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Three ESA satellites reveal Etna’s complexity
by the European Space Agency
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Smoke and ash drifts toward the African coast from
Mount Etna in this ESA MERIS image of 28 October,
2002
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| 30 October
2002 As detected by ESA satellite sensors, the recent
eruptions of the Mount Etna volcano in Sicily are throwing huge amounts of
ash and trace gases into the atmosphere. Instruments on three different
ESA spacecraft have acquired imagery of the eruptions that shed new light
on the event and its impact on the Earth’s
environment. Working with data from the Global Ozone
Monitoring Experiment (GOME) sensor onboard ESA’s ERS-2 spacecraft,
scientists at the German aerospace centre (DLR) report that levels of
sulphur dioxide from the eruptions on Sunday and Monday are at least 20
times higher than normal.
This latest activity from Etna, the second in a little over a year,
marks the beginning of another period of activity of Europe’s largest
volcano, says Werner Thomas, an atmospheric scientist with DLR’s Remote
Sensing Technology Institute.
“As in July and August 2001 eruptions of Etna, dense ash clouds and
gaseous emissions were again detected by several space-borne sensors,” he
said.
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GOME-based analysis of sulphur dioxide levels from
the Mt. Etna eruption shows levels 20 times higher than
normal.
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| The normal background
level of sulphur dioxide is typically below 0.5 Dobson Units (DU), a
measure of atmospheric gas concentrations from ground level to the top of
the atmosphere, about 70 km in altitude.
"In the plume, we measured atmospheric content of sulphur dioxide of
about 10 DU, at least 20 times higher than normal," Thomas said.
Sulphur dioxide in the troposphere, the lowest part of the atmosphere
where most weather changes occur, is known to be responsible for the
so-called "acid rain" phenomenon. Stratospheric sulphur dioxide, from
about 11 km to 50 km above the Earth’s surface, causes the formation of
sulphate aerosol particles that may have a serious impact on the global
climate. Etna is one of the most prominent sources of natural sulphur
dioxide worldwide. 
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ATSR-2 image of Etna
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| The ERS’ GOME
instrument is dedicated for remote sensing of the atmosphere and can
detect a variety of atmospheric trace gases, including sulphur dioxide.
The first GOME data after the beginning of the eruptions was recorded and
analysed on 29 October around 10:15 UTC. As seen in the accompanying
chart, enhanced levels of sulphur dioxide are evident in the southeast of
Sicily, indicating that the tropospheric sulphur dioxide was carried away
from the volcano by the winds in that direction.
The Italian government declared a state of emergency yesterday in
Sicily in the wake a series of earthquakes, measuring between 3.6 and 4.3
on the Richter scale, that forced the evacuation of approximately 1000
homes, according to reports from BBC and Italian newspapers. Meanwhile,
three streams of lava from the eruption flowed down the south, northeast
and northwest slopes of the mountains, the media reports
stated.
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Eruption spews lava and ash
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| Ash to affect
global environment Europe's highest and most
active volcano (3370 m) hurled lava and ash from several craters into the
sky with a speed between 350 and 450 metres per second, exceeding the
speed of sound. According to data from volcanologists, the lava and ash
were ejected from the main crater and from at least nine new craters that
developed in the mountain between 2300 to 2700 metres in altitude.
As seen in the image acquired Monday by the Medium Resolution Imaging
Spectrometer (MERIS) onboard ESA’s Envisat satellite, the eruptions spewed
significant amounts of ash, along with sulphur dioxide, into the
atmosphere The plume from the volcano can be seen in the image stretching
south and west from Sicily to the north African coast. The larger volcanic
ash particles are expected to settle out in a short period of time, but
the sulphuric acid aerosols produced by the sulphur dioxide will persist
for several years.
These aerosols will
impact the Earth’s energy budget, both regionally and on a global scale.
Aerosols containing black graphite and carbon particles are dark, thus
absorbing sunlight. As these atmospheric particles reduce the amount of
sunlight reaching the planet’s surface, they increase the amount of solar
energy absorbed in the atmosphere, thus simultaneously cooling the surface
and warming the atmosphere.
The capability of the MERIS instrument to observe the spatial
distribution of these aerosol plumes can be exploited to measure the
amounts of airborne particles and to examine the role of these aerosols as
cloud condensation nuclei and their impact on the hydrologic cycle through
changes in cloud cover, cloud properties and precipitation.
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Proba's CHRIS shows the smoke
plume
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| Today’s images from
Proba Just 60x60x80 cm and weighing only 94 kg,
ESA’s Project for On-Board Autonomy satellite, better known as Proba, is
one of the most advanced small satellites ever flown in space.
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Another Proba view of Etna
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| Since its launch last
year, Proba’s high-performing computer system and technologically advanced
instruments have enabled it to demonstrate and evaluate onboard
operational autonomy, new spacecraft technology both hardware and
software, and to test Earth observation and space environment instruments
in space.
The imagery captured today by Proba demonstrate the capabilities of
CHRIS, the Compact High Resolution Imaging Spectrometer, which is
providing important information on the Earth and its environment, and will
be a valuable tool in remote sensing during the extended mission.
The instrument
acquired the accompanying Etna images in four standard bands, although the
instrument is capable of image acquisition in up to 19 different
bands.
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