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Microgravity and deformation observations and modelling in volcanology
Philippe Jousset
last updated 10 october 2002

The objective of this research is to
understand volcanic processes using
temporal observations and modelling of gravity field and displacements.


 


Principle


 
No pic? P.Jousset@earth.leeds.ac.uk From an initial state considered as a time-reference, gravity may change on volcanoes because of
  • deformation of the volcano
  • displacement of mass at the surface of within the edifice (water, magma, ...)
  • change in density within the edifice
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;).


Examples of studies


    Merapi, Indonesia
    Komagatake, Japan
    Usu, Japan
    Usu 2000 eruption


Collaborations

  • Volcanological Survey of Indonesia
  • Usu Volcano Observatory, Japan
  • Institut de Physique du Globe de Paris, France


  • Further information


    Please contact: P.Jousset@earth.leeds.ac.uk


     
     
     



    Microgravity studies at Merapi volcano, Jawa, Indonesia


     
    No Image? P.Jousset@earth.leeds.ac.uk 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).



    Microgravity studies at Komagatake volcano, Hokkaido, Japan


    Hokkaido-Komagatake, or Komagatake (Hokkaido), Volcano is located 30 km north of Hakodate City with a population of 320,000. This is an andesite stratovolcano (1,133 m high) whose summit has a 2 km-wide horseshoe-shaped caldera open to the E, resulted from large collapse 30-40 ka. Large-scale pumice-flow eruptions had occurred several times from craters within the caldera, including historical 3 major eruptions; 1640, 1856, and 1929. In the 1640 eruption, the summit part collapsed and the avalanche entered into sea, resulting in the generation of tsunami, killing 700 people. In 1929, one-day eruption issued 0.38 km^3 of ash falls and 0.14 km^3 of pumice flows; 2 killed and 4 injured. The eruption column height was 14 km. The pumice flows descended in all directions, reached about 8 km from the summit. Major eruptions at this volcano are characterized by very short activity duration (< a few days). The latest eruption took place in moderate-scale, such that eruption column reached 8 km above, in 1942. " (from Volcano Research Center, ERI, University of Tokyo).
     
     
    Image no there? P.Jousset@earth.leeds.ac.uk

    Figure caption
    Modelling of the gravity variations between November 1997 and May 1998. Observations are consistent with a double-source model: (1) a deep increase of mass at a depth of about 4 to 5 km below the surface, which contributes to the large-scale positive residual gravity signal (red curve); and (2) a shallow decrease of mass within the first hundred meters below the surface, which contributes to the crater-scale residual relative negative signal (green curve). The addition of these two computed signals explains the observed data (after Jousset et al., 2000).

    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.



    Microgravity studies at Usu volcano, Hokkaido, Japan

    Usu volcano(Hokkaido) is one of the most active volcanoes in Japan and was formed on the southern rim of the Toya Caldera around ten thousand years ago. Usu consists of a basaltic main edifice (49-53% SiO2) with a small summit caldera and ten dacitic lava or crypto domes (68-73 % SiO2) on the summit and northern slope. These are aliened in two parallel lines running NW-SE. Several thousand years ago the main edifice collapsed to the south and debris flowed down to the sea. After a long repose period the volcano erupted again in 1663 and since then has undergone six further eruptions. The eruptions that occurred at the summit (1663, 1769, 1822, 1853 and 1977-1978) commenced with a strong Plinian eruption and, apart from 1977-1978 were accompanying by pyroclastic flows. Except the 1769 (?), they also involved the growth of lava or crypto domes in the middle to
    final eruption stages. In the eruptions that occurred on the slopes (1910 and 1943-1945) the building of lava or crypto domes was proceeded phreatic explosions in the initial stage. Each eruption lasted for one month to two years, with between thirty and hundred years of repose period between them." (from Volcano Research Center, ERI, University of Tokyo).
     
     
    No Image? claim to P.Jousset@earth.leeds.ac.uk 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.
    Top: Normally gravity and elevation changes are inversely corralated. If no mass change is associated with the elevation change, then the gravity follows the free-air gradient. Both theoretical and estimated gradients are indicated on the figure. Similarly, if no density change occurs with elevation changes, then gravity follows the Bouguer-corrected gradient. When observations reveal departure from these predicted gradients, sub-surface and/or density changes are implied.
    Bottom: Residual gravity after estimated free-air gradient correction as a function of elevation. Normally, residual variations should follow the variations of the attraction of the topography.
    We clearly see that at Usu-Shinzan dome, these models do not explain the ecess of residual gravity, indicating an increase of density within the crypto-dome. We modelled the excess in gravity as a combination of underground water level rise by 1.5 m and the density Jousset et al., 1999).




    Eruption of 2000 at the western flank of Usu Volcano

    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.