The objective of this research is to
understand volcanic processes using
temporal observations and
modelling of gravity field and displacements.
From an initial state considered as a time-reference, gravity may change
on volcanoes because of
Tha amplitude changes are of the order of centimeters to meters for the deformation, whereas it is of the order of 1-1000 microgal (1 microgal=10-8 m/s2). Very accurate instruments are required and we need to obtain observation or to model other variables at the same time, like the deformation (accuracy for height change at 1 cm level) or the pressure. Figure caption Schematic temporal evolution of an active volcano. Possibilities to produce gravity changes are reported in the figure. From an initial state (state 1), where blacks dots represent the location of measurement points, the gravity variation at the second state (state 2) may change due to surface movement (which involves free-air elevation change and volume change of the volcano), mass redistribution of the topography at surface (extrusions) and internal mass redistribution, the amount of which we are looking for (after Jousset et al., 1999;Jousset et al., 2000;). |
Volcanological Survey of Indonesia Usu Volcano Observatory, Japan Institut de Physique du Globe de Paris, France
Merapi, one of Indonesia's most active volcanoes, lies in one of the world's most
densely populated areas and dominates the landscape immediately N of the
major city of Yogyakarta. The steep-sided modern Merapi edifice, its upper
part unvegetated due to frequent eruptive activity, was constructed to
the SW of an arcuate scarp cutting the eroded older Batulawang volcano.
Pyroclastic flows and lahars accompanying growth and collapse of the steep-sided
active summit lava dome have devastated cultivated and inhabited lands
on the volcano's western-to-southern flanks and caused many fatalities
during historical time. The volcano is the object of extensive monitoriong
efforts by the Merapi Volcano Observatory of the Volcanological Survey
of Indonesia." (from GVP/USGS Weekly Volcanic Activity Report).
Within the Arrangement between the Volcanological Survey of Indonesia and the French Goverment, a series of studies have been carried out in the mid-90's, involving the observations of gravity and deformation, during an intense activity of the volcano. The gravity variations were linked to the growth and collapse of the
dome (figure), but also allowed to propose a model for the activity of
the volcano at the time. The crystallisation and degassing of implaced
magma would be responsible of the dome growth.
Figure caption Observed gravity variations for 1993-1994 period at Merapi volcano. Despite the small deformation, large gravity variations occured at the summit area, whereas no changes occured far from the volcano summit. This effect is mainly due to the dome activity. The open squares indicate the theoretical attraction of the extruded dome, computed form the estimations of the dome shape (using a density oof 2400 kg.m-3). The error bar associated to these squares refelct the range of the possible theoretical attractions computed from different cases of dome, including shape, volume and density (after Jousset et al., 2000). |
Figure caption
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Several small phreatic eruption occured in March 1996, October 1998
and November 2000. The Coordinating Committee for Prediction of Volcanic
Eruption (CCPVE) noted that repeating small-scale phreatic eruptions may
be possible advance signs of a large eruption, such as for the 1929 eruption.
Within this context, a two-year project of the Japanese Society for the Promotion of Science, 4 sessions of gravity and displacement have been obtained by teams of the Usu Volcano Observatory. Our observations are consistent with a model of underground shallow-water evaporation occuring as a result of heat rising from a hot and dense body (density contrast of 200 kg.m-3) of about 10^11 kg at 4-5 kg in depth. |
Within the same project of the Japanese Society for the Promotion of
Science at Komagatake volcano, several sessions
of observations have been carried out at Usu
Volcano between September 1996 and August 1998, using both
microgravity and GPS observations on a large network covering
Results revealed that the dome associated with the 1977-1978 eruption was still contracting due to compaction and cooling. There was also a rise of 1.5 m of the water table, which might be a precursor to the 2000 eruption (see below).
Figure caption Gravity Variations as a function of height
variations.
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At 13:10 (JST), 31 March [2000], an eruption started at about 4 km NW
of the summit, and at about 2 km NE of the epicenter of volcanic earthquakes,
that occured within the few days before the outburst.
The National Committee of Volcanic Eruption Prediction, chaired by
Prof. Yoshiaki Ida (U. Tokyo) showed the official comments on 22 May as
follows:
"At Usu volcano, eruption has continued
since March 31, though it became small in the activity. In the initial
stage of eruption, many craters appeared and issued volcanic ash. The eruption
activity concentrated into a few craters in the mid-April, repeating intermittent
explosions. The degree of explosion and amount of eruption cloud gradually
decreased with time. Magmatic material (pumice) that was found in the initial
stage of eruption were hardly observed in products of successive eruptions.
Although many felt earthquakes occurred
before and after the commencement of eruption (the maximum M=4.6), such
the seismicity declined soon. Though earthquakes have still continued several
kilometers below the western and southern parts of the volcano, their distribution,
frequency and magnitude (M2 to 3) have not been changed since the mid-April.
During the activity, the West-Nishiyama
area was largely uplifted, the highest part reaching about 60 m, and the
volume of uplifting is
estimated about 40 million cubic meters. The uplifting rate decreased
with time, and is 10 cm a day these days. The time needed for the uplifting
rate declining is smaller by one order than those associated with the dome
formation in the 1944-45 and 1977-78 eruptions, and the same in order as
that in the 1910 eruption.
As the above, the magma activity had
gradually declined and there is a possibility that the activity comes to
an end. As eruption, uplifting and seismicity have still continued, however,
it is still probably that explosions damaging the areas around the present
active craters take place due to new interaction of magma with underground
water.
Although it is impossible to deny the
possibility of a new lager eruption due to the increase of magma supplied
from beneath, it is likely that such the eruption can be predicted as changes
in ground deformation, seismicity, and mode of eruption cloud. Should still
pay attention to the eruptive activity near the crater areas. Careful and
continuous monitoring of the eruptive activity is critical to detection
of its reactivation."
Within this context the Comite d'Evaluation des Risques Volcaniques (France) decided to learm from this experience how to manage a volcanic crisis. New observations of gravity have been obtained and are currently under process. The huge deformation associated with this eruption (figure) is the first reason of the gravity change in this eruption. With gravity variation ranging 0 to more than 3 mGal at some station, these observations include some of the most large values of gravity change ever recorded on a volcano. This excellent data should be able to help quantifying the amount of new magma that intruded within the edifice, in association with this eruption.