VOLCANO: Bulletin of the Global Volcanism Network Volume 34, Number 10, October 2009

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Bulletin of the Global Volcanism Network Volume 34, Number 10, October 2009
From: "Venzke, Ed" <VENZKEE@xxxxxx>
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Bulletin of the Global Volcanism Network
Volume 34, Number 10, August 2009
http://www.volcano.si.edu/

Gaua (Vanuatu) Eruptions during September-November 2009 cause ashfall
and evacuations
Tinakula (Santa Cruz Islands) Eruption suggested by satellite thermal
data and confirmed in the field
Ulawun (Papua New Guinea) Earthquake swarm followed by incandescence
in June 2008
Batu Tara (Indonesia) Frequent ash plumes through October 2009
Egon (Indonesia) Update on the 15 April 2008 eruption and April-May
2008 seismicity
Ibu (Indonesia) Ongoing dome growth during July-August 2009
Mayon (Philippines) Increased activity in mid-2009; November 2009 eruption
Cleveland (USA) Two explosive ash emissions in June and October 2009
Soufriere Hills (Monserrat) A lull during late 2008 and intermittent
high activity during late 2009
San Vicente (El Salvador) Landslide in November 2009 after heavy rains
Fernandina (Ecuador) Thermal and gas analyses of April 2009 eruption


Editors: Rick Wunderman, Edward Venzke, and Sally Kuhn Sennert
Volunteer Staff: Paul S. Berger, Russell Ross, Hugh Replogle, Catie
Carter, Ludmila Eichelberger, Robert Andrews,
Margo Morell, Jacquelyn Gluck, and Stephen Bentley



Gaua
Vanuatu, SW Pacific
14.27°S, 167.50°E; summit elev. 797 m
All times are local (= UTC + 11 hours)

An eruption on Gaua Island in September 2009 was described in a report
from the Vanuatu Geohazards unit (Vanuatu Department of Geology,
Mines, and Water Resources, DGMWR) sent by Esline Garaebiti on 16
November. A later government report and several news reports extended
into late November. According to the DGMWR, elevated volcanism in 1973
led to the evacuation of the entire island, which then was home to 600
people; Gaua Island now has more than 3,000 residents. News reports
cited no fatalities and by the end of November hundreds of evacuees
had moved to the safer E side of the island.

Gaua island, round in shape, is ~ 20 km in diameter and lies in the N
part of the archipelago (Banks Islands, Torba Province), ~ 100 km NE
of the closest parts of the island Espiritu Santo (figure 1). The
volcano is basaltic to andesitic in composition, and it contains a 6 x
9 km summit caldera that is ~ 700 m deep. Within the caldera sits
Mount Garat (Gharat), a prominent cone that supports the summit and
the crater complex that is the scene of the eruption. This caldera
contains a large, crescent-shaped lake (Lake Letas) (Thery and Thery,
1995).

Figure 1. Map of Vanuatu (formerly New Hebrides) showing major islands
and province names. On this map Gaua island is labeled with its other
name, Santa Maria. Inset shows Vanuatu with respect to other islands
in this portion of the South Pacific. Ambrym volcano, S of Gaua at the
E extent of Malampa province, sits on the island of the same name.
Courtesy of Relief Web and from an original map by the Central
Intelligence Agency.


Activity during September-October 2009. Toward the end of September
2009, the island's inhabitants reported both strong degassing from
Mount Garat's summit, gradual discoloration of the SW part of Lake
Letas, and the strong smell of sulphur in the villages on the W coast.
Mont Garat eruptions probably started on 27 September 2009.

Around noon on 29 September 2009 a group of young men hunting close to
the volcano witnessed a series of large explosions propelling an
umbrella-shaped column of ash up to a height of ~ 3 km. They also
noted a small pyroclastic flow limited to the W caldera. Due to
prevailing E wind on that day, minor ashfalls were reported on the W
part of Gaua. This explosive episode was also detected by the
satellite-borne ozone monitoring instrument (OMI ) in measurements of
sulfur dioxide (SO2) emissions the same day (figure 2).
Figure 2. SO2 emissions recorded over and around Gaua at 0224 UTC on
29 September 2009 corresponding to the eruptive activity seen in the
field. Note the higher, but normal, SO2 emission above Ambrym ~250 km
farther S. Courtesy of DGMWR, with data provided by the OMI website.

During 2-8 October 2009 a DGMWR team visiting the volcano found
elevated SO2. They recorded an average flux of ~ 3,000 tons/day. They
also noted an increase of the discolored area in Lake Letas (figures 3
and 4). Vegetation on NW part of the volcanic edifice, present in
2007, had been burned by acidic gases released from the volcano
(figure 5). The team indicated that gas emissions had begun days to
weeks earlier to cause such damage.

Figure 3. Continuous degassing from the summit crater of Gaua. There
are at least three active vents in the crater, one of which released a
combination ash and gas. Photo taken 6 October 2009, courtesy S.
Wallez.

Figure 4. Strong discoloration was present at Gaua in the SW part of
Lake Letas in 2003 (inset) and in 2009 (background). The 2003 photo
showed discoloration with shades of green to pale yellow. The 2009
photo showed intense red-orange discoloration. Photos courtesy DGMWR
(2003) and S. Wallez (2009).

Figure 5. Views of Gaua's NW flank taken in the year 2007 and in
November 2009, highlighting the almost complete loss of green
vegetation. Photos courtesy of P. Bani, Research Institute for
Development (IRD).

The team installed a seismic station on 2 October 2009 to help track
the volcanic activity. Many explosions were recorded during 10-11
October (figure 6), and on 13 October the seismic signals suggested
strong volcanism as well as continuous degassing. Consequently the
Alert Level was raised to 2 (on a scale of 0-4), advising the
population not to venture close to the volcano and to stay out of
potential drainages that might serve as flow paths.

Figure 6. Seismic record from the Gaua seismic station illustrating
that many explosions occurred between 1200 on 10 October 2009 and 1200
on 11 October 2009. Courtesy of DGMWR.

Activity during November 2009. From the end of October to around 4
November, witnesses noted explosions with strong ash emissions (figure
7). A substantial ash plume, both reported by observers and confirmed
by seismic recording, occurred on 31 October 2009. This was followed
by ashfall in the NW part of the island, where 53 inhabitants were
relocated to safer areas.

Figure 7. Plumes released at Gaua on 3 November 2009. All three active
vents emitted plumes, one a vigorous ash plume. Photo courtesy of
Sylvain Todman, DGMWR.

Gaua Bulletin No. 3 from DGMWR, dated 24 November 2009, reported a
large explosion around 1400 on 18 November. The explosion produced
very dense and high ash columns that blew W. The ash plumes from the
31 October and 18 November events photographed from the airport but
were apparently not assessed for plume heights. Activity remained
significant through at least 24 November. DGMWR recommended alert
level 2 and noted the persisting danger of ashfalls and mudflows.

News media reports and other data. Radio Australia News reported on 2
October 2009 that the last time the hazard concern was so high was in
1974 when volcanism led to inhabitants evacuated from the island for
months. According to Radio Australia Net in an interview with Charles
Bice (one of the Gaua Island community headmen), the early explosions
had been heard by both residents and pilots on Air Vanuatu flights.
During September-October, residents also found ash on their cabbage
crops.

A 26 November AFP report indicated that the Red Cross was dispensing
containers and water purification tablets. It said the public had
suffered respiratory problems and diaharrea. Rural water supplies
often come from surface water, or from rainwater collected from areas
such as roofs, and then stored in open drums or cisterns. These
sources are often vulnerable to contamination from ashfall.

A Vanuatu newspaper article by Len Garae printed after 18 November
noted that by then the first phase of evacuation, aided by three
ships, had taken ~ 159 villagers from the high-risk zone on the W side
of the island to the E side of the island. The article stated that a
larger eruption would mean evacuation of an additional 200 villagers
on the island's W shoreline. An even more vigorous eruption would
require inter-island ships to move residents to other islands.

A Vanuatu news article emphasized three new explosion on 26 November
and one on 27 November. It said that the additional villagers on the W
side of the island were in the process of evacuating. Although yet to
be confirmed elsewhere, the article said "the entire village of
'Waterfall' was destroyed by landslides."

MODIS thermal alerts were absent during the 2009 eruption.

A video shot in January 2003 from a low-flying helicopter showed
fumarolic plumes rising from the summit craters. The video is
available on YouTube from Geoff Mackley
(http://www.youtube.com/user/geoffmackley).

Reference: Thery, L., and Thery, J., 1995, Bathymetrie du lac Letas
lle de GAUA (Banks) (Vanuatu), Port-Vila, Vanuatu: Institut Francais
de Recherche Scientifique pour le Developpement en Cooperation, 1995.
17 p. : ill., maps; 28 cm. Series-Sciences de la terre
geologie-geophysique ; no. 10 (in French and English)

Geologic Summary. The roughly 20-km-diameter Gaua Island, also known
as Santa Maria, consists of a basaltic-to-andesitic stratovolcano with
an 6 x 9 km wide summit caldera. Small parasitic vents near the
caldera rim fed Pleistocene lava flows that reached the coast on
several sides of the island; several littoral cones were formed where
these lava flows reached the sea. Quiet collapse that formed the
roughly 700-m-deep caldera was followed by extensive ash eruptions.
Construction of the historically active cone of Mount Garat (Gharat)
and other small cinder cones in the SW part of the caldera has left a
crescent-shaped caldera lake. The symmetrical, flat-topped Mount Garat
cone is topped by three pit craters. The onset of eruptive activity
from a vent high on the SE flank of Mount Garat in 1962 ended a long
period of dormancy.

Information Contacts: E. Garaebiti, S. Todman, C. Haruel, D. Charley,
D. Nakedau, J. Cevuard, and A. Worwor, Department of Geology, Mines
and Water Resources (DGMWR), Geohazards Unit, Vanuatu (URL:
http://www.geohazards.gov.vu/); P. Bani, Institut de recherche pour la
developpment (IRD), Noumea, New Caledonia (URL: http://www.ird.nc/);
OMI (Ozone Monitoring Instrument) Sulfur Dioxide Group, Joint Center
for Earth Systems Technology, University of Maryland Baltimore County
(UMBC), 1000 Hilltop Circle, Baltimore, MD 21250, USA
(http://so2.umbc.edu/omi/); Relief Web (URL: http://www.reliefweb.in);
Agence France-Press (AFP) (URL: http://www.afp.com/); Radio Australia
News (URL: http://www.radioaustralianews.net.au); The
Independent/L'Indepednant, Vanuatu (URL: http://www.independent.vu/);
Geoff Mackley, PO Box 12926, Penrose, Auckland 1135, New Zealand
(http://www.youtube.com/user/geoffmackley,
http://www.geoffmackley.com/).



Tinakula
Santa Cruz Islands, SW Pacific
10.38°S, 165.80°E; summit elev. 851 m
All times are local (= UTC + 11 hours)

MODIS/MODVOLC satellite thermal alerts data for Tinakula (table 1)
suggests continuing eruptive activity during the period mid-June 2007
through early December 2009; however, these data lack validation by
field observations. Similar intermittent alerts have been detected
since mid-February 2005 (BGVN 31:03, 32:03, and 32:07).

Table 1. MODIS/MODVOLC satellite thermal alerts measured at Tinakula
during the period mid-June 2007 through early December 2009 (continued
from table in BGVN 32:07). Note particularly the number of alerts
recorded at 0230 on 15 February 2009 (5 pixels), indicating a possible
eruption resulting in thermal anomalies covering an area of 5 to 7.5
km2. Courtesy of the Hawai'i Institute of Geophysics and Planetology
(HIGP) Thermal Alerts System.

   Date           Time     Pixels    Satellite
                  (UTC)

   24 Sep 2007    1140       2         Terra
   19 Oct 2007    1430       1         Aqua
   09 Nov 2007    1150       1         Terra
   19 Sep 2008    1130       1         Terra
   26 Sep 2008    1140       1         Terra
   04 Nov 2008    1145       1         Terra
   29 Nov 2009    1440       2         Aqua
   15 Feb 2009    0230       5         Aqua
   04 May 2009    1205       1         Terra
   12 Aug 2009    1140       1         Terra
   14 Aug 2009    1125       1         Terra

A possible observation of eruptive activity was found on a website by
Clark Berge dated 22 September 2009: "A tall plume of steam and smoke
streams from the top of a majestic cone rising direct from the sea....
During my visit to Temotu Province last week ... we circled [Tinakula
in a motorized canoe], which seemed lush and harmless until we rounded
a point and saw the steep black face of stone. Boulders were detaching
themselves and bounding down the cliff amid a shower of sparks. I
quickly realized the stones were glowing red!"

Geologic Summary. The small 3.5-km-wide island of Tinakula is the
exposed summit of a massive stratovolcano that rises 3-4 km from the
sea floor at the NW end of the Santa Cruz islands. Tinakula resembles
Stromboli volcano in containing a breached summit crater that extends
from the 851-m-high summit to below sea level. Landslides enlarged
this scarp in 1965, creating an embayment on the NW coast. The
satellitic cone of Mendana is located on the SE side. The dominantly
andesitic Tinakula volcano has frequently been observed in eruption
since the era of Spanish exploration began in 1595. In about 1840, an
explosive eruption apparently produced pyroclastic flows that swept
all sides of the island, killing its inhabitants. Frequent historical
eruptions have originated from a cone constructed within the large
breached crater. These have left the upper flanks of the volcano and
the steep apron of lava flows and volcaniclastic debris within the
breach unvegetated.

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://hotspot.higp.hawaii.edu/); Clark Berge (URL:
http://brclarkberge.blogspot.com/2009/09/tinakula-volcanoe.html).



Ulawun
New Britain, Papua New Guinea
5.05°S, 151.33°E; summit elev. 2,334 m

Aactivity at Ulawun since early 2007 has consisted primarily of
low-frequency earthquakes and white vapor emissions, with ash reported
on 1 May and 25 December 2007 (BGVN 33:03). No additional activity was
reported by the Rabaul Volcano Observatory (RVO) until a seismic swarm
preceded observations of glow on 13-14 June 2008. Incandescence was
seen again in mid-May 2009.

RVO reported that increased seismic activity at Ulawun consisting of
high-frequency volcano-tectonic (VT) earthquakes began on 7 June 2008.
After peaking at 22 events on 12 June, the daily totals dropped and
fluctuated between one and seven events per day, although totals of
14-15 events occurred on 14, 29, and 30 June. Some of the VT
earthquakes were felt, including three on 30 June. Low-frequency
earthquakes continued to occur as well, but remained within background
levels; daily totals were between 257 and 775.

Summit activity was very low and consisted of variable amounts of
white vapor. Bluish vapor was observed on some days during 16-21 June.
Other reported activity included low roaring noises on 1, 2, 12, and
14 June, and summit glow on the 13th and 14th. On 22 June noises heard
in villages to the NE accompanied some of the earthquakes. On 28 June
an earthquake accompanied by a booming noise was felt in nearby areas.
White vapor plumes were emitted during 2-6 July, and occasional
roaring noises were reported during 1-3 July.

Additional reports by RVO in February and April 2009 noted that the
volcano remained quiet, only releasing white vapor, with no reports of
glow at night. Seismicity was moderate to low in February until power
problems disabled the instrument. The number of seismic events that
month fluctuated between 400 and 950 before declining to a range of
250-300 during 20-24 February. Low-frequency events dominated the
record, although some high-frequency activity was recorded at a daily
rate of 1-6 events.

Ulawun remained quiet throughout September and October 2009. Summit
activity was dominated by weak to moderate volumes of white vapor, and
seismicity was generally low. During September, daily totals for
high-frequency volcano-tectonic events ranged between 0 and 7, and
low-frequency earthquakes were registered at a rate of 167-547. For
the month of October, daily totals for high-frequency volcano-tectonic
events were as high as 11, and the number of low-frequency earthquakes
ranged between 74 and 404.

Geologic Summary. The symmetrical basaltic-to-andesitic Ulawun
stratovolcano is the highest volcano of the Bismarck arc, and one of
Papua New Guinea's most frequently active. Ulawun volcano, also known
as the North Son, rises above the north coast of the island of New
Britain across a low saddle NE of Bamus volcano, the South Son. The
upper 1000 m of the 2334-m-high Ulawun volcano is unvegetated. A
prominent E-W-trending escarpment on the south may be the result of
large-scale slumping. Satellitic cones occupy the NW and eastern
flanks. A steep-walled valley cuts the NW side of Ulawun volcano, and
a flank lava-flow complex lies to the south of this valley. Historical
eruptions date back to the beginning of the 18th century.
Twentieth-century eruptions were mildly explosive until 1967, but
after 1970 several larger eruptions produced lava flows and basaltic
pyroclastic flows, greatly modifying the summit crater.

Information Contacts: Ima Itikarai, Rabaul Volcano Observatory (RVO),
P.O. Box 386, Rabaul, Papua New Guinea (Email: hguria@xxxxxxxxxxxxx).



Batu Tara
Lesser Sunda Islands, Indonesia
7.792°S, 123.579°E; summit elev. 748 m

Batu Tara has been active since January 2007, with thermal anomalies
and occasional low-level ash plumes at least through 24 November 2009.
This report discusses activity since our previous report (BGVN 34:01),
which covered activity through 10 March 2009.

Since 10 March 2009, the eruption of low-level ash plumes has
continued at least through 24 November 2009. Many reports of Batu Tara
plumes came from the Darwin Volcanic Ash Advisory Centre (table 2).

Table 2. Summary of Volcanic Ash Advisories for Batu Tara reported by
the Darwin Volcanic Ash Advisory Centre (VAAC) during 11 March 2009-24
November 2009. Many of these plumes were described as ash plumes. This
table continues the table in BGVN 34:01. Courtesy of the Darwin VAAC.

   Date (2009)               Plume top      Plume drift direction(s)
                           altitude (km)    and extent

   11 Mar                        2.1        N, NW
   20 Mar                        2.4        NW
   25-27 Mar                     2.1        ~30-110 km NW
   05-06 Apr                     2.4        40-210 km W
   11-12, 14 Apr             1.8-2.4        35-90 km W, NW
   15-16 Apr                 1.8-2.4        35-75 km W, NW
   24-25, 28 Apr                 3.0        Up to 110 km in variable directions
   29-30 Apr, 03-04 May      2.4-3.0        45-185 km W, NW
   05 May                        2.4        55 W
   14-19 May                     3.0        35-75 km W, NW, N
   20 May                        3.0        65 km NW
   26 May                        2.4        55 km NW
   27 May-02 Jun                 2.4        25-75 km NW, W, SW
   03-08 Jun                     2.4        40-75 km NW, W, SW
   09 Jun                        --         140 km W
   10-16 Jun                 1.5-2.4        25-185 km SW, NW, N, NE
   25-30 Jun                     1.5        35-130 km SW, W, NW
   01-07 Jul                 1.5-2.4        35-110 km W, NW, N.
   08 Jul                        2.4        55 km W, NW
   12-14 Jul                     1.5        25-55 km W, NW, and N.
   15-18 Jul                     1.5        20-55 km in multiple directions
   23 Jul                        2.4        55 km W
   27-28 Jul                     1.5        Up to 150 km NW
   29-31 Jul                     1.5        Up to 37 km NW, N
   04-07 Aug                 1.5-2.1        45-90 km W, NW, N
   12-13, 15-17 Aug          1.5-3.0        5-110 km W, NW, N
   19, 21-25 Aug                 1.5        35-150 km W, WNW, NW
   26 Aug-01 Sep             1.5-2.4        15-55 km W, NW, N
   02-08 Sep                     1.5        10-55 km W, NW
   09-11, 14-15 Sep              1.5        25-45 km W, NW
   16-19, 21-22 Sep              1.5        20-65 km W, NW, N, NE
   23-29 Sep                 1.5-2.4        15-75 km W, NW
   30 Sep-03, 05-06 Oct          2.4        25-75 km W, NW, N
   06 Oct                        2.4        65 km W
   14-16 Oct                     1.8        25-185 km W, N
   27 Oct                        2.1        65 km W, NW
   24 Nov                        2.4        90 km NW

NASA's Earth Observatory described the scene from an image taken on 30
April 2009 (figure 8). "In this true-color picture, Batu Tara looks
like a small, smoking speck in the Flores Sea. Initially blowing
toward the NW, the volcanic plume changes direction multiple times,
forming a large question-mark shape, mingling with clouds in the N.
When volcanic gases mingle with oxygen and moisture in the presence of
sunlight, vog, or volcanic smog, often results. The off-white color
and diffuse shape of the volcanic plume in the N are suggestive of
vog." MODVOLC recorded thermal alerts at Batu Tara on 26 and 29 May,
and 3 July 2009.

Figure 8. Image of plume from Batu Tara taken on 30 April 2009 by the
Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA's Terra
satellite. Plume extends W and NW. Courtesy NASA Earth Observatory.

Geologic Summary. The small isolated island of Batu Tara in the Flores
Sea about 50 km N of Lembata (fomerly Lomblen) Island contains a scarp
on the E side similar to the Sciara del Fuoco of Italy's Stromboli
volcano. Vegetation covers the flanks of Batu Tara to within 50 m of
the 748-m-high summit. Batu Tara lies N of the main volcanic arc and
is noted for its potassic leucite-bearing basanitic and tephritic
rocks. The first historical eruption from Batu Tara, during 1847-52,
produced explosions and a lava flow.

Information Contacts: Darwin Volcanic Ash Advisory Centre (VAAC),
Bureau of Meteorology, Northern Territory Regional Office, PO Box
40050, Casuarina, NT 0811, Australia (URL:
http://www.bom.gov.au/info/vaac/); NASA Earth Observatory (URL:
http://earthobservatory.nasa.gov/); Hawai'i Institute of Geophysics
and Planetology (HIGP) Thermal Alerts System, School of Ocean and
Earth Science and Technology (SOEST), University of Hawai'i, 2525
Correa Road, Honolulu, HI 96822, USA (URL:
http://hotspot.higp.hawaii.edu/).



Egon
Lesser Sunda Islands, Indonesia
8.67°S, 122.45°E; summit elev. 1,703 m
All times are local (= UTC + 8 hours)

 Since the eruption of 28 January 2004, Egon has frequently undergone
phreatic eruptions without any significant increase in volcanic tremor
or earthquakes. Our last report on Egon (BGVN 33:08) summarized the
gradual decline of activity during April-May 2008. This report
overlaps with the earlier one but benefits from better report
translation. The closest large city to Egon is Maumere (Flores), ~ 25
km WNW.

The Center of Volcanology and Geological Hazard Mitigation (CVGHM)
provided additional information on the April-May 2008 disturbances
(BGVN 33:08). A spike in the volcano's activity took place on 6-7
April 2008 (table 3). Reports noted a subsequent decrease in earth
movements. On 4-15 April 2008 thin white smoke was seen rising ~ 25-50
m above the crater. This emission was considered a daily activity;
however seismicity became evident.

Table 3. Seismicity and observations of activity at Egon during 5-28
April 2009. "--" indicates no data reported. Courtesy of CVGHM.

   Date           Deep Volcanic       Shallow Volcanic    Tremor Duration
                  Earthquakes (VA)    Earthquakes (VB)      (seconds)

       Observations

   05 Apr 2008          3                   0                   --
       Usual daily occurrence of hot air blasts and whitish smoke
   06 Apr 2008         38                  93                   --
       Hot air blasts and "whitish smoke," rising 25-50 m
   07 Apr 2008         15                   2                   --
       Hot air blasts and "whitish smoke," rising ~35 m
   08-14 Apr 2008       6                   3                   --
       Hot air blasts and "whitish smoke," rising ~25 m above the crater and
       a significant decrease in volcanic quakes
   15 Apr 2008         --                  --                 1290 s
       Ash plume to 4,000 m height
   20 Apr 2008         --                  --                 1073.5 s
       Ash plume to 2,000 m height
   24 Apr 2008         --                  --                   91 s
       Ash plume to 850 m height
   28 Apr 2008         --                  --                   60.5 s
       Ash plume to 75 m height

On 15 April 2008 a phreatic eruption occurred and CVGHM raised the
Alert Level to 3 ("Saga" - on a scale of 1-4). Visual observations
indicated that the ash column rose ~ 4,000 m above the crater; however
the ash was not identifiable from satellite survey due to cloud cover.
The eruption was accompanied by a "grumbling" sound. An ash/cinder
cloud reached the city of Maumere (Flores), ~ 20 km WNW. Because of
the height of eruptive plume, authorities at Waioti Airport serving
Maumere were alerted. The emergency response team, together with the
district government of Sikka (Flores) onsite at the villages closest
to the eruption, reported that ~ 600 persons from local villages
evacuated; they reported no fatalities.

The Darwin Volcanic Ash Advisory Center (VAAC) issued two alerts of
the volcanic activity at Egon, on 15 and 16 April 2008. Between 15
April and 11 May 2008, four explosive tremor events were recorded
(table 3). Land deformation in the vicinity of the volcano stabilized
after 27 April 2008.

During 15 April-10 May 2008, 1-2 deep volcanic earthquakes occurred
daily. Between 25 April to 10 May, shallow volcanic earthquakes
decreased from 6-20 daily to 1-10 daily. During that time, tremors
caused by hot air blasts continued to be recorded, reaching a rather
high total range of around 6-47 events per day. The higher values are
comparatively large; a normal stasis condition is considered to be a ~
1-9 hot air blast signals per day. On 12 May 2008, hot air tremors had
amplitudes of 2 mm and durations of 5-11 seconds. Whitish smoke could
frequently be seen reaching a height of only 10 m above the peak. On
13 May, CVGHM downgraded the hazard status to Alert Level 2 (Waspada).

For the rest of May 2008 and for more than a year, Egon's was
relatively quiet. From 4 March to 12 July 2009, type-A earthquakes
were recorded at a rate of 1-2 events per day; type-B earthquakes, 1-3
events per day; (except on 6 May when six were recorded). During that
interval there were 1-9 hot air blast earthquakes per day and the hot
air blasts of smoke were generally whitish in color and were rose to ~
10 m over the peak. Eruptive earthquakes were absent. Although tremor
was still recorded (with an amplitude of 0.5-4 mm), since 4 March
2009, earth movements have decreased. On 17 July 2009, the CGVHM.
downgraded the hazard status to Alert Level 1 (Normal).

MODVOLC review of activity shows no thermal indicators of volcanic activity.

Geologic Summary. Gunung Egon volcano sits astride the narrow waist of
eastern Flores Island. The barren, sparsely vegetated summit region
has a 350-m-wide, 200-m-deep crater that sometimes contains a lake.
Other small crater lakes occur on the flanks of the 1703-m-high
volcano, which is also known as Namang. A lava dome forms the southern
1671-m-high summit. Solfataric activity occurs on the crater wall and
rim and on the upper southern flank. Reports of historical eruptive
activity prior to explosive eruptions beginning in 2004 were
inconclusive. A column of "smoke" was often observed above the summit
during 1888-1891 and in 1892. Strong "smoke" emission in 1907 reported
by Sapper (1917) was considered by the Catalog of Active Volcanoes of
the World (Neumann van Padang, 1951) to be a historical eruption, but
Kemmerling (1929) noted that this was likely confused with an eruption
on the same date and time from Lewotobi Lakilaki volcano.

Information Contacts: Center of Volcanology and Geological Hazard
Mitigation, Saut Simatupang, 57, Bandung 40122, Indonesia (URL:
http://portal.vsi.esdm.go.id/joomla/); Hawai'i Institute of Geophysics
and Planetology (HIGP) Thermal Alerts System, School of Ocean and
Earth Science and Technology (SOEST), University of Hawai'i, 2525
Correa Road, Honolulu, HI 96822, USA (URL:
http://hotspot.higp.hawaii.edu/).



Ibu
Halmahera, Indonesia
1.488°N, 127.63°E; summit elev. 1,325 m
All times are local (= UTC + 9 hours)

Thermal anomalies detected by satellites (MODVOLC thermal alerts)
through June 2009 suggested continued growth of a lava dome in the
crater (BGVN 34:05). The Center of Volcanology and Geological Hazard
Mitigation (CVGHM) reported that prior to 11 July 2009, white and gray
plumes from Ibu rose ~ 600 m above the crater rim. After 11 July, the
plumes were gray and rose only ~ 400 m above the crater rim. Ash from
the gray plumes fell on areas within a 3-km radius of Ibu.

Observers noted an increase of eruptive activity after mid-July.
During the period 27 July to 3 August, the total number of eruptive
events showed a tendency to increase. Each eruptive earthquake was
then followed by the expulsion of lava that reached the upper slopes.
Plumes seen during 15 July to 4 August 2009 were grayish-white and
reached a height of ~ 300-400 m above the crater rim. The lava
extrusions accompanied rather strong rumbling noises on five
occasions. The incandescent material was seen coming from the summit
on 2 August 2009, and lava flows were seen. Later that day, a
thunderous sound was followed by incandescence at the summit.

On 3 August, incandescent material was ejected as high as 20 m above
the crater. The total of explosion earthquakes increased from the
20-49 events of mid-July to 50-80 events during 27 July to 4 August.
Villagers in Desa Duono, Going, and Sanghaji noted strong rumbling
sounds. No volcanic earthquakes were recorded during that time frame.
On 4 August 2009, 82 volcanic earthquakes were recorded. Each eruptive
earthquake was followed by the expulsion of lava which reached the
upper slopes.

The observation post in the village of Duono, 5 km NW of Ibu, reported
that the lava dome continued to grow. As a result, local residents
were advised to prepare for times when they needed to wear masks that
cover both the nose and the mouth. Visitors and tourists were asked to
remain at least 2 km from the crater.

Geologic Summary. The truncated summit of Gunung Ibu stratovolcano
along the NW coast of Halmahera Island has large nested summit
craters. The inner crater, 1 km wide and 400 m deep, contained several
small crater lakes through much of historical time. The outer crater,
1.2 km wide, is breached on the north side, creating a steep-walled
valley. A large parasitic cone is located ENE of the summit. A smaller
one to the WSW has fed a lava flow down the western flank. A group of
maars is located below the northern and western flanks of the volcano.
Only a few eruptions have been recorded from Ibu in historical time,
the first a small explosive eruption from the summit crater in 1911.
An eruption producing a lava dome that eventually covered much of the
floor of the inner summit crater began in December 1998.

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



Mayon
Luzon, Philippines
13.257°N, 123.685°E; summit elev. 2,462 m
All times are local (= UTC + 8 hours)

On 10 August 2008 an explosion and resulting ash plume followed weeks
of increased activity and summit incandescence (BGVN 34:02). According
to a Philippine Information Agency (PIA) Daily News Reader press
release, the 10 August eruption was followed by an M 5.8 earthquake on
15 August and a series of aftershocks that continued through at least
20 August.

On 10 July 2009, the Philippine Institute of Volcanology and
Seismology (PHIVOLCS) noted increased activity beginning in June 2009.
According to PHIVOLCS, there was a rise in low-frequency volcanic
earthquakes, a ground uplift of ~ 1 cm, moderate steam emissions, and
summit incandescence. An 8 July overflight discovered the crater
contained a "cone-shaped pile of hot, steaming old rocks." The fresh
deposits were possibly from a previous eruption, and may have been the
source of the glow in the crater. The Alert Level for Mayon was raised
from 1 (low level unrest) to 2 (unrest which could lead to more ash
explosions or eventually to hazardous magmatic eruptions).

According to a 6 August 2009 article from the Philippine Daily
Inquirer, resident PHIVOLCS volcanologist Eduardo Laguerta reported
that the number of earthquakes at Mayon had decreased by early August
2009. However, the Inquirer reported that SO2 emissions had increased,
with a maximum of 1,977 tons per day on 6 August, compared to 500 tons
per day when there is no activity.

PHIVOLCS reported that 11 earthquakes were detected during 14-15
September, with steam plumes drifting NW and ENE. On 15 September,
three ash explosions produced a brownish ash plume that rose 700 m
above the crater and drifted SW. On 28 October a minor explosion
produced a brownish ash plume that rose 600 m above the crater and
drifted NE, preceded by 13 volcanic earthquakes over the previous
24-hour period.

On 11 November 2009 another ash eruption occurred at 0158 that lasted
for ~ 3 minutes and ejected incandescent rock fragments seen from
nearby villages. The explosion was accompanied by rumbling sounds and
light ashfall in surrounding areas to the SW, W, and NW. According to
the Inquirer, a second explosion was recorded at 0702, with an ash
plume reaching 300 m above the crater. The Inquirer reported that
residents in Daraga township to the S were ordered to evacuate early,
but that further mass evacuations would not be ordered until the Alert
Level was raised to Level 3. An aviation ash advisory from the Tokyo
VAAC noted continuous ash erupting in MTSAT-IR satellite imagery at
0800 on 11 November.

A 21 November 2009 article from Vox Bikol confirmed that as of 17
November, Mayon continued to exhibit summit incandescence and emit
fluctuating amounts of SO2. Due to the continuing unrest PHIVOLCS
installed additional seismic monitoring equipment, including three
sets of broadband instruments from the Japan International Cooperating
Agency (JICA).

A news article from Vox Bikol stated that PHIVOLCS did not observe
summit incandescence during 2-3 December due to heavy cloud cover, but
as of 4 December 2009 ground deformation and moderate steam emissions
were continuing. PHIVOLCS continued to enforce the 6-km-radius
Permanent Danger Zone (PDZ) and the 7-km-radius Extended Danger Zone
(EDZ) on the SE flank, and urged residents to avoid river channels
that are prone to lahars.

Geologic Summary. Beautifully symmetrical Mayon volcano, which rises
to 2,462 m above the Albay Gulf, is the Philippines' most active
volcano. The structurally simple volcano has steep upper slopes
averaging 35-40 degrees that are capped by a small summit crater. The
historical eruptions of this basaltic-andesitic volcano date back to
1616 and range from strombolian to basaltic plinian, with cyclical
activity beginning with basaltic eruptions, followed by longer term
andesitic lava flows. Eruptions occur predominately from the central
conduit and have also produced lava flows that travel far down the
flanks. Pyroclastic flows and mudflows have commonly swept down many
of the approximately 40 ravines that radiate from the summit and have
often devastated populated lowland areas. Mayon's most violent
eruption, in 1814, killed more than 1,200 people and devastated
several towns.

Information Contacts: Philippine Institute of Volcanology and
Seismology (PHIVOLCS), University of the Philippines Campus, Diliman,
Quezon City, Philippines (URL: http://www.phivolcs.dost.gov.ph/);
Philippine Daily Inquirer, (URL: http://www.inquirer.net/); Tokyo
Volcanic Ash Advisory Center (VAAC), Tokyo, Japan (URL:
http://ds.data.jma.go.jp/svd/vaac/data/); Vox Bikol (URL:
http://www.voxbikol.com/); Philippine Information Agency (URL:
http://www.pia.gov.ph/).



Cleveland
Aleutian Islands, United States
52.825°N, 169.944°W; summit elev. 1,730 m

As previously reported (BGVN 33:11) , the Alaska Volcano Observatory
(AVO) had raised the aviation color code for Cleveland on 24 December
2008 to Yellow and the alert level to Advisory, following a thermal
anomaly near the summit that was present for two days. The anomaly was
occasionally observed into early January 2009. On 2 January, a
short-lived ash explosion produced an ash plume that rose ~ 6 km and
drifted ~ 240 km ESE before dissipating.

A small explosive eruption on 25 June 2009 sent an ash cloud rose to
an estimated altitude of 4.6 km, which quickly detached from the
volcano and drifted S. Another small and brief explosive eruption
occurred on 2 October. A small detached ash cloud rose to maximum
altitudes of 4.6-6.1 km and drifted ~ 600 km NE, dispersing over the
Bering Sea. No further activity was detected through  19 October, so
the Alert Levels were lowered to "Unassigned." Cleveland is not
monitored by a real-time seismic network, thus the levels "Green" or
"Normal" do not apply because background activity is not defined.

Geologic Summary. Beautifully symmetrical Mount Cleveland
stratovolcano is situated at the western end of the uninhabited,
dumbbell-shaped Chuginadak Island. It lies SE across Carlisle Pass
strait from Carlisle volcano and NE across Chuginadak Pass strait from
Herbert volcano. Cleveland is joined to the rest of Chuginadak Island
by a low isthmus. The 1,730-m-high Mount Cleveland is the highest of
the Islands of the Four Mountains group and is one of the most active
of the Aleutian Islands. The native name for Mount Cleveland,
Chuginadak, refers to the Aleut goddess of fire, who was thought to
reside on the volcano. Numerous large lava flows descend the
steep-sided flanks of the volcano. It is possible that some
18th-to-19th century eruptions attributed to Carlisle should be
ascribed to Cleveland (Miller et al., 1998). In 1944 Cleveland
produced the only known fatality from an Aleutian eruption. Recent
eruptions from Mount Cleveland have been characterized by short-lived
explosive ash emissions, at times accompanied by lava fountaining and
lava flows down the flanks.

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, P.O. Box 757320,
Fairbanks, AK 99775-7320, USA (Email: eisch@xxxxxxxxxxxxxxxxxx), and
the Alaska Division of Geological and Geophysical Surveys, 794
University Ave., Suite 200, Fairbanks, AK 99709, USA (Email:
cnye@xxxxxxxxxxxxxxxxx).



Soufriere Hills
Montserrat, West Indies
16.72°N, 62.18°W; summit elev. 915 m

Dome collapse at Soufriere Hills (figure 9) and an eruption on 28 July
2008 was followed by dome regrowth (BGVN 33:10). During October
through 4 December 2008, low-level activity included occasional
earthquakes and explosion, lahars, and small pyroclastic flows. The
current report describes activity from 5 December 2008 through 10
December 2009, primarily based on information provided by the
Montserrat Volcano Observatory (MVO). Activity was intermittent during
2009 (table 4), with high-level activity resuming in November and
continuing through at least 11 December.

Figure 9. Visible satellite imagery showing Soufriere Hills and the
southern part of Montserrat on 24 June 2006. Courtesy of Google Earth,
with data provided by Europa Technologies and DigitalGlobe.

Table 4. Ash plumes or plumes that may have contained ash from
Soufriere Hills between 5 December 2008 and 2 December 2009. Courtesy
Washington Volcanic Ash Advisory Center (VAAC), based on analysis of
satellite imagery, information from MVO, and pilot reports.

   Date              Ash plume height,            Remarks
                     flow direction

   13 Dec 2008       4.6-5.2 km
   14 Dec 2008       1.8 km, W
   15 Dec 2008       2.4-3 km, SW
   16 Dec 2008       S                            Thermal anomaly
   19-23 Dec 2008    4.3 km, various              Thermal anomalies on
19 and 21 Dec
   24 Dec 2008       3 km                         Caused by pyroclastic flow
   26-30 Dec 2008    2.1-4.9 km,                  Thermal anomalies on 27 Dec
                       various (28 and 30 Dec)    Thermal anomaly
   03 Jan 2009       2.4-10.7 km, various
   04 Jan 2009       W, WSW
   25 Feb 2009       W                            Caused by pyroclastic flow
   06 Apr 2009       2.7-4.9 km, NW
   24 May 2009       --                           Caused by pyroclastic flow
   04-06 Oct 2009    3.4-5.5 km, W, WNW
   23-25 Oct 2009    W                            Caused by pyroclastic flows
   24 Nov 2009       6.1 km                       Caused by pyroclastic flows
   02 Dec 2009       4.6-6.1 km                   Caused by pyroclastic flows

Activity during December 2008. Subsequent to the four explosions
between 2-5 December 2008, the MVO reported that seismicity from the
lava dome remained elevated. The volcano continued to inflate and
discharge lava and ash during December 2008. Frequent pulses of ash
rose from multiple places on the NW face of the lava dome and from a
low on the dome behind Gages Mountain (as seen from Salem). A series
of pyroclastic flows and rockfalls descended the Gages Valley and
other valleys during December 2008, at least two reaching Plymouth (~
5 km W). Significant lava dome growth on the SW flank was observed.
Photographs showed that most of the growth had taken place since 8
December; lava was filling in the area between the lava dome and
Chance's Peak. Initial calculations suggested that the dome grew at a
rate of 1 m^3/s during this time.

During the last two weeks of December 2008, the lava dome was
characterized by increased lava extrusion, rockfalls, and pyroclastic
flows. Lava extrusion on the N, W, and SW sides of the dome continued
and incandescence on the dome was visible at night when weather was
favorable. On 22 December, the Hazard Level was increased to 4 (on a
scale 1-5) due to the repeated occurrences of pyroclastic flows in the
lower part of Tyers Ghaut.

On 24 December, a large pyroclastic flow that reached Plymouth, and
possibly the sea, generated an ash plume that rose to an altitude of 3
km. Ashfall was reported in areas 6-7 km NW. Large incandescent
blocks, deposited by rockfalls and pyroclastic flows, were visible on
multiple occasions at night in the lower parts of Tyers Ghaut. Fires
triggered by surges were visible in the neighboring valley.

Activity during January-May 2009. On 2-3 January 2009, activity from
the lava dome increased drastically. On 2 January, an energetic
pyroclastic flow and associated surge traveled down Tyers Ghaut (NW)
and reached the upper part of Belham River. On 3 January, after a
period of elevated seismicity, two explosions produced large ash
plumes that rose to altitudes greater than 10.7 km. Ashfall affected
most of the island at elevations of 1.2 km and above. The explosions
had significant "jet components" that rose to at least 500 m above the
dome. In-column collapses resulted in pyroclastic flows that traveled
W and reached Plymouth (~ 5 km W). According to news articles, about
70 people were evacuated from an area about 6-8 km NW.

According to MVO, the level of seismic activity decreased dramatically
after 3 January. It increased slightly in early February, with
occasional rockfalls, and several small pyroclastic flows. On 19
February 2009, the Hazard Level was lowered to 3. Seismic activity
remained low during March through May. Occasionally, lahars caused by
heavy rainfall descended through multiple river valleys. Thermal
images of a pyroclastic flow on 25 February 2009, and other videos,
can be viewed on the MVO YouTube channel
(http://www.youtube.com/user/montserratvolcanoobs).

In mid-May 2009, activity from the Soufriere Hills lava dome increased
slightly, but generally remained at a low level. Tectonic earthquakes
were noted on 16, 18, 20, and 21 May at depths less than 3 km beneath
the lava dome. Two possible explosions were detected on 21 May. The
second and larger signal was followed by an ash plume that drifted W
over Gages Mountain. During 21-22 May, a strong smell of sulfur
dioxide was noted from Salem (6 km NW) to Woodlands (1 km N of Salem).
Heavy rainfall caused erosion of the lava dome and hot pyroclastic
flow deposits; steam plumes occasionally laden with ash occurred
periodically from the base of Tyre's ghaut. Lahars traveled down
multiple river valleys on 18 May.

Activity during May-December 2009. Between the latter part of May and
4 October 2009, activity remained low with only periodic rockfalls and
small pyroclastic flows. On 4 October 2009, a short volcano-tectonic
earthquake swarm from the Soufriere Hills lava dome was detected. A
period of tremor and vigorous ash venting followed about an hour
later. The resulting ash plume drifted WNW across the island and out
to sea, causing ashfall in Old Towne and Olveston. The seismic signals
indicated no explosive activity or pyroclastic flows, but only two
rockfalls after the ash-venting event. On 5 October, intermittent ash
venting continued (figure 10), and ash fell S of inhabited areas.
Early on 7 October, the ash-venting events from the lava dome ceased
after a total of 13 had occurred. The last three were associated with
small pyroclastic flows that traveled about 500 m down Tyers Ghaut to
the NNW.

Figure 10. Earth Observatory natural-color satellite photo of
Soufriere Hills acquired on 6 October 2009. The photo shows an ash
plume extending W, a day after eruptive activity resumed on 5 October.
According to the U.S. Air Force Weather Agency, ash rose to 3.6 km and
extended 280 km. Courtesy NASA Earth Observatory (image by Jeff
Schmaltz, MODIS Rapid Response, NASA Goddard Space Flight Center).

By mid-October 2009, activity from the Soufriere Hills lava dome rose
to a high level. A new lava dome, first reported on 9 October,
continued to grow. The new lava dome summit was about 60 m above the
old dome structure. Seismicity was high and cycles of low-level tremor
occurred at regular intervals. Over 1,200 rockfalls were detected and
pyroclastic flows traveled down every major drainage valley except the
Tar River valley to the E, resulting in ash plumes (figure 11). Heavy
rainfall caused a lahar in the Belham Valley to the NW on 14 October.
On 16 October, several large pyroclastic flows descended the White
River to the S and reached the sea. Moderate-sized pyroclastic flows
traveled 3 km NE down Tuitts Ghaut and White Bottom Ghaut, and a few
smaller pyroclastic flows descended Tyers Ghaut to the N. Extensive
ash clouds rose to an altitude of 6 km and drifted WNW, resulting in
multiple minor ashfall in inhabited areas. Venting on 6 October 2009
can be seen on the YouTube channel for the Government Information Unit
of Montserrat (http://www.youtube.com/user/GIUGOV). Lahars traveled NW
down the Belham valley.

Figure 11. Photo of Soufriere Hills taken from the International Space
Station on 11 October 2009. Photo shows ash and steam plume extending
W. Gray deposits that include pyroclastic flows and lahars are visible
extending from the volcano toward the coastline. Courtesy NASA Earth
Observatory.

During the last week of October 2009, seismicity decreased slightly.
However, numerous pyroclastic flows, some of which produced ash
plumes, occurred in most of the major drainage valleys. Rockfalls were
concentrated in the S. Heavy rainfall continued to cause lahars in the
Belham Valley. On 29 October, a 40-m-high spine was seen protruding
from the summit. Changes in lava-dome morphology seen on 30 October,
and occurrences of pyroclastic flows traveling NE, indicated that
growth was concentrated in the central part of the lava dome.

By 30 October, activity was again at a high level. Hybrid earthquakes
were recorded for the first time since the renewal of activity in
early October. Numerous pyroclastic flows occurred in most of the
major drainage valleys. The frequency of pyroclastic flows increased
on 5 November and particularly vigorous flows occurred in Tuitt's
Ghaut to the NE. Ash fell in inhabited areas on a few occasions.
Lahars descended the Belham Valley several times. Good views of the
lava dome on 9 and 10 November revealed that recent lava-dome growth
was concentrated on the WSW side, immediately NE of Chances Peak;
intense incandescence and rockfalls were noted at night. Ash fell
across the Montserrat on 11 November, and about 6-8 km NW in Salem,
Old Towne, Olveston, and Woodlands on 12 November. One pyroclastic
flow nearly reached the sea at Kinsale village (WSW).

By mid-November, activity from the Soufriere Hills lava dome consisted
of ash venting along with semi-continuous rockfalls and pyroclastic
flows that were concentrated on the W flank. Ashfall occurred across
many areas of the island. On 19 November, heavy ashfall occurred to
the NW between Old Towne and Brades. Views of the lava dome on 16
November showed that the dome height had decreased because of
collapses and that a deep channel had developed NE of Chances Peak.
Pyroclastic flows in the Gages Valley (W) continued down Spring Ghaut
and Aymer's Ghaut, and spread onto the alluvial fan below St. Georges
Hill.
On 21 November 2009, activity returned to a high level. Periods of
tremor were detected on 23 November. Lava extrusion during this period
shifted from the W side of the lava dome to the summit region. As a
result, abundant pyroclastic flows traveled NE down Tuitt's Ghaut on
23 November for the first time in several weeks. On 24 November there
was a period of 120 minutes of continuous pyroclastic flow activity,
followed by 90 minutes of semi-continuous activity. The pyroclastic
flows traveled W down Gages Valley and into Spring Ghaut, and NE down
Tuitt's Ghaut and Whites Bottom Ghaut reaching Tuitt's village.
Associated ash plumes rose to an altitude of 6.1 km. On 26 November, a
pyroclastic flow that descended the Tar River valley was caused by
collapse of part of the old, pre-2009 lava dome. Ashfall occurred in
Old Towne and parts of Olveston. Incandescent material seen in a
photograph taken at night on 29 November traveled down the flanks of
the lava dome in several areas.

High-level activity from the lava dome continued through the first
half of December 2009. Dome growth was concentrated on the N side,
which has led to approximately 100 m of lateral growth of the lava
dome in a northward direction. This growth has increased the available
material for the formation of pyroclastic flows. Pyroclastic flows
down the N flank became more abundant and their runout distance
steadily increased. Pyroclastic flows also occurred to the NE and W,
and one reached within 200 m of the sea. Ash vented from the S part of
the lava dome.

On 10 December 2009, a large pyroclastic flow traveled down Tyers
Ghaut. This pyroclastic flow reached to below the west end of Lees
village in the Dyers river, some 3.5 km from the lava dome. This event
prompted MVO to raise the Hazard Level from 3 to 4. The higher Hazard
Level signifies that larger pyroclastic flows moving down the Belham
valley are a more likely possibility. According to MVO, larger
pyroclastic flows could be formed by a partial dome collapse which
could involve several million cubic meters of material. Helicopter
observations have shown that the head of Tuitt's Ghaut down to the
junction with Whites Bottom Ghaut is full of pyroclastic flow deposits
such that there is now a continuous surface across from Farrell's
plain. The head of Tyers Ghaut is also now nearly full. This means
that future pyroclastic flows are likely to be less confined by
topography and will spread more readily across the N flanks of the
volcano.

Thermal anomalies. MODIS satellite imagery recorded many thermal
anomalies during December 2008, a smaller number in January 2009, none
in February 2009, one in March 2009, and none during April through 10
October 2009. Beginning on 11 October through 11 December 2009, MODIS
recorded a large number of thermal anomalies.

Geologic Summary. The complex, dominantly andesitic Soufriere Hills
volcano occupies the southern half of the island of Montserrat. The
summit area consists primarily of a series of lava domes emplaced
along an ESE-trending zone. English's Crater, a 1-km-wide crater
breached widely to the east, was formed during an eruption about 4000
years ago in which the summit collapsed, producing a large submarine
debris avalanche. Block-and-ash flow and surge deposits associated
with dome growth predominate in flank deposits at Soufriere Hills.
Non-eruptive seismic swarms occurred at 30-year intervals in the 20th
century, but with the exception of a 17th-century eruption that
produced the Castle Peak lava dome, no historical eruptions were
recorded on Montserrat until 1995. Long-term small-to-moderate ash
eruptions beginning in that year were later accompanied by lava-dome
growth and pyroclastic flows that forced evacuation of the southern
half of the island and ultimately destroyed the capital city of
Plymouth, causing major social and economic disruption.

Information Contacts: Montserrat Volcano Observatory (MVO), Fleming,
Montserrat, West Indies (URL: http://www.mvo.ms/); Washington Volcanic
Ash Advisory Center, Satellite Analysis Branch (SAB), NOAA/NESDIS
E/SP23, NOAA Science Center Room 401, 5200 Auth Rd, Camp Springs, MD
20746, USA (URL: http://www.ssd.noaa.gov/VAAC/); NASA Earth
Observatory (URL: http://earthobservatory.nasa.gov/); 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://hotspot.higp.hawaii.edu/); U.S. Air Force Weather Agency
(AFWA)/XOGM, Offutt Air Force Base, NE 68113, USA (Email:
Charles.Holliday@xxxxxxxxxxx).



San Vicente
El Salvador
13.595°N, 88.837°W; summit elev. 2,182 m
All times are local (= UTC - 6 hours)

During 7-8 November 2009, heavy rains caused landslides and flooding
in areas NE to NW of San Vicente in central El Salvador (figure 12),
resulting in flooded rivers, buried homes and car, and casualties. The
most recent volcanic activity consisted of lava flows that were
covered by an eruption of neighboring Ilopango volcano in 260 AD.
According to the USGS, previous earthquake-and rainfall-triggered
landslides and lahars occurred in 1774, 1934, 1996, and 2001. In 1774,
a lahar on the NE flank affected the town of San Vicente. The 1934
lahar on the N flank destroyed the town of Tepetitan, more than 6 km
from the summit. In 1996, landslides and lahars on the S flank damaged
the major roadway between Tecoluca (17 km NW) and Zacatecoluca (6 km
SSW). On 13 February 2001, a M 6.6 earthquake caused more than 25
landslides on the N and NW flanks of the volcano that reportedly
killed 39 people. However, no subsequent volcanic activity occurred
from San Vicente, San Miguel, San Salvador, or Santa Ana volcanoes.

Figure 12. Location map of San Vicente volcano in the Departamento of
San Vicente, in El Salvador. The country is divided into 14
Departamentos; five of these were affected by the 7-8 November events.
The capital is San Salvador, 40 km WNW of San Vicente.

Frequent and heavy rains on 7 November 2009 and into the next morning
caused landslides, lahars, and flooding in the major drainages around
the northern flanks of San Vicente. Servicio Nacional de Estudios
Territoriales (SNET) reported that debris flows traveled up to 7 km
away, severely affecting roads and towns. Loss of life and property
were particularly severe in Verapaz, population ~ 3,000, (about 6 km
NW of the summit) and Guadalupe (5 km NW from the summit, on the
flanks), although damage was reported in several areas, including in
the capital of San Salvador, 40 km WNW. According to the Pan American
Health Organization (PAHO), the rate of rainfall at San Vicente
volcano was 81 mm/hour, for a total of 355 mm in a 24-hour period.
Five of the 14 Departamentos were affected by events caused by the
rainfall: San Vicente, La Paz, La Libertad, San Salvador, and
Cuscatlan.

On 9 November an eyewitness living in Verapaz noted in media reports
that, "It was about two in the morning when the rain started coming
down harder, and the earth started shaking... The next thing I knew I
was lying among parts of the walls of my house." Another resident
stated, "I started to hear roaring noises and the ground began to
shake. Then my windows broke and lots of mud came in..." According to
news articles, about 300 houses were flooded when a river in the town
overflowed. Extensive damage was done to roads (figure 13), water and
power sevices, and croplands in Verapaz.

Figure 13. A resident walks through an area hit by a landslide after
torrential rains in Verapaz, El Salvador, on 9 November 2009. Photo by
Yuri Cortez, AFP/Getty Images.

In the capital of San Salvador, eyewitnesses described an area of 8
km^2 that had been covered by rocks, mud, and debris, and that many
houses and hamlets had completely disappeared. At least six bridges
were swept away and landslides blocked major and secondary roads,
cutting communication and hindering clean-up efforts.

Based on information from PAHO, the number of people in shelters
peaked on 16 November at 15,090. As of 22 November, 198 people had
died, 77 were missing, and 5,759 remained in shelters. The estimated
number of affected people was 75,000.

Geologic Summary. The twin peaks of San Vicente volcano, also known as
Chichontepec, rise dramatically to the SE of Lake Ilopango. The modern
andesitic stratovolcano was constructed within the Pleistocene La
Carbonera caldera, whose rim is visible only on its SW side. San
Vicente volcano, the second highest in El Salvador, grew within the
caldera to form a paired volcano with summit craters oriented along a
WSW-ENE line. The northern and southern flanks are covered by lava
flows from the central vent, but lava flows on the eastern side
originated from a vent on the upper flank. Volcanism has continued
into the Holocene, but the latest lava flows are covered by deposits
from the major ca. 260 AD eruption from neighboring Ilopango volcano.
Reports of historical eruptions in 1643 and 1835 are false (Catalog of
Active Volcanoes of the World; Sapper, 1917), but numerous hot springs
and fumaroles are found on the northern and western flanks of the
volcano.

Information Contacts: Servicio Nacional de Estudios Territoriales
(SNET), Km. 5 1/2 carretera a Santa Tecla y Calle las Mercedes,
contiguo a Parque de Pelota, Edificio SNET, Apartado Postal 27, Centro
de Gobierno, El Salvador 2283-2246 (URL: http://www.snet.gob.sv/); Pan
American Health Organization (PAHO) - El Salvador, 73 Avenida Sur No.
135, Colonia Escalon, San Salvador, El Salvador (URL:
http://devserver.paho.org/els/); Associated Press (URL:
http://www.ap.org/); Los Angeles Times, 202 West 1st Street, Los
Angeles, CA 90012, USA (URL: http://www.latimes.com/); BBC News (URL:
http://news.bbc.co.uk/).



Fernandina
Galapagos Islands, Ecuador
0.37°S, 91.55°W; summit elev. 1,476 m
All times are local (= UTC - 6 hours)

Silvana Hidalgo and Patricia Mothes of the Ecuador Instituto Geofisco,
Escuela Politecnica Nacional (IG-EPN) (Geophysical Institute, National
Polytechnic School) sent an informal report on gas and temperature
measurements during the final stage of the April 2009 eruption of
Fernandina (Bourquin and others, 2009). Our last report on Fernandina
in April 2009 (BGVN 34:04) discussed this eruption. The following
information came from that document.

The 2009 Fernandina volcano eruption, beginning 11 April 2009, was
characterized by an extensive lava outpouring on the SW flank and
sulfur dioxide (SO2) gas emission. First eyewitnesses reported an
eruptive column on the morning of 11 April. Thermal and SO2 anomalies
were shown by MODIS and AURA satellites, respectively. Rangers from
the Galapagos National Park Service (GPNS) found the active eruptive
fissure during a flight on 13 April 2009 (figure 14) . That fissure
was near the 2005 eruptive fissure (BGVN 30:04). The 2009 fissure was
~ 200 m long and 10 m wide, and ejected lava fountains 15 m high. A
gas and ash plume drifted SW, and a steam plume rose where the lava
flow poured into the ocean (figure 15).

Figure 14. Aerial photograph taken 13 April 2009 of the eruptive
fissure seen as a horizontal band with a curtain of lava fountains
during the Fernandina eruption. Courtesy of Oscar Carvajal, GNPS
ranger; from (Bourquin and others, 2009).

Figure 15. Aerial photograph taken 13 April 2009 of the steam plume
caused by lava flowing into the ocean during the Fernandina eruption.
Courtesy of Oscar Carvajal, GNPS ranger; from (Bourquin and others,
2009).

During a flight on the morning of 15 April, personnel from the GNPS
verified that the eruption continued, but with lower intensity than in
the days before. Three vents discharging lava at ~ 400 m elevation on
the SW flank along a radial fissure were active, feeding a lava flow
up to 10 m wide. During 15-16 April, gas-and-steam plumes from
Fernandina drifted up to 555 km W.

The images recorded by the OMI (ozone monitoring instrument)
satellite-borne platform showed a drastic decrease of activity after
16 April and a new increase on the 23 April (there was no data between
19 and 23 April due to a satellite update). This decrease in the
eruption intensity correlated with a drop in the number of thermal
alerts detected by MODIS satellite. The eruption ended on 28 April
2009.

A field campaign was conducted by IGEPN from 27 April to 5 May 2009 to
compare ground results with satellite data. Measurements of the SO2
associated with the eruption were conducted 29-30 April. At this time
the eruption was nearing completion; the scientists were unable to
make field measurements of the high SO2 fluxes during the earlier,
more vigorous eruption phase.

SO2 measurements. The SO2 measurements were carried on using a
mobile-DOAS (differential optical absorption spectroscopy) instrument
composed of a small, upward-looking telescope, connected by optical
fiber to a spectrometer and a GPS (global positioning system) receiver
(figure 16). The measurements were performed during several traverses
around the eruption vent using a small boat supplied by the Galapagos
National Park. One traverse along the W side (downwind side) of the
island, conducted on 29 April 2009, found a SO2 flux maximum
measurement of 2,997 tons/day. On 30 April, a traverse along the S and
SW side of the island measured 527 tons/day. The IG-EPN report gave
more detailed data on all measurements in support of the SO2 program
made during the 2-day survey.

Figure 16. Shaded relief map [digital elevation model (DEM)] of
Fernandina Island including the NW part of Isabela to the E. The
labeled lines correspond to the small boat traverses done on 29-30
April 2009 to measure environmental properties for SO2 flux analyses .
Courtesy of Bourquin and others, 2009.

Ozone monitoring instrument (OMI) satellite images showed degassing
from 11-16 April 2009, with the higher SO2 values on 12 and 14 April.
This degassing was associated with ash emission observed with MODIS
satellite (shown in BGVN 34:04). From 17-19 April almost no SO2 was
visible in the satellite images. After 4 days without data, satellite
images showed a high SO2 emission on 23 April, increasing until 25
April when the eruption began its decline. After this date, and for
the days when the field measurements were conducted, little SO2 was
present in the atmosphere.

Thermal measurements. The team made measurements using a forward
looking infrared (FLIR) thermal camera during a flight over the zone
covered by the fresh lava flows (figure 17, table 5). These
measurements, associated with post eruption satellite images, allowed
an estimation of the area covered by the eruption products.

Figure 17. High-resolution satellite image after the April 2009
Fernandina eruption identifying individual lava flows and other points
of interest. Courtesy of Bourquin and others (2009).

Table 5. Description of points of interest at Fernandina from
comparison of satellite thermal images and lava flow photographs.
Location numbers in the first column correspond to the numbered points
in figure 17. Courtesy of Bourquin and others (2009).

   Location    Date of event
    number

                   Comments

      1        1995 eruption (radial fissure)
                   Upper vents at elevation of ~1,000 and ~750 m with
the associated lava flows.
      2        2005 eruption (circumferential fissure)
                   Upper vents with the associated lava flows.
      3        2009 eruption (radial fissure)
                   Upper vents at elevation of ~550 m covering part of
the 1995 eruptive fissure
                   and lava flows; vents displayed activity during the
first overflight (13
                   April 2009) (figure 18); maximum apparent
temperature measured with the
                   thermal camera was 179.3°C.
      4        2009 eruption (radial fissure)
                   Upper vents at elevation of ~700 m located to W of
1995 eruptive fissure;
                   vents active during the first flight (13 April
2009); maximum apparent
                   temperature measured with the thermal camera was 67°C.
      5        2009 eruption
                   Dark grey patch not observed on images previous to
April 2009 eruption; might
                   correspond to a short-life vent with small lavas.
      6        2009 eruption (radial fissure)
                   Principal vents at elevation of ~500 m; last visual
observation of
                   incandescence was on 29 April 2009 during;
measurements with the thermocouple
                   in a 50 cm crack and greater-than-30-m-long crack
gave maximum temperature of
                   970°C.
      7        2009 eruption
                   Area covered by principal April 2009 lava flows
that reached the sea; maximum
                   apparent temperature measured with the thermal
camera was 131.9°C.
      8        1995 eruption (radial fissure) influence 2009 lava flow
                   Principal 1995 vent; during the first part of 2009
eruption, lava flowed W to
                   this vent and reached the ocean; after a while, it
changed its course and
                   flowed E to the vent but never reached the ocean.
      9        1995 lava field and 2009 lava flow
                   SE lobe of the 2009 lava flow borders 1995 lava
field and ends 1,800 m before
                   entering into the ocean; maximum apparent
temperature measured with the
                   thermal camera was 70.9°C (figure 19).
     10        2009 eruption
                   April 2009 lava flows entered into the ocean the
first days of the eruption;
                   this region of the lava flows is 800 m-wide (figure
20); maximum apparent
                   temperature measured with the thermal camera was 132°C.
     11        1995 eruption
                   1995 eruption lava field.

Figure 18. Aerial photo showing the upper fissure and the principal
vents of the April 2009 Fernandina eruption. Courtesy of Bourquin and
others (2009).

Figure 19. Photograph of SE lava flow (area 9) from the April 2009
Fernandina eruption. Area number 11 corresponds to the 1995 eruption
lava field. Courtesy of Bourquin and others (2009).

Figure 20. Photograph of lava flow entering the ocean on the SW coast
(area 10) from the April 2009 Fernandina eruption. Courtesy of
Bourquin and others (2009).

Estimation of the area covered. The area covered by the April 2009
Fernandina volcano eruption was estimated using (1) thermal images
taken with the infrared camera FLIR during the overflight of 1 May
2009, (2) QUICKBIRD satellite image (browse image visible; 11 May
2009), (3) ASTER satellite image (16 May 2009), (4) photographs taken
by the personal of IGEPN and GNPS during the overflight of 1 May 2009,
and (5) a Digital Elevation Model (DEM) provided by the IGEPN. Thanks
to the strong thermal contrast between the new products and the older
lava flows, it was possible to map precisely the limits of April 2009
eruption.

The thermal contrast information was stacked on the satellite images
and the area has been calculated with the help of the DEM (figure 21).
The area covered by the April 2009 eruption is of about 6.7 km^2 which
is a value similar to the 1995 eruption (6.5 km^2; Rowland and others,
2003). Unfortunately no thickness measurements are available for the
April 2009 lava flows. Nevertheless, considering the similarities
between both eruptions, IGEPN scientists used the average thickness
calculated by Rowland and others (2003) for the 1995 eruption (8.5 +-
2 m), to calculate the 2009 eruption volume. It gives an approximate
volume of 57 +- 13 million^ m^3 of lava emitted. This volume is
equivalent to those of 1995 and 1988 but the emission rates were
drastically different. This estimation has to be taken carefully as no
thickness measurement was done during the fieldwork.

Figure 21. Map of Fernandina showing the extent of the April 2009 lava
flows extending down the SW flank to the ocean. Courtesy of Bourquin
and others (2009).

Satellite thermal data. As shown in BVGN 34:04, from 11 April to 22
June 2009 MODVOLC detected 789 hot-spots on Fernandina Island with 725
during the time of the eruption and 64 after it. The number of thermal
alerts was the highest for 12 April and then decreased until the end
of the eruption. At least three episodes of high effusion occurred,
during 11-14, 16-19, and 28 April. Comparing these observations with
the OMI satellite images, the first two effusive episodes were
accompanied by high SO2 emissions, but not the last one. This could be
due to an artifact on the OMI satellite image for 28 April. The
decreasing number of thermal alerts after 28 April is thought to
illustrate the cooling of the lava flows, as they are not associated
with SO2 emissions.

Eruption photos. The smugmug.com website shows a number of photos of
the April 2009 Fernandina eruption from offshore. According to the
website, the vessel carrying the photographers was restricted from
sailing to visit the side of Fernandina Island where the volcano was
erupting in mid-April. On 19 April the vessel was given permission by
the Galapagos National Park to see the volcano. The boat anchored ~
1.6 km offshore and the photographers boarded small boats to get
within ~ 90 m of where the lava was pouring into the sea (figures 22
and 23).

Figure 22. Night photo of the ocean entry area at Ferandina taken 19
April 2009. In this photo a small boat is apparent in the right
midground, with siloutees of people highlighed by incandescene in the
background. Courtesy of smugmug; the photographer's name was not
specified on that website.

Figure 23. Photo of the ocean entry area at Fernandina taken 19 April
2009. In this photo the red-orange lava about to enter the ocean is
apparent at right and at elevation on the left appears a a fountain
jets towards the night sky. Courtesy of smugmug; the photographer's
name was not specified on that website.

References: Bourquin, J., Hidalgo, S., Bernard, B., Ramon, P.,
Vallejo, S., and Parmigiani, A, 2009, April 2009 Fernandina volcano
eruption, Galapagos Islands, Ecuador: SO2 and thermal field
measurements compared with satellite data: Informal report, Instituto
Geofisco Escuela Politecnica Nacional (IGEPN).

Rowland, S.K., Harris, A.J.L., Wooster, M.J., Amelung, F., Garbeil,
H., Wilson, L, and Mouginis-Mark, P.J., 2003, Volumetric
characteristics of lava flows from interferometric radar and
multispectral satellite data: The 1995 Fernandina and 1998 Cerro Azul
eruptions in the western Galapagos: Bulletin of Volcanology, v. 65,
no. 5, p. 311-330.

Geologic Summary. Fernandina, the most active of Galapagos volcanoes
and the one closest to the Galapagos mantle plume, is a basaltic
shield volcano with a deep 5 x 6.5 km summit caldera. The volcano
displays the classic "overturned soup bowl" profile of Galapagos
shield volcanoes. Its caldera is elongated in a NW-SE direction and
formed during several episodes of collapse. Circumferential fissures
surround the caldera and were instrumental in growth of the volcano.
Reporting has been poor in this uninhabited western end of the
archipelago, and even a 1981 eruption was not witnessed at the time.
In 1968 the caldera floor dropped 350 m following a major explosive
eruption. Subsequent eruptions, mostly from vents located on or near
the caldera boundary faults, have produced lava flows inside the
caldera as well as those in 1995 that reached the coast from a
SW-flank vent. Collapse of a nearly 1 cu km section of the east
caldera wall during an eruption in 1988 produced a debris-avalanche
deposit that covered much of the caldera floor and absorbed the
caldera lake.

Information Contacts: Silvana Hidalgo and Patricia Mothes, Instituto
Geofisco Escuela Politecnica Nacional (IGEPN) (Geophysical Institute,
National Polytechnic School), Casilla 1701-2759, Quito, Ecuador
(Email: shidalgo@xxxxxxxxxxxx and pmothes@xxxxxxxxxxxx; URL:
http://www.igepn.edu.ec/); 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://hotspot.higp.hawaii.edu/);
SmugMug (URL: http://www.smugmug.com;
http://www.wildphotopics.com/Travel-International/Galapagos-Islands-and-Quito/Fernandina-Island-La/8109366_9nVGc/1/528644840_CChcM).

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