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From March 18 to 31, 2003,
a team of fourteen scientists(*) set up geophysical instruments
around the Ethiopian volcano Erta Ale, located in the Danakil rift, where
a chain of volcanoes has formed over millions of years. The scientists
took samples of gases and lava. This is the first time since 1974 that
a French scientific mission financed by the CNRS has been able to return
to study this region of the Afar triangle.
Erta Ale is an exceptional volcano in more ways than one. It is one of
three volcanoes in the world that has had a continuously active lava lake,
probably since at least 1873. In addition, Erta Ale is part of a chain
of active volcanoes located in the center of one of the six Afar rifts
where an open ocean has formed in connection with a hot spot (inner Earth
volcanism). The mission was organized in the framework of the "The
Earth's Interior" Program and the "National program for major
natural risks" of the CNRS National Institute for Sciences of the
Universe. It was organized by laboratories belonging to the "Institut
de physique du globe" in Paris (IPGP), in association with the CNRS,
with the logistic support of Géo-découverte.
The initial objectives of the mission included understanding how a lava
lake works: the structure of the volcano's feeder conduits under the lake
and the processes involved in eruption. Judging by the lake's size, 80
meters in diameter in 2001, its depth is estimated to be at least 100
meters. Given its age, scientists think the lake must have a continuous
link to a shallow magma chamber, which is itself fed on a regular basis
by magma uplifts more directly connected to the formation of the rift.
The activity of the lava lake is characterized by several points of gas
discharge that release bubbles and by what appears to be rather stable
convection. The spots where the lava uplifts correspond to the location
of gas release. The study of convection in the lava lake (the number of
conduits or rising feeding currents, the depth at which bubbles appear,
etc.) is a key parameter in the dynamics of lava lakes. During the mission,
the scientists observed that the level of the lake had gone down 10 meters
since compared to the level recorded in 2001.
On March 18, the team of scientists set up its equipment along the edges
of the volcano and made a first helicopter flight to photograph the small
rift that was forming along the axis along which Erta Ale formed. A second
flight enabled team members to photograph the relief from a different
angle. These images will be used to create a digital elevation model,
i.e., a highly accurate three-dimensional relief map.
During the mission, the scientists took continuous recordings of geophysical
measurements for eight days. A network of temporary seismological stations
was set up around the crater to obtain an image of the deep structure
of the volcano under the lake, and to locate the position, shape and size
of what is probably the magma chamber. It recorded the ground vibrations
caused by volcanic activity. This technique is based on the same principle
as ultrasound, except that the emission of seismic waves recorded by seismologists
is natural. The network was composed of four so-called large-band stations
(which register seismic waves in a wide range of frequencies) located
in a radius near the lava lake and of five short-term stations (which
record only high frequencies) placed in a radius of two kilometers. This
system should make it possible to obtain an image of the structure of
the volcano under the lake, reaching a depth of around two kilometers.
In order to hear the "breathing" of the volcano, a set of microphones
and micro-barometers were arranged around the edge of the crater to study
the way the gas bubbles are released, and thus determine the depth and
shape of the conduit that likely connects the lake with the magma chamber.
Lastly, during the entire mission two cameras (one infrared and one digital)
took pictures in order to study the means of convection inside the lake.
The scientists observed magma surfaces at relatively stable locations,
which indicate that rising currents are associated with the gas bubbles.
The lava then flows to the surface and descends in what are also rather
stable locations. GPS readings were also taken around the crater to monitor
the deformations over time was also performed.
In addition to setting up instruments for taking geophysical measurements,
samples of gas and lava were also obtained. Ongoing fumarolian activity
occurs in the volcano. Scientists took samples of gases in the lava lake
and at a fumarole site. Some of the analyses were carried out while on-site
(for example, SO2 content) using a spectrometer, while other analyses
will be made in the laboratory. The gas samples were sealed in glass vials.
Samples of lava projections due to the formation of "pit craters"
and/or caldeira were also taken to determine their distribution and composition.
The surface map developed using aerial photographs will enable the scientists
to create a digital elevation model and conduct an in-depth study of the
small rift in formation. Seismological data of the deep structure of the
eruptive conduits and the underlying longitudinal magma chamber should
make it possible to analyze the interactions between the tectonic activity
and the magma activity near the volcano.
(*) In
particular:
The laboratories
of the "Institut de physique du globe" in Paris, research units
run jointly by the CNRS, Denis Diderot University, and Pierre and Marie
Curie University:
http://www.ipgp.jussieu.fr/francais/rub-institut/acc-inst.html
"lnstitut de
physique du globe" in Strasbourg, IPGS (CNRS, Louis Pasteur University
of Strasbourg): http://www-ulp.u-strasbg.fr/unite_recherche.php?u=12
The "Laboratoire
de Sciences de la Terre" (laboratory of Life Sciences" of the
Ecole Normale Supérieure in Lyon: http://www.ens-lyon.fr/LST/
The Magma and volcano
laboratory (CNRS, Blaise Pascal University of Clermont Ferrand, Jean Monnet
University of Saint-Etienne): http://wwwobs.univ-bpclermont.fr/lmv/
The Pierre Sue Laboratory
(CNRS, CEA): http://www-drecam.cea.fr/lps/index.html
The United States
Geological Survey
Contacts, project
leaders for the mission:
Jean-Louis Cheminée, IPGP
Tel: +33 1 44 27 34 67
e-mail: cheminee@ipgp.jussieu.fr
Eric Humler, IPGP
Tel:+33 1 44 27 50 88
e-mail: humler@ipgp.jussieu.fr
Isabelle Manighetti,IPGP
Tel: +33 1 44 27 24 37
e-mail: manig@ipgp.jussieu.fr
Communications contact INSU CNRS:
Christiane Grappin
Tel: +33 1 44 96 43 37
e-mail: christiane.grappin@cnrs-dir.fr
Press contact :
Magali Sarazin
Tel : +33 1 44 96 46 06
e-mail : magali.sarazin@cnrs-dir.fr
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