23. The highest peak on the new land as seen as seen on 6 March 2015. Note extensive rills and gullies. Taken from Luntz (2015) with photo credit to GP Orbassano.

"There are thousands of seabirds--all kinds, laying eggs on the island," Orbassano said (figure 24).

Figure 24. On the new land surface at Hunga Tonga-Hunga Ha'apai, these sea bird eggs were found laid directly upon the fragmental deposits. Taken on 6 March 2015. Courtesy of Iflscience and GP Orbassano.

References. Allen, J, and Riebeek, H, 2009, Submarine Eruption in the Tonga Islands NASA image, (28 March 2009, NASA Earth Observatory, Image of the Day) NASA (URL: http://earthobservatory.nasa.gov/IOTD/view.php?id=37657) (accessed May 2015)

Australian Aviation, 2015, Volcano ash cloud disrupts Tonga flights, Australianaviation.com.au (posted 13 January 2015) (accessed May 2015) (URL: http://australianaviation.com.au/2015/01/volcano-ash-cloud-disrupts-tonga-flights/ )

Airbus Defense and Space, 2015, Eruption of a volcano in the Tonga archipelago, Pléiades captures the birth of a new island (accessed March 2015) (URL: http://www.geo-airbusds.com/en/6322-eruption-of-a-volcano-in-the-tonga-archipelago-pleiades-captures-the-birth-of-a-new-island)

Bohnenstiehl D.R., Dziak R.P., Matsumoto H., Lau T.K. Underwater acoustic records from the March 2009 eruption of Hunga Ha'apai–Hunga Tonga volcano in the Kingdom of Tonga. J. Volc. Geotherm. Res. 2013;249:12-24.

Culture Volcan (Journal d'un volcanophile), 2015, L'activité du volcan Hunga Tonga Hunga Ha'apai a-t-elle changé de style? (posted 14 January 2014) (URL: http://laculturevolcan.blogspot.com/2015/01/lactivite-du-volcan-hunga-tonga-hunga.html)

Field, M, 2015, Tonga volcanic eruption creates new island, Stuff.co, posted 16 January 2015 (URL: http://www.stuff.co.nz/world/south-pacific/65103454/tonga-volcanic-eruption-creates-new-island ).

Klemetti, E, 2014, New Eruption at Hunga Tonga-Hunga Ha'apai, Wired (online), posted 30 December 2014 (accessed 6 June 2015).

Luntz, S, 2015, Newly emerged Pacific "Island" photographed for the first time, IFLSCIENCE (posted 13 March 2015. Accessed March 2015 (URL: http://www.iflscience.com/physics/newly-emerged-pacific-peak-photographed-first-time).

Mantas, V M, Pereira, AJSC., and Morais, PV, 2011, Plumes of discolored water of volcanic origin and possible implications for algal communities. The case of the Home Reef eruption of 2006 (Tonga, Southwest Pacific Ocean). Remote Sensing of Environment, v. 115, no. 6, p. 1341-1352.

Matangi Tonga, 2014, Hunga Ha'apai eruption continues, Matangi Tonga (Posted 30 December 2014; free content accessed in May 2015) (URL: http://matangitonga.to/2014/12/30/hunga-haapai-eruption-continues).

Matangi Tonga, 2015a, Fua'amotu airport's busiest day, as flights resume, Matangi Tonga (Posted 15 January 2015; free content accessed in May 2015) (URL: https://matangitonga.to/2015/01/15/fuaamotu-airports-busiest-day-flights-resume).

Matangi Tonga, 2015b, Nature plays with the sea and sky in Tonga, Matangi Tonga (Posted 15 January; free content accessed in May 2015) (URL: http://matangitonga.to/2015/01/15/nature-plays-sea-and-sky-tonga).

Matangi Tonga, 2015c, New volcanic island attracts sightseers, Matangi Tonga (Posted 9 March 2015; free content accessed in May 2015) (URL: http://matangitonga.to/2015/03/09/new-volcanic-island-attracts-sightseers).

MIC, 2015a, Government of Tonga Ministry of Information and Communication 3 (issued 14 January 2015) (URL: http://www.mic.gov.to/news-today/press-releases/5180-advisory-of-volcanic-activity-no3) (Accessed April 2015).

MIC, 2015b, Government of Tonga Ministry of Information and Communication 4 (issued 19 January 2015) (URL: http://www.mic.gov.to/news-today/press-releases/5185-volcanic-advisory-4) (Accessed April 2015).

MIC, 2015c, Government of Tonga Ministry of Information and Communication 5 (issued 19 January 2015) URL: http://www.mic.gov.to/news-today/press-releases/5183-volcanic-advisory-5) (Accessed April 2015).

MIC, 2015d, Government of Tonga Ministry of Information and Communication 6 (issued 28 January 2015) (URL: http://www.mic.gov.to/news-today/press-releases/5197-volcanic-advisory-6) (Accessed April 2015).

Vaughan, RG, Webley, P, 2010, Satellite observations of a surtseyan eruption: Hunga Ha'apai, Tonga, Journal of Volcanology and Geothermal Research. 12/2010; 198(1-2):177-186. DOI: 10.1016/j.jvolgeores.2010.08.017.

Geologic Background. The small andesitic islands of Hunga Tonga and Hunga Ha'apai are part of the western and northern remnants of the rim (~6 km diameter) of a largely submarine caldera located about 30 km SSE of Falcon Island. The topmost sequence of welded and unwelded ignimbrite units from a caldera-forming eruption was 14C dated to 1040-1180 CE (Cronin et al., 2017; Brenna et al. 2022). At least two additional welded pumice-rich ignimbrite units and nonwelded pyroclastic flow deposits, below paleosols and other volcaniclastic deposits, indicated more very large previous eruptions (Cronin et al., 2017; Brenna et al. 2022). Several submarine eruptions have occurred at this caldera system since the first recorded eruption in 1912, including 1937 and S of the islands in 1988. A short eruption in 2009 added land to to Hunga Ha'apai. At that time the two islands were each about 2 km long, displaying inward-facing sea cliffs with lava and tephra layers dipping gently away from the caldera. An eruption during December 2014-January 2015 was centered between the islands, and combined them into one larger structure. Major explosive eruptions in late 2021 initially reshaped the central part of the combined island before stronger activity in mid-January 2022 removed most of the 2014-15 material; an even larger eruption the next day sent an eruption plume high into the stratosphere, triggered shock waves through the atmosphere and tsunami across the Pacific Ocean, and left only small remnants of the islands above the ocean surface.

Information Contacts: Tonga’s Ministry of Information and Communications (URL: http://www.mic.gov.to); Tonga’s Natural Resources Division of the Ministry of Lands and Natural Resources (URL: http://www.mic.gov.to/ministrydepartment/14-govt-ministries/lands-survey-nat-res/); Mary Lyn Fonua, Matangi Tonga online (URL: http://matangitonga.to/); NASA Earth Observatory (URL: http://earthobservatory.nasa.gov/); Wellington Volcanic Ash Advisory Centre, NZ Meteorology Service (URL: http://vaac.metservice.com/); Tonga Meteorological and Coastal Radio service (URL: http://www.met.gov.to); GNS Science (formerly New Zealand’s Institute of Geological and Nuclear Sciences Limited), Taupo, New Zealand (URL: http://www.gns.cri.nz/); and GP (Gianpiero(?)) Orbassano, Waterfront Lodge, Vuna Road, Ma'ufanga, PO Box 1001, Nuku'alofa, Tonga (URL: http://www.waterfront-lodge.com/).

This report covers activity at Nyamuragira (also called Nyamulagira) (figure 47), primarily from April 2014 to January 2015, during which time there were intervals with lava fountains, high SO₂ fluxes, elevated thermal infrared emissions, and high seismicity. A lava lake was in clear evidence starting in November 2014 and into 2015. In the previous reporting interval (BGVN 39:03) an eruption occurred on 6 November 2011 and continued through April 2012. The reporting below begins with [information provided] by Benoît Smets and scientific colleagues including Nicolas d'Oreye, Nicolas Theys, and Julien Barriere.

Figure 47. 3D perspective view of the Virunga Volcanic Province, located between D.R. Congo and Rwanda. During the project TanDEM-X, radar interferometry was used to calculate a Digital Elevation Model (5-m resolution). Courtesy of F. Albino.

Activity during 2012 to early 2015. [The following is from the report submitted by Smets.]

"Starting from early March 2012, i.e. in the final stage of the five month-long eruption on the NE flank of Nyamulagira, SO₂-rich gas fumaroles were observed in the summit caldera of the volcano (D. Tedesco, Pers. Comm.). These fumaroles escaped from several fractures and from the 400-m-wide, 50-80-m-deep pit crater located in the NE part of the caldera. During the second half of April 2012, a larger and permanent SO₂-rich gas plume started to escape from that pit crater.

"In April 2014, local testimonies reported red glow on top of Nyamulagira. This was accompanied by unusual seismic activity recorded by the Goma Volcano Observatory (GVO). Because of intense degassing, helicopter flights at day and night did not allow detecting any fresh lava at ground surface. This kind of event reappeared on 22 June 2014. This time, helicopter flights and field surveys on 1 and 5 July 2014 did allow observing lava fountains escaping from the lowest inner flanks of the now ~500 m-deep and ~400 x 600 m-wide pit crater [figure 48]. At that time, lava fountains were not vigorous enough to create and sustain a basin of molten lava in the pit crater. This [lava fountaining] was also characterized by large amounts of SO₂-rich gas emissions.

Figure 48. A lava fountain in the deep crater at Nyamuragira, as seen by Smets from a helicopter on 1 July 2014. In addition, he posted a video of the helicopter flyby to YouTube (see Benoît Smets, 2015, in the References section). A lava lake was not indicated. Courtesy of Benoît Smets.

"This [lava fountaining] stopped mid-September 2014 and, on 1 November 2014, a small lava lake, i.e. a small bubbling lava basin, appeared in the deepest section of the pit crater (GVO, Pers. Comm.). The related SO₂ emissions appeared lower than during lava fountain activity. The lava lake activity at Nyamulagira seems to continue since [1 November 2014 through at least January 2015]. SO₂ gas emissions, radiated energy, and seismic activity during the April-December 2014 period illustrate very well the evolution of this new activity and the transition from lava fountaining activity to long-lived lava lake activity [figure 49]."

Figure 49. Graphs illustrating (top panel) seismicity, and (bottom panel) SO2 flux and radiated infrared energy at Nyamuragira during April to December 2014; (Green) seismicity in terms of Realtime Seismic Amplitude Measurement (RSAM), calculated using broadband seismometers at the Rumangabo station, ~20 km NE of the crater (installed in the RESIST and RGL-GEORISK projects); (Blue) SO2 emissions in the Virunga region, calculated using OMI measurements; (Red) radiated energy over Nyamuragira, calculated using MODIS imagery and the MODVOLC algorithm (Wright and others, 2004). Courtesy of Smets, d'Oreye, Nicolas Theys, and Julien Barriere.

Labels at the top of figure 49 represent behavior that Smets' team inferred on the basis of field observations. The intervals of quiet are unlabeled. The intervals with lava fountaining correspond with some intervals of high seismicity, high radiance, and pronounced SO₂ emissions. The intervals with the lava lake are somewhat similar to the fountaining in terms of seismicity and radiance but the SO₂ emissions were subdued.

According to the NASA MEASURES dataset, total atmospheric column SO₂ spiked during 19 to 26 June 2014. There was a period of low values during late September to early November 2014. After that and during the rest of the reporting interval, SO₂ was often elevated.

Lava lake. Observations of a lava lake were infrequent during much of 2014. Landsat 8 satellite images taken on 30 June 2014 and 29 July 2014 were interpreted by NASA Earth Observatory analysts Jesse Allen and Robert Simmon. They found "very hot surfaces" they interpreted as representing "the lava lake within the summit crater." Smets' team did not observe a lava lake during helicopter missions and an expedition to the volcano in July 2014. The team noted that by 1 November 2014 GVO had seen a small lava lake in the deepest part of the crater.

According to Bobrowski and others (2015) during 25 October to 5 November 2014 the lava lake was "still under formation" and field surveys carried out failed to find evidence for it. On the other hand, lava fountains were clearly observable in a ~350-m-wide crater, originating from an area of ~20 to 40 m². These fountains ejected materials and exhibited activity that the authors said might evolve into a new lava lake.

Once formed (by 1 November 2014), the lava lake was described as deep-seated and formed in a pit within the caldera's central N to NE area (Campion, 2014; Smets and others, 2014). As mentioned at the top of this report, Smets also noted that the lava lake continued to exist through and beyond January 2015 (the end of this reporting interval).

MIROVA stands for Middle InfraRed Observation of Volcanic Activity, where middle infrared is defined as 0.4-14.4 micrometer wavelengths. The infrared processing system uses source data that comes from the MODIS instrument that flies on the Aqua and Terra satellites. MIROVA makes plots of Volcanic Radiative Power (VRP). These are measurements of the heat radiated by hot volcanic products at the time of satellite acquisition. The VRP is calculated in Watts (W) and represents a combined measurement of the area of the volcanic emitter and its effective radiating temperature. MIROVA calculates the Volcanic Radiative Power (VRP) by using the "MIR method", an approach which was initially introduced by in order to estimate the heat radiated by active fires using satellite data (Wooster et al., 2003).

This approach (also known as Middle InfraRed method) relies on the fact that whenever a hot emitter has an effective radiating temperature higher than 600 K, the excess radiance detected in the MIR region (DLMIR), can be linearly related to the radiative power. Hence, for any individual hot-spot contaminated MODIS pixels, MIROVA calculates the VRP. (VRP = 18.9 x APIX x DLMIR where 18.9 is a best-fit regression coefficient (Wooster and others, 2003), APIX is the pixel size (1 km² for the MODIS pixels) and DLMIR is the above background MIR radiance of the pixel.) When a hot-spot is detected in more than one pixel, the total VRP is calculated as the sum of all pixels detecting a hot-spot.

Figure 50 is a time-series plot compiled by the MIROVA infrared processing system. All of the events on the plot that correspond to thermal anomalies are in the categories labeled low, moderate, and high. All of the events in the range moderate to high came from sources within 5 km of the crater (blue data points). Thermal emissions increased in June 2014, were minor for a period from late September to early November 2014, and increased once again for an interval extending through January 2015. Note the continuity of more elevated anomalies starting in November 2014, when there was clear evidence of the lava lake.

Figure 50. MODIS infrared data using MIROVA for the interval May 2014 through January 2015. The vertical scale shows 'Volcanic Radiative Power' (VRP, in Watts on a log scale, see text). Time is on the horizontal scale. As seen in the key at upper left, the blue data points represent those that occurred within 5 km of Nyamuragira's active crater, and the dark gray ones, over 5 km away. Courtesy of MIROVA.

MODIS instrument infrared data is automatically analyzed with the MODVOLC algorithm, creating alerts for cases with above-threshold thermal emissions. During April-May 2014, there were only six days with thermal alerts. Subsequently, the number of alerts increased in June 2014, in concurrence with the lava fountains. There were heightened periods of activity during 22–29 June and 1–3, 10–12, and 28 July. During August and September 2014, thermal events were once again sparse with occurrences only on three days. No events were observed in October. Consistent with other observations of the formation of a lava lake, alerts increased on 1 November and continued during 6–10 and 22–26 November. Thermal events occurred during 10–15 December and on 22, 24, and 31 December 2014. In January 2015, thermal activity was detected regularly during 9–18 and 25–30 January.

References. Bobrowski, N., Calabrese, S., Giuffrida, G., Scaglione, S., Liotta, M., Brusca, L., D'Alessandro, W., Yalire, M., Arellano, S., Galle, B., Tedesco, D, 2015, Intercomparison of gas emissions from the lava lakes of Nyiragongo and Nyamulagira, DR Congo/ Plume composition and volatile flux from Nyamulagira volcano, (abstract) Geophysical Research Abstracts, 2015 European Geophysical Union Meeting, Vienna, Austria (URL: http://meetingorganizer.copernicus.org/EGU2015/EGU2015-6540.pdf; http://meetingorganizer.copernicus.org/EGU2015/EGU2015-13100-1.pdf)

Campion, R., 2014, New lava lake at Nyamuragira volcano revealed by combined ASTER and OMI SO₂ measurements, 7 November 2014, Geophysical Research Letters (URL: http://onlinelibrary.wiley.com/doi/10.1002/2014GL061808/full)

Calabrese, S., Scaglione, S., Milazzo, S., D'Alessandro, W., Bobrowski, N., Giuffrida, G. B., and Yalire, M., 2014, Passive degassing at Nyiragongo (DR Congo) and Etna (Italy) volcanoes. Annals of Geophysics.

ESA Eduspace, date unknown, Nyiragongo and Nyamuragira, based on USGS, European Science Agency (URL: http://www.esa.int/SPECIALS/Eduspace_Disasters_EN/SEMDGLNSNNG_0.html) [accessed in May 2015]

Smets, B., 2015, Renewing activity at Nyamulagira volcano, 30 April 2015, Youtube (URL: https://www.youtube.com/watch?v=w1IHSjsgL48) [accessed in May 2015]

Smets, B., d'Oreye, N., Kervyn, F., 2014, Toward Another Lava Lake in the Virunga Volcanic Field?, 21 October 2014, EOS, Transactions American Geophysical Union (URL: http://onlinelibrary.wiley.com/doi/10.1002/2014EO420001/pdf)

Wooster, MJ, Zhukov, B, Oertel, D, 2003, Fire radiative energy for quantitative study of biomass burning: derivation from the BIRD experimental satellite and comparison to MODIS fire products. Remote Sensing Of Environment, 86(1), 83-107.

Wright, R., Flynn, L.P., Garbeil, H., Harris, A.J.L., Pilger, E., 2004. MODVOLC: near-real-time thermal monitoring of global volcanism. Journal of Volcanology and Geothermal Research 135, 29–49. doi:10.1016/j.jvolgeores.2003.12.008

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: Benoît Smets, (a) Center for Geodynamics and Seismology, Walferdange, Luxembourg; (b) Vrije Universiteit Brussel, Department of Geography; Earth System Science, Brussels, Belgium; (c) Royal Museum for Central Africa, Department of Earth Sciences, Natural Hazards and Cartography Service, Tervuren, Belgium; Nicolas d’Oreye, European Center for Geodynamics, and Seismology, Walferdange, Luxembourg and National Museum of Natural History, Geophysics/Astrophysics Department, Walferdange, Luxembourg; Nicolas Theys, Belgian Institute for Space Aeronomy, Brussels, Belgium; and Julien Barriere, European Center for Geodynamics and Seismology, Walferdange, Luxembourg and National Museum of Natural History, Geophysics/Astrophysics Department, Walferdange, Luxembourg; Goma Volcanological Observatory (GVO, aka Observatoire Volcanologique de Goma), Mt. Goma, Goma, Democratic Republic of Congo; Jesse Allan and Robert Simmon, NASA Earth Observatory (URL: http://earthobservatory.nasa.gov); NASA MEASURES (URL: https://so2.gsfc.nasa.gov/); MODVOLC alerts team, Hawai’i Institute of Geophysics and Planetology (HIGP), University of Hawai’i at Manoa, 1680 East-West Road, Post 602, Honolulu, HI 96822, USA (URL: http://modis.higp.hawaii.edu/); and MIROVA, Universities of Turin and Florence, Italy, Centre for Volcanic Risk of the Italian Civil Protection Department (URL: http://www.mirovaweb.it/).

Shishaldin, located on Unimak Island, is one of the most active volcanoes within the Aleutian Islands (figure 6). [Our last Bulletin report (BGVN 33:08) discussed activity at Shishaldin in February 2008, when a pilot reported a 3 km altitude ash plume. This report summarizes activity] from January to December 2009 and from January 2014 to March 2015. During 2009, Shishaldin emitted steam plumes, generated thermal anomalies, and underwent several episodes of tremor[; information for 2009 drew heavily on McGimsey and others (2014)]. From 2014 through March 2015, Shishaldin experienced elevated surface temperatures, steam emissions, and starting in March 2014, an ongoing low-level lava eruption within the summit crater that occasionally deposited ash on the upper flanks. As of March 2015, this low-level eruption continued. Considerable information in this report was found in material released by the Alaska Volcano Observatory (AVO).

Figure 6. Map showing the location of Shishaldin. The volcano is located near the center of Unimak Island, and is the tallest peak and one of the most active volcanoes within the Aleutians Islands. False Pass, located 38 km to the NE, is the closest town. Map is courtesy of Alaska Volcano Observatory and Alaska Division of Geological & Geophysical Surveys.

Activity during January-December 2009. According to AVO, activity began on 5 January (± 1 month) and ended on 16 August, and was characterized as a questionable eruption. According to McGimsey and others (2014), increased seismicity, small steam plumes as well as thermal anomalies characterized activity during 2009. Steam plumes are considered normal at Shishaldin according to McGimsey and others (2014).

McGimsey and others (2014), stated that there was an increase in observed thermal anomalies at Shishaldin in early January 2009. On 5-6 January, an AVHRR satellite image of Unimak Island showed a thermal anomaly centered on Shishaldin's summit crater. The anomaly reached a 2-pixel size on 6 January. There was also a slight increase in seismicity. These observations indicated a clear departure from background conditions. On 6 January, AVO increased Shishaldin's Aviation Color Code (ACC) from Green to Yellow and the Volcano Alert Level from Normal to Advisory. That day, pilots and ground observers reported a constant steam plume rising ~300 m above the summit and drifting 16-25 km SE (McGimsey and others, 2014).

Over the next few days, AVO continued observing a thermal anomaly in satellite images. On 7 January 2009, AVO received both a pilot report and observations from Cold Bay (93 km to the NE, figure 6) noting a vigorous steam plume rising from Shishaldin. On 8 January, satellite images showed a steam-filled crater with no ash on the flanks (McGimsey and others, 2014). AVO's 9 January 2009 Weekly Update stated "Although detection of a thermal anomaly is rare at this volcano, it is not certain that this unrest will lead to an eruption. A thermal anomaly was observed in the months leading up to the last significant eruption at Shishaldin [that occurred] in 1999; this fact, combined with the likelihood that an eruption at Shishaldin could occur with little or no seismic precursors, drove AVO's decision to raise the Color Code and Alert Level."

On 11 January 2009, a photo captured by a pilot showed pulsing steam plumes. Two days later, AVO seismologists identified a minor, low-amplitude tremor that persisted for a few weeks. According to McGimsey and others (2014), during the next few weeks, seismicity remained low, a few thermal anomalies were detected, and steaming was observed.

According to AVO's 13 February 2009 Weekly Update, a very weak thermal anomaly was detected on 3 February. The Update went onto say that on 11 February, the ACC was downgraded to Green and the Volcano Alert Level lowered to Normal, due to Shishaldin's return to background conditions. That Update also mentioned that seismic activity had remained low, since decreasing to background levels in late December 2008.

McGimsey and others (2014) reported that over the next seven weeks (mid-February to early April 2009) occasional thermal anomalies were observed along with continuous low-level tremor, which was not considered unusual. On 7 April, a pilot reported that he saw Shishaldin steaming more vigorously than he had previously observed during his weekly flights past Shishaldin over the last 16 months. That day, a thermal anomaly was also observed in satellite imagery (McGimsey and others, 2014).

On 20 April 2009, thermal activity at Shishaldin's summit spiked based on multiple thermal anomalies containing saturated pixels observed in satellite imagery (McGimsey and others, 2014). According to McGimsey and others (2014), these anomalies indicated high ground temperatures (greater than 300°C). This level of thermal activity was last seen before Shishaldin's eruption in 1999. On 5 May, a pilot reported steaming from Shishaldin and a passenger on a different flight reported dark-colored linear features on the N side of the summit. According to McGimsey and others (2014), these linear features were later interpreted as minor streams of dirty water trailing downslope.

McGimsey and others (2014) reported that throughout June 2009, thermal anomalies were detected on about one third of days, with a particularly strong anomaly being recorded on 9 June. No unusual seismic activity was noted. On the night of 25 June, an ASTER thermal infrared satellite image captured a thermal anomaly and a 22 km-long steam plume extending E-NE from Shishaldin. Then on 29 June, an observer in Cold Bay (93 km NE) reported increased steaming at Shishaldin over the past few days.

In the first week of July 2009, thermal anomalies at Shishaldin increased in intensity, with a return of saturated pixels, indicating high ground temperatures. On 10 July, AVO increased the ACC from Green to Yellow and the Volcano Alert Level from Normal to Advisory, due to the increase and continued presence of thermal anomalies. Seismicity and deformation did not change significantly during this time and satellite data did not show any noteworthy SO₂ emissions. On 13 July, emissions were detected in satellite imagery and a pilot reported a steam plume rising 600 m above Shishaldin and moving NW. On 15 July, the satellite-based Ozone Monitoring Instrument (OMI) detected a small cloud rich in SO₂ that originated from Shishaldin. For the rest of July and the first half of August 2009, steaming was observed from Shishaldin's summit, when weather permitted. Thermal anomalies were also detected in satellite images during August; one example was on 16 August.

In mid-September 2009, pressure sensors at Shishaldin detected anomalous airwaves. According to McGimsey and others (2014), the airwaves could be indicative of minor explosions; however, in retrospective analysis of the data collected by the pressure sensors, the airwaves were found to be a common occurrence and linked to episodic gas bursts (examples of which were seen during 2003-2004). On 19 October 2009, due to the continued absence of thermal anomalies, a decrease in steam emissions and seismicity considered within background levels, AVO lowered the ACC to Green and the Volcano Alert Level to Normal. Besides a weak thermal anomaly detected on 2 November, Shishaldin remained quiet for the remainder of 2009.

Non-eruptive interval during 2010-2013. AVO reported no unusual activity at Shishaldin between the years 2010 and 2013. In 2010, 2012 and 2013, AVO uploaded photos of Shishaldin, some of which showed the volcano emitting steam (figure 7).

Figure 7. Photograph of Shishaldin emitting a steam plume on 14 September 2013. The photograph was taken from Korpiewski (2013).

Activity during January 2014-March 2015. [AVO reported increased activity] on 28 January 2014 at Shishaldin. A low-level lava eruption within the summit crater then began in March 2014 and continued through March 2015. In addition to the ongoing eruption, there were also instances of heightened activity, one such example occurring around 28 October 2014, after AVO noted several days of elevated tremor and stronger thermal anomalies. AVO provides a description that synthesizes Shishaldin activity from late January 2014 through March 2015 on their website (as accessed on 1 May 2015). What follows is a quote of that description. For greater detail on activity during this interval, please see AVO's Weekly and Daily reports. Any information added to the quote by Bulletin editors has been [bracketed]. Bulletin editors also included pictures, depicting certain events that were described in the quote.

"On January 30, 2014, the Alaska Volcano Observatory raised the Volcano Alert Level to ADVISORY and the Aviation Color Code to YELLOW for Shishaldin, based on satellite observations of the previous days [figure 8]. Satellite observations included increased surface temperatures in the summit crater, as well as increased emissions of steam. Similar levels of unrest were last observed during 2009, and did not result in an eruption.

Figure 8. Satellite image of Shishaldin on Unimak Island captured at 0838 UTC on 30 January 2014. The image shows the elevated surface temperatures in the summit crater of Shishaldin. According to the AVO caption for this image, "This mid-infrared image is scaled so that warm values are bright white and cold values (like high clouds are dark). The elevated surface temperatures are visible as the white pixels within the yellow circle that indicates the location of Shishaldin." Image was created by Dave Schneider and is courtesy of Alaska Volcano Observatory/ U.S. Geological Survey.

"For the next week, persistent elevated surface temperatures were visible in satellite imagery of the summit crater during clear-weather intervals. On February 7, a possible volcanic cloud was observed in satellite images beginning around 1545 UTC (6:45 AKST). This cloud may have resulted from a small explosive event at the volcano. The event was small enough that it was not detected by the one working seismic station near the volcano, but it appears to coincide with a signal recorded by a nearby tiltmeter. Satellite images suggest that the cloud may have reached as high as [7.6 km above sea level], was ash-poor, and short-lived. There was no evidence of elevated surface temperatures observed in satellite data immediately following this event, suggesting it was primarily a gas event and very little to no hot material was produced or deposited on the flanks of the volcano.

"On March 19, elevated surface temperatures were again detected in satellite data, accompanied by ground-coupled airwaves seen in the seismic data. On March 28, after seeing persistent elevated surface temperatures since March 19, and continuing ground-couple airwaves, AVO data analysis showed temperatures in satellite images consistent with the eruption of lava within the summit crater. [The 28 March 2014 Volcanic Activity Notification (VAN) stated, 'The current activity appears to be confined to the deep summit crater and there have been no observations of lava on the flanks of the volcano or surrounding the summit crater.']

"During the week of April 11, minor ash deposits extending several hundreds of meters from the summit crater were observed in satellite imagery. Infrasound signals from Shishaldin were occasionally detected at sensors located at Dillingham [585 km to the NE] and Akutan Island [145 km to the SW].

"Throughout April, May, June, and July, elevated surface temperatures consistent with low-level eruptive activity in the summit crater were observed in satellite data, and small explosion signals were detected in seismic data. Occasional clear webcam views often showed minor steaming. An AVO overflight on August 10 showed hot, glowing material in the crater [figure 9]. On August 13, AVO received a pilot report of a low-level plume. [On 23 August, a pilot reported a steam-and-ash plume rose ~300 m above the summit and drifted NE.] Similar levels of activity continued throughout August, September, and October.

Figure 9. Photograph of incandescent material within Shishaldin's steaming summit crater and steam being emitted. This aerial photograph was captured on 10 August 2014 and shows ash deposited on the snow (in the left of the photo). Photo was captured by Cyrus Read and is courtesy Alaska Volcano Observatory/ U.S. Geological Survey.

"On October 28, 2014, AVO noted an increase in intensity over the past several days, including elevated seismic tremor and stronger thermal anomalies. New deposits of ash and ballistics darkened the summit area, and the activity was also recorded on infrasound stations at Akutan and Dillingham. [On 26 October, clear webcam images revealed tephra deposits at the summit. The 28 October 2014 VAN stated that these new deposits indicated, '…the activity was energetic enough to eject material from a depth of several hundred meters (~600 ft) within the summit crater.'] This period of increased tremor lasted for several further days.

"On November 24, seismic activity at Shishaldin again increased.... This increased seismicity declined by November 27, but remained above background. [AVO's 28 November 2014 Weekly Update said, 'Although the level of seismic activity has declined during the week, it is likely that a low-level lava eruption is ongoing within the summit crater of the volcano.'] Weak, but above background seismicity, along with weakly elevated crater surface temperatures, continued in December 2014 and January 2015.

"In late January 2015, strongly elevated temperatures were observed in satellite images, consistent with active lava within the crater. [AVO's 23 January 2015 Weekly Update stated, 'Activity [over the past week was] consistent with what we have observed at Shishaldin during the past several months, which includes lava effusion in the crater with occasional production of small amounts of ash restricted to the volcano's upper flanks.'] A wispy, low-level ash emission was observed in webcam images on February 2, 2015.

"Throughout February and March 2015, clear satellite views often show elevated surface temperatures at the crater, seismicity remained above background, and low-level steam emissions were frequently seen in webcam images. It is likely that low-level eruptive activity continued within the summit crater."

References.

Alaska Volcano Observatory (AVO), Shishaldin reported activity, URL: https://www.avo.alaska.edu/volcanoes/volcact.php?volcname=Shishaldin, date accessed: 1 May 2015

Alaska Volcano Observatory (AVO), Shishaldin reported activity, Event specific information [for 2009], URL: https://www.avo.alaska.edu/volcanoes/activity.php?volcname=Shishaldin&page=basic&eruptionid=76, date accessed: 1 May 2015

Alaska Volcano Observatory (AVO), Shishaldin reported activity, Event specific information [for 2014], URL: https://www.avo.alaska.edu/volcanoes/activity.php?volcname=Shishaldin&page=basic&eruptionid=77, date accessed: 1 May 2015

Alaska Volcano Observatory/Alaska Division of Geological & Geophysical Surveys, 2009, URL: http://www.avo.alaska.edu/images/image.php?id=16190, date accessed: 1 May 2015

Korpiewski, J., U.S. Coast Guard, 2013, URL: http://www.avo.alaska.edu/images/image.php?id=57087, date accessed: 13 May 2015

McGimsey, R.G., Neal, C.A., Girina, O.A., Chibisova, Marina, and Rybin, Alexander, 2014, 2009 Volcanic activity in Alaska, Kamchatka, and the Kurile Islands - summary of events and response of the Alaska Volcano Observatory: U.S. Geological Survey Scientific Investigations Report 2013-5213, 125 p., URL: http://pubs.usgs.gov/sir/2013/5213/

Read, C., Alaska Volcano Observatory/U.S. Geological Survey, 2014, URL: http://www.avo.alaska.edu/images/image.php?id=66771, date accessed: 13 May 2015

Schneider, D., Alaska Volcano Observatory/U.S. Geological Survey, 2014, URL: http://www.avo.alaska.edu/images/image.php?id=57691, date accessed: 13 May 2015.

Geologic Background. The symmetrical glacier-covered Shishaldin in the Aleutian Islands is the westernmost of three large stratovolcanoes in the eastern half of Unimak Island. The Aleuts named the volcano Sisquk, meaning "mountain which points the way when I am lost." Constructed atop an older glacially dissected edifice, it is largely basaltic in composition. Remnants of an older edifice are exposed on the W and NE sides at 1,500-1,800 m elevation. There are over two dozen pyroclastic cones on its NW flank, which is covered by massive aa lava flows. Frequent explosive activity, primarily consisting of Strombolian ash eruptions from the small summit crater, but sometimes producing lava flows, has been recorded since the 18th century. A steam plume often rises from the summit crater.

Information Contacts: Alaska Volcano Observatory (AVO), a cooperative program of the U.S. Geological Survey, 4200 University Drive, Anchorage, AK 99508-4667, USA (URL: http://www.avo.alaska.edu/), the Geophysical Institute, University of Alaska, PO Box 757320, Fairbanks, AK 99775-7320, USA, and the Alaska Division of Geological and Geophysical Surveys, 794 University Ave., Suite 200, Fairbanks, AK 99709, USA; Anchorage Volcanic Ash Advisory Center (VAAC), Alaska Aviation Weather Unit, and NWS NOAA US Dept of Commerce, 6930 Sand Lake Road, Anchorage, AK 99502-1845, USA (URL: http://vaac.arh.noaa.gov/).