Saunders
- United Kingdom
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- 2015 CE
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- 57.8°S
- 26.483°W
- 843 m
2765 ft - 390090
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- Summit
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Most Recent Weekly Report: 30 September-6 October 2015 
Cite this Report
The MODVOLC thermal alert system detected thermal anomalies over Michael’s summit crater during 30 September-7 October (GMT time, local -2).
Source: Hawai'i Institute of Geophysics and Planetology (HIGP) Thermal Alerts Team
Most Recent Bulletin Report: February 2016 (BGVN 41:01) Cite this Report
Thermal anomalies during August-October 2015
The Michael stratovolcano forms the emergent small, unpopulated, mostly ice-covered Saunders Island, part of the South Sandwich Islands. The volcano is primarily monitored using satellite imagery. Prior to August 2015, the most recent eruptive activity detected was in the second half of 2012 (BGVN 38:02).
Infrared MODIS satellite data processed by MODVOLC showed thermal alerts at the summit of Michael during 28 August to 8 October 2015 (figure 9, table 4). MODIS data presented on the MIROVA site shows increased radiative power (measured from satellite thermal data) from late August through October 2015, with a very strong maximum near the end of August (figure 10); lower-power gradually decreasing detections during late November 2015-January 2016 may represent a cooling lava flow. It should be noted that cloud cover over a volcano may prevent the measurement of infrared data.
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Figure 9. MODVOLC map of measured thermal alerts (each colored rectangle represents a pixel) during 28 August through 8 October 2015. Courtesy of MODVOLC. |
Table 4. Satellite thermal alerts measured by MODVOLC over Michael during August-October 2015. Pixel sizes generally range from 1-1.5 km2. Courtesy of MODVOLC.
| Date | Time (UTC) | Number of pixels | Satellite |
| 28 Aug 2015 | 0050 | 1 | Terra |
| 28 Aug 2015 | 0235 | 1 | Aqua |
| 30 Aug 2015 | 0225 | 1 | Aqua |
| 31 Aug 2015 | 0120 | 1 | Terra |
| 30 Sep 2015 | 0130 | 1 | Terra |
| 02 Oct 2015 | 0120 | 2 | Terra |
| 06 Oct 2015 | 1610 | 1 | Aqua |
| 08 Oct 2015 | 1660 | 1 | Aqua |
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Figure 10. MIROVA graph showing radiative power measured by satellite over Michael during April 2015 to April 2016, with a strong maximum on the last day of August 2015. Courtesy of MIROVA. |
Information Contacts: MIROVA, 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/)
Weekly Reports - Index
30 September-6 October 2015 Cite this Report
The MODVOLC thermal alert system detected thermal anomalies over Michael’s summit crater during 30 September-7 October (GMT time, local -2).
Source: Hawai'i Institute of Geophysics and Planetology (HIGP) Thermal Alerts Team
12 October-18 October 2005 Cite this Report
The first MODVOLC alerts at Mount Michael since May 2003 recently began, indicating an increased level of activity in the island's summit crater (and presumed lava lake). The alerts occurred on 3, 5, and 6 October.
Sources: Hawai'i Institute of Geophysics and Planetology (HIGP) Thermal Alerts Team; British Antarctic Survey
Bulletin Reports - Index
Reports are organized chronologically and indexed below by Month/Year (Publication Volume:Number), and include a one-line summary. Click on the index link or scroll down to read the reports.
Information is preliminary and subject to change. All times are local (unless otherwise noted)
February 2003 (BGVN 28:02) Cite this Report
Lava lake detected in satellite imagery during 1995-2002
Although previous eruptions have been recorded in the South Sandwich Islands (Coombs and Landis, 1966), ongoing volcanic activity has only recently been detected and studied. These islands (figure 1) are all volcanic in origin, but sufficiently distant from population centers and shipping lanes that eruptions, if and when they do occur, currently go unnoticed. Visual observations of the islands probably do not occur on more than a few days each year (LeMasurier and Thomson, 1990). Satellite data have recently provided observations of volcanic activity in the group, and offer the only practical means to regularly characterize activity in these islands.
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Figure 1. The South Sandwich Island archipelago, located in the Scotia Sea. The South Sandwich Trench lies approximately 100 km E, paralleling the trend of the islands, where the South American Plate subducts westward beneath the Scotia Plate. Courtesy Hawaii Institute of Geophysics and Planetology and British Antarctic Survey. |
Using Advanced Very High Resolution Radiometer (AVHRR) data, Lachlan-Cope and others (2001) discovered and analyzed an active lava lake on the summit of Saunders Island (figure 2) that was continuously present for intervals of several months between March 1995 and February 1998; plumes originating from the island were observed on 77 images during April 1995-February 1998. J.L. Smellie noted that during helicopter overflights on 23 January 1997 (Lachlan-Cope and others, 2001) "dense and abundant white steam was emitted from the crater in large conspicuous puffs at intervals of a few seconds alternating with episodes of less voluminous, more transparent vapour." Smellie also observed that the plume commonly extended ~8-10 km downwind.
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Figure 2. Map of Saunders Island, adapted from Holdgate and Baker (1979). Lighter shaded stippled areas show rock outcrop, the remainder is snow or ice covered. Relief is shown by form lines that should not be interpreted as fixed-interval contours. Courtesy Hawaii Institute of Geophysics and Planetology and British Antarctic Survey. |
The MODIS Thermal Alert system also detected repeated thermal anomalies throughout 2000-2002 in the summit area (figure 3), indicating that activity at the lava lake has continued. Anomalous pixels (1 km pixel size) were detected intermittently and were all 1-2 pixels in size, consistent with the relatively small confines of the crater. The timing of anomalous images in this study likely has more to do with the viewing limitations imposed by weather (persistent cloud cover masks any emitted surface radiance in the majority of images) than it has to do with fluctuations in activity levels, so this plot of radiance (figure 4) should not be used as a proxy for lava lake vigor.
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Figure 3. Selected MODIS images showing thermal anomalies on Saunders Island. Band 20 (3.7 µm) is shown here. Anomalous pixels on Saunders Island correspond to the lava lake in the summit crater of Mt. Michael volcano. Images are not georeferenced for purposes of radiance integrity, therefore coastlines are approximate. Courtesy Hawaii Institute of Geophysics and Planetology and British Antarctic Survey. |
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Figure 4. Summed radiance of anomalous pixels in each image. Band 21 (3.9 µm) was used for these plots. Points show the result for each image, and the line is a three point running mean of values. Courtesy Hawaii Institute of Geophysics and Planetology and British Antarctic Survey. |
References. Coombs, D.S., and Landis, C.A., 1966, Pumice from the South Sandwich eruption of March 1962 reaches New Zealand: Nature, v. 209, p. 289-290.
Holdgate, M.W., and Baker, P.E., 1979, The South Sandwich Islands, I, General description: British Antarctic Survey Science Report, v. 91, 76 p.
Lachlan-Cope, T., Smellie, J.L., and Ladkin, R., 2001, Discovery of a recurrent lava lake on Saunders Island (South Sandwich Islands) using AVHRR imagery: Journal of Volcanology and Geothermal Research, v. 112, p. 105-116.
LeMasurier, W.E., and Thomson, J.W. (eds), 1990, Volcanoes of the Antarctic Plate and Southern Oceans: American Geophysical Union, Washington, D.C., AGU Monograph, Antarctic Research Series, v. 48.
Wright, R., Flynn, L.P., Garbeil, H., Harris, A.J.L., and Pilger, E, 2002, Automated volcanic eruption detection using MODIS: Remote Sensing of Environment, v. 82, p. 135-155.
Information Contacts: Matt Patrick, Luke Flynn, Harold Garbeil, Andy Harris, Eric Pilger, Glyn Williams-Jones, and Rob Wright, HIGP Thermal Alerts Team, Hawai'i Institute of Geophysics and Planetology (HIGP) / School of Ocean and Earth Science and Technology (SOEST), University of Hawai'i, 2525 Correa Road, Honolulu, HI 96822, USA (URL: http://modis.higp.hawaii.edu/); John Smellie, British Antarctic Survey, Natural Environment Research Council, High Cross, Madingly Road, Cambridge CB3 0ET, United Kingdom (URL: https://www.bas.ac.uk/).
March 2004 (BGVN 29:03) Cite this Report
A MODIS thermal alert on 7 May 2003 (no secondary confirmation)
The only previous report on the remote Michael volcano was in BGVN 28:02, which commented on a lava lake detected by satellite imagery over the period 1995-2002. A review of MODIS data for the period from that report (end 2002) to 16 March 2004 (UTC) reveals one thermal alert, on 7 May 2003 (UTC). No corroborative report is available, although previous alerts were interpreted as possibly representing lava lake activity.
Information Contacts: Rob Wright, Luke Flynn, and Eric Pilger; MODIS Thermal Alert System, Hawaii Institute of Geophysics and Planetology (HIGP), School of Ocean and Earth Science and Technology, University of Hawaii at Manoa (URL: http://modis.higp.hawaii.edu/).
April 2006 (BGVN 31:04) Cite this Report
Lack of new thermal signals suggesting any eruption since October 2005
The last reported activity of Mount Michael was noted in the SI/USGS Weekly Report of 12-18 October 2005. At that time the first MODVOLC alerts for the volcano since May 2003 indicated an increased level of activity in the island's summit crater and a presumed semi-permanent lava lake that appeared confined to the summit crater. Those alerts occurred on 3, 5, and 6 October 2005. Since that time there has been no additional information concerning Mount Michael and presumably little to no activity.
Information Contacts: Matt Patrick, Luke Flynn, Harold Garbeil, Andy Harris, Eric Pilger, Glyn Williams-Jones, and Rob Wright, HIGP Thermal Alerts Team, Hawai'i Institute of Geophysics and Planetology (HIGP) / School of Ocean and Earth Science and Technology (SOEST), University of Hawai'i, 2525 Correa Road, Honolulu, HI 96822, USA (URL: http://modis.higp.hawaii.edu/); John Smellie, British Antarctic Survey, Natural Environment Research Council, High Cross, Madingly Road, Cambridge CB3 0ET, United Kingdom (URL: https://www.bas.ac.uk/).
October 2006 (BGVN 31:10) Cite this Report
Clear IR satellite view on 28 October 2006 suggests lava inside the crater
Matt Patrick sent a new Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER) image, collected 28 October 2006 over Saunders Island . In his opinion this is the best image collected to date owing to the lack of a plume obscuring the summit crater, which was a problem in all previous images. The improved image provides a clear view of the crater (figures 5 and 6).
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Figure 5. An ASTER image of Mt. Michael created using energy in the visible near-infrared wavelength ("VNIR"; bands 3-2-1, RGB), with the inset showing a closer view of the summit crater. There are two small near-IR anomalies (band 3, 0.807 microns wavelength) in the otherwise dark center of the crater, shown as red spots in the colored image. The two anomalies suggest very high temperatures and support the idea that fresh lava may reside at the surface or a shallow level in the crater. Courtesy of Matt Patrick. |
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Figure 6. The ASTER Short Wave Infrared (SWIR; band 9, 2.4 microns) image with a conspicuous anomaly at the summit, with numerous saturated pixels. Courtesy of Matt Patrick. |
Analyzing the VNIR, SWIR, and Thermal Infrared (TIR) (not shown in figures 5 or 6) images together shows that the outer crater is 500-600 m wide, with a 180m high-temperature crater interior. The latter shows up as an SWIR anomaly and may indicate the rough extent of active lava flow being ~ 180 m wide. Matt Patrick chose Villarrica volcano in Chile for comparison to Mt. Michael (figure 7) since it presents a potentially good analogue in terms of morphology and activity style. Maximum radiant heat flux values were similar (up to ~ 150 MW), suggesting that the maximum intensity of activity may be similar. Mt. Michael shows a much lower frequency of thermal alerts, which may be the result of more frequent cloud cover in the South Sandwich Islands or a greater depth to molten lava in the Mt. Michael crater.
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Figure 7. The real-time satellite thermal monitoring (MODVOLC) radiant heat flux values for Michael and Villarrica volcanoes during the period 2000-11 November 2006. Courtesy of Matt Patrick. |
Table 1 shows a summary of thermal anomalies and possible eruptions from Moderate Resolution Imagine Spectroradiometer (MODIS) satellites since November 2005. The last reported activity of Mount Michael was noted in the SI/USGS (Smithsonian Institution/U.S. Geological Survey) Weekly Volcanic Activity Report of 12-18 October 2005 (see BGVN 31:04). At that time the first MODVOLC alerts for the volcano since May 2003 indicated an increased level of activity in the island's summit crater and a presumed semi-permanent lava lake that appeared confined to the summit crater. Those alerts occurred on 3, 5, and 6 October 2005.
Table 1. Thermal anomalies measured by MODIS satellites for Mount Michael for the period 3 October 2005 to 1 November 2006. All of the anomalies appeared on the SW side of the volcano. Courtesy of Hawai'i Institute of Geophysics and Planetology (HIGP) Thermal Alerts Team.
| Date | Time (UTC) | Number of pixels | Satellite |
| 01 Nov 2006 | 0125 | 1 | Terra |
| 31 Oct 2006 | 1600 | 1 | Aqua |
| 21 Oct 2006 | 1120 | 1 | Terra |
| 20 Oct 2006 | 0250 | 2 | Aqua |
| 20 Oct 2006 | 0100 | 3 | Terra |
| 21 Jul 2006 | 0120 | 1 | Terra |
| 09 Jun 2006 | 0920 | 2 | Aqua |
| 21 Jan 2006 | 0100 | 1 | Terra |
| 20 Dec 2005 | 0100 | 1 | Terra |
| 06 Oct 2005 | 0115 | 1 | Terra |
| 05 Oct 2005 | 0220 | 1 | Aqua |
| 03 Oct 2005 | 0045 | 1 | Terra |
References. Lachlan-Cope, T., Smellie, J.L., and Ladkin, R., 2001, Discovery of a recurrent lava lake on Saunders island (South Sandwich Islands) using AVHRR imagery: Journal of Volcanology and Geothermal Research, vol. 112, no. 1-4, p. 105-116 (authors are members of the British Antarctic Survey).
LeMasurier, W.E., and Thomson, J.W. (eds), 1990, Volcanoes of the Antarctic Plate and Southern Oceans: American Geophysical Union, Washington, D.C., AGU Monograph, Antarctic Research Series, v. 48.
Information Contacts: Matt Patrick, Michigan Technological University, Houghton, MI; Thermal Alerts Team, Hawai'i Institute of Geophysics and Planetology (HIGP), School of Ocean and Earth Science and Technology (SOEST), University of Hawai'i, 2525 Correa Road, Honolulu, HI 96822, USA (URL: http://modis.higp.hawaii.edu/); John Smellie, British Antarctic Survey, Natural Environment Research Council, High Cross, Madingly Road, Cambridge CB3 0ET, United Kingdom (URL: https://www.bas.ac.uk/); ASTER Science Project Teams, United States and Japan (URL: https://asterweb.jpl.nasa.gov/).
April 2008 (BGVN 33:04) Cite this Report
No thermal anomalies detected since December 2006
The frigid, remote, and uninhabited region of Michael volcano is seldom visited. Thermal anomalies detected by satellite-based MODIS instruments, processed using the MODVOLC algorithm by the Thermal Alerts System of the Hawai'i Institute of Geophysics and Planetology, provide some data about possible eruptive activity (BGVN 28:02, 29:03, 31:04, and 31:10). During 3-6 October 2005 there were three days with thermal anomalies (BGVN 31:04). MODIS data indicates that anomalous pixels were also detected on 19 December 2005 (20 December UTC) and on 20 January 2006 (21 January UTC) (BGVN 31:10). The most recently reported MODIS thermal anomalies indicated activity during 19-21 October 2006 (20-21 October UTC) and again on 31 October-1 November 2006 (BGVN 31:10). The source of these anomalies was an inferred lava lake in a central vent as shown on an Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER) image collected 28 October 2006 (BGVN 31:10). Additional anomalies occurred on 13 November and 6 December 2006 (7 December UTC). No anomalies were measured after that date through May 2008. Since August 2000 there have been six periods when thermal anomalies were detected in satellite imagery (table 2).
Table 2. Eruptive periods at Michael as inferred from MODIS thermal data from January 2000 through May 2008. Courtesy of the Hawai'i Institute of Geophysics and Planetology Thermal Alerts System.
| Date (UTC) | Thermal pixel data | Bulletin reference |
| 30 Aug 2000-03 Feb 2001 | 3 days with pixels | BGVN 28:02 |
| 05 Aug 2001-21 Nov 2001 | 10 days with pixels | BGVN 28:02 |
| 05 Jul 2002-01 Nov 2002 | 12 days with pixels | BGVN 28:02 |
| 07 May 2003 | 2 anomalous pixels | BGVN 29:03 |
| 03 Oct 2005-21 Jan 2006 | 5 days with pixels, three during 3-6 Oct | BGVN 31:04, 31:10 |
| 09 Jun 2006-07 Dec 2006 | 9 days with pixels | BGVN 31:10, 33:04 |
Information Contacts: Hawai'i Institute of Geophysics and Planetology (HIGP) 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/).
February 2013 (BGVN 38:02) Cite this Report
Eruption from ‘new’ vent
Matthew Patrick (USGS-HVO) notified Bulletin editors that in late 2012 images from thermal sensing satellites showed a 'new' active vent on Mount Michael on Saunders Island in the South Sandwich Islands (see location map, figure 1 in BGVN 28:02). This prompted scrutiny of the same vent in earlier images. Patrick noted that, although the vent was first identified in the 2012 images, it also appeared as activity in satellite images starting in 2006. The South Sandwich Islands are generally devoid of vegetation and habitants, and are largely ice-bound. Thus, satellite thermal alerts are strong evidence of volcanism.
Patrick shared with us the following information from a paper by Patrick and Smellie (2013) about the vent, labeled as Old Crater (SE and outside of main crater, see figure 2 in BGVN 28:02). ASTER [Advance Spaceborne Thermal Emission and Reflection Radiometer] imagery provided "new information on the small subordinate crater, marked as 'Old Crater' by Holdgate and Baker (1979), presumably because it was inactive at the time of their observations." An ASTER image on 28 October 2006 showed an apparent SWIR [short-wave infrared] anomaly at Old Crater. The crater itself appeared to be snow-free and was approximately 150 m in diameter. An ASTER image from 5 January 2008, showed a steam plume coming from this vent, which appeared to be about 190 m wide, as well as a TIR [thermal infrared] anomaly. A very high resolution image from November 2009 available on Google Earth showed a small steam plume emanating from the crater, which is about 190 m wide (figure 8). An ASTER image from 17 November 2010, showed apparently recent eruptive activity in Old Crater, evidenced by tephra fallout emanating from the crater and a small TIR anomaly (at the time there was also a TIR anomaly in the main crater). According to Patrick and Smellie, the plume, tephra fall, SWIR anomalies, and crater enlargement (from 150 to 190 m) indicated that this vent had reactivated by late 2006.
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Figure 8. Annotated Google Earth imagery of Michael volcano (Saunders Island) acquired on 19 November 2009. (a) Saunders Island is mostly glacier covered, and steam plumes rose from the summit area. The scale bar indicates a distance of ~2.4 km. (b) A close up of the summit area that clearly shows steam plumes emanating from both the summit crater as well as the snow-filled 'Old Crater' (as termed by Holdgate and Baker, 1979). The scale bar indicates a distance of ~0.5 km. Courtesy of Google Earth. |
MODVOLC satellite thermal alerts measured from the volcano since our last Bulletin report (BGVN 33:04, activity through May 2008) and to 4 April 2013 are shown in Table 3. A solitary alert appeared 25 October 2008, followed by a four year period of apparent inactivity. Then, another solitary alert was measured in late June 2012, followed by alerts for two days in October 2012 and two days in November 2012. Patrick noted that occasional and sporadic alerts are very typical for Michael.
Table 3. Satellite thermal alerts measured by MODVOLC over Michael from 2008-February 2013. Pixel sizes generally range from 1-1.5 km2. Note that previous satellite thermal alerts for Michael were listed in BGVN 31:10 (October 2005-November 2006) and 33:04 (August 2000-May 2008). Courtesy of MODVOLC.
| Date | Time (UTC) | Number of pixels | Satellite |
| 25 Oct 2008 | 0100 | 1 | Terra |
| 30 Jun 2012 | 0100 | 1 | Terra |
| 02 Oct 2012 | 0110 | 1 | Terra |
| 28 Oct 2012 | 0200 | 2 | Aqua |
| 28 Oct 2012 | 1125 | 2 | Terra |
| 14 Nov 2012 | 0055 | 3 | Terra |
| 22 Nov 2012 | 1120 | 2 | Terra |
References. Patrick, M.R., and Smellie, J.L., 2013, A spaceborne inventory of volcanic activity in Antarctica and southern oceans, 2000-2010, Antarctic Science, v. 25, no. 4, p. 475-500.
Holdgate, M.W., and Baker, P.E., 1979. The South Sandwich Islands: I. General description, British Antarctic Survey Scientific Reports, No. 91, pp. 1-76.
Information Contacts: Matthew Patrick, Hawaiian Volcano Observatory (HVO), U.S. Geological Survey, PO Box 51, Hawai'i National Park, HI 96718, USA (URL: https://volcanoes.usgs.gov/observatories/hvo/); MODVOLC, Hawai'i Institute of Geophysics and Planetology (HIGP) 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/).
February 2016 (BGVN 41:01) Cite this Report
Thermal anomalies during August-October 2015
The Michael stratovolcano forms the emergent small, unpopulated, mostly ice-covered Saunders Island, part of the South Sandwich Islands. The volcano is primarily monitored using satellite imagery. Prior to August 2015, the most recent eruptive activity detected was in the second half of 2012 (BGVN 38:02).
Infrared MODIS satellite data processed by MODVOLC showed thermal alerts at the summit of Michael during 28 August to 8 October 2015 (figure 9, table 4). MODIS data presented on the MIROVA site shows increased radiative power (measured from satellite thermal data) from late August through October 2015, with a very strong maximum near the end of August (figure 10); lower-power gradually decreasing detections during late November 2015-January 2016 may represent a cooling lava flow. It should be noted that cloud cover over a volcano may prevent the measurement of infrared data.
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Figure 9. MODVOLC map of measured thermal alerts (each colored rectangle represents a pixel) during 28 August through 8 October 2015. Courtesy of MODVOLC. |
Table 4. Satellite thermal alerts measured by MODVOLC over Michael during August-October 2015. Pixel sizes generally range from 1-1.5 km2. Courtesy of MODVOLC.
| Date | Time (UTC) | Number of pixels | Satellite |
| 28 Aug 2015 | 0050 | 1 | Terra |
| 28 Aug 2015 | 0235 | 1 | Aqua |
| 30 Aug 2015 | 0225 | 1 | Aqua |
| 31 Aug 2015 | 0120 | 1 | Terra |
| 30 Sep 2015 | 0130 | 1 | Terra |
| 02 Oct 2015 | 0120 | 2 | Terra |
| 06 Oct 2015 | 1610 | 1 | Aqua |
| 08 Oct 2015 | 1660 | 1 | Aqua |
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Figure 10. MIROVA graph showing radiative power measured by satellite over Michael during April 2015 to April 2016, with a strong maximum on the last day of August 2015. Courtesy of MIROVA. |
Information Contacts: MIROVA, 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/)
This compilation of synonyms and subsidiary features may not be comprehensive. Features are organized into four major categories: Cones, Craters, Domes, and Thermal Features. Synonyms of features appear indented below the primary name. In some cases additional feature type, elevation, or location details are provided.
Cones |
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| Feature Name | Feature Type | Elevation | Latitude | Longitude |
| Ashen Hills | Cone | 57° 49' 29" S | 26° 27' 14" W | |
| Fin | Cone | -276 m | 58° 0' 0" S | 26° 45' 0" W |
| Humpback | Cone | -75 m | 57° 35' 21" S | 27° 3' 28" W |
|
Michael
Miguel |
Stratovolcano | 843 m | 57° 48' 0" S | 26° 29' 0" W |
| Minke | Cone | -480 m | 57° 24' 0" S | 26° 27' 45" W |
| Orca | Cone | -344 m | 57° 32' 0" S | 26° 47' 30" W |
| Southern Right | Cone | -400 m | 58° 5' 0" S | 27° 0' 0" W |
| West Minke | Cone | -1500 m | 57° 22' 45" S | 26° 42' 45" W |
Craters |
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| Feature Name | Feature Type | Elevation | Latitude | Longitude |
| Old Crater | Crater | |||
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Eruptive History
There is data available for 19 Holocene eruptive periods.
| Start Date | Stop Date | Eruption Certainty | VEI | Evidence | Activity Area or Unit |
|---|---|---|---|---|---|
| 2015 Aug 28 | 2015 Oct 8 | Confirmed | 0 | Historical Observations | |
| 2012 Jun 30 (?) | 2012 Nov 22 (?) | Confirmed | 0 | Historical Observations | |
| 2010 Nov 17 (?) | 2010 Nov 17 (?) | Confirmed | 1 | Historical Observations | Main crater |
| [ 2009 Nov 19 (?) ] | [ 2009 Nov 19 (?) ] | Uncertain | Old Crater | ||
| 2008 Oct 25 (?) | 2008 Oct 25 (?) | Confirmed | 0 | Historical Observations | |
| 2008 Jan 8 (?) | 2008 Jan 8 (?) | Confirmed | 0 | Historical Observations | Old Crater |
| 2006 Jun 9 (in or before) | 2006 Dec 6 (?) | Confirmed | 0 | Historical Observations | Old Crater |
| 2005 Oct 2 (?) | 2006 Jan 20 (?) | Confirmed | 0 | Historical Observations | |
| 2003 May 6 (?) | 2003 May 6 (?) | Confirmed | 0 | Historical Observations | |
| 2002 Jul 16 (?) ± 15 days | 2002 Nov 16 (?) ± 15 days | Confirmed | 0 | Historical Observations | |
| 2001 Sep 16 (?) ± 15 days | 2001 Nov 16 (?) ± 15 days | Confirmed | 0 | Historical Observations | |
| 2000 Aug 16 (?) ± 15 days | 2001 Jan 16 (?) ± 15 days | Confirmed | 0 | Historical Observations | |
| 1997 May 16 (?) ± 15 days | 1998 Feb 16 (in or after) ± 15 days | Confirmed | 0 | Historical Observations | |
| 1996 Oct 16 ± 15 days | Unknown | Confirmed | 0 | Historical Observations | |
| 1995 Oct 5 ± 4 days | 1996 Apr 16 ± 15 days | Confirmed | 0 | Historical Observations | |
| 1995 Apr 16 (?) ± 15 days | 1996 Jun 16 ± 15 days | Confirmed | 0 | Historical Observations | |
| 1900 ± 10 years | Unknown | Confirmed | 0 | Tephrochronology | North flank |
| [ 1823 ] | [ Unknown ] | Uncertain | 2 | ||
| 1819 Dec 29 | Unknown | Confirmed | 2 | Historical Observations |
Deformation History
There is no Deformation History data available for Saunders.
Emission History
There is no Emissions History data available for Saunders.
Photo Gallery
| Glacier-covered Mount Michael stratovolcano dominates Saunders Island. Cordelia Bay lies between the Blackstone Plain (top) and the snow-free Ashen Hills (right), a cluster of parasitic cones on the SE flank. Ash clouds were reported from the summit crater in 1819, and an effusive eruption was inferred to have occurred from a north-flank fissure around the turn of the 19th century. Recent AVHRR and MODIS satellite imagery has revealed evidence for lava lake activity in the summit crater of Mount Michael. ASTER satellite image, 2002 (National Aeronautical and Space Administration, courtesy of ASTER science team). |
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Smithsonian Sample Collections Database
There are no samples for Saunders in the Smithsonian's NMNH Department of Mineral Sciences Rock and Ore collection.
Affiliated Sites
| DECADE Data | The DECADE portal, still in the developmental stage, serves as an example of the proposed interoperability between The Smithsonian Institution's Global Volcanism Program, the MAGA Database, and the EarthChem Geochemical Portal. The Deep Earth Carbon Degassing (DECADE) initiative seeks to use new and established technologies to determine accurate global fluxes of volcanic CO2 to the atmosphere, but installing CO2 monitoring networks on 20 of the world's 150 most actively degassing volcanoes. The group uses related laboratory-based studies (direct gas sampling and analysis, melt inclusions) to provide new data for direct degassing of deep earth carbon to the atmosphere. |
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WOVOdat
Single Volcano View Temporal Evolution of Unrest Side by Side Volcanoes |
WOVOdat is a database of volcanic unrest; instrumentally and visually recorded changes in seismicity, ground deformation, gas emission, and other parameters from their normal baselines. It is sponsored by the World Organization of Volcano Observatories (WOVO) and presently hosted at the Earth Observatory of Singapore. |
| Large Eruptions of Saunders | Information about large Quaternary eruptions (VEI >= 4) is cataloged in the Large Magnitude Explosive Volcanic Eruptions (LaMEVE) database of the Volcano Global Risk Identification and Analysis Project (VOGRIPA). |
| MIROVA | Middle InfraRed Observation of Volcanic Activity (MIROVA) is a near real time volcanic hot-spot detection system based on the analysis of MODIS (Moderate Resolution Imaging Spectroradiometer) data. In particular, MIROVA uses the Middle InfraRed Radiation (MIR), measured over target volcanoes, in order to detect, locate and measure the heat radiation sourced from volcanic activity. |
| MODVOLC Thermal Alerts | Using infrared satellite Moderate Resolution Imaging Spectroradiometer (MODIS) data, scientists at the Hawai'i Institute of Geophysics and Planetology, University of Hawai'i, developed an automated system called MODVOLC to map thermal hot-spots in near real time. For each MODIS image, the algorithm automatically scans each 1 km pixel within it to check for high-temperature hot-spots. When one is found the date, time, location, and intensity are recorded. MODIS looks at every square km of the Earth every 48 hours, once during the day and once during the night, and the presence of two MODIS sensors in space allows at least four hot-spot observations every two days. Each day updated global maps are compiled to display the locations of all hot spots detected in the previous 24 hours. There is a drop-down list with volcano names which allow users to 'zoom-in' and examine the distribution of hot-spots at a variety of spatial scales. |
| EarthChem | EarthChem develops and maintains databases, software, and services that support the preservation, discovery, access and analysis of geochemical data, and facilitate their integration with the broad array of other available earth science parameters. EarthChem is operated by a joint team of disciplinary scientists, data scientists, data managers and information technology developers who are part of the NSF-funded data facility Integrated Earth Data Applications (IEDA). IEDA is a collaborative effort of EarthChem and the Marine Geoscience Data System (MGDS). |
