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Transition from effusive to explosive activity during lava dome eruption: the example of the 2010 eruption of Merapi volcano (Java, Indonesia)

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Transition from effusive to explosive activity during lava dome eruption: the example of the 2010 eruption of

Merapi volcano (Java, Indonesia)

Mélissa Drignon, Laurent Arbaret, Alain Burgisser, Jean-Christophe Komorowski, Caroline Martel, Radit Yaputra

To cite this version:

Mélissa Drignon, Laurent Arbaret, Alain Burgisser, Jean-Christophe Komorowski, Caroline Martel, et al.. Transition from effusive to explosive activity during lava dome eruption: the example of the 2010 eruption of Merapi volcano (Java, Indonesia). American Geophysical Union, Fall Meeting 2014, Dec 2014, San Francisco, United States. pp.abstract #V51B-4759. �insu-01386845�

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Transition from effusive to explosive activity during lava dome eruption: the example of the 2010 eruption of

Merapi volcano (Java, Indonesia)

Mélissa J Drignon1*, Laurent Arbaret1, Alain Burgisser1, Jean-Christophe Komorowski3, Caroline Martel1, Radit Yaputra4

email address: melissa.j.drignon@gmail.com 1 Institut des Sciences de la Terre d’Orléans (ISTO), CNRS, Université d’Orléans, BRGM, Orléans, France

2 ISTerre, Université de Savoie – CNRS, Chambéry, France

3 Institut de Physique du Globe de Paris, Sorbonne Paris Cité, Université Paris Diderot, Paris, France 4 Pusat Vulkanologi dan Mitigasi Bencana Geologi, CVGHM, Yogyjakarta, Indonesia

*Current Address: College of Earth, Ocean and Atmospheric Sciences, Oregon State University, Corvallis, OR, USA

We imaged the pumice of the two explo-sive events using the SEM at the Univer-sity of Orléans. The aim was then to be able to trace the plagioclase microlites ma-nually, and the oxides and bubbles automa-tically in order to obtain the glass propor-tion. At the same time, we obtained the bulk water content of the pumice using an Elemental Analyzer. We then combined these results to obtain the water content of the glass.

The first part of the model uses our textural analyses to obtain the initial pressures and porosi-ties of our samples.

Then, the second part of the model determines the initial depths of the samples based on these parameters.

2. Eruptive Depth and Pressure Model

We used the two-part eruptive depth and pressure model de-veloped in Burgisser et al. (2010; 2011) for the 88 Vulcanian explosions that occurred at Soufrière Hills (Montserrat) in 1997.

Temperature magma -chbr(°C) 950

ρmagma (kg,m-3) 2455

Pressuremagma -chbr (MPa) 300

XH2O max (%wt) 7,38

Merapi volcano (Java, Indonesia) is one of the most dangerous volcanoes on Earth. It is known to produce lava domes that collapse in deadly pyroclastic flows because of gravity or auto-explosivity. Even though this volcano is mostly effusive, explosive eruptions occur in its history, most recently in 2010. Two major explosive events occurred that year, the first one on October 26, and the second one on November 05. They produced explosive co-lumns that quickly collapsed in pumice-rich pyroclastic flows that ran up to 15.5 km from the summit. The 2010 eruption was very well observed, making this event a good candidate for investigating the effusive-explosive transition with a full suite of geochemical and geophysical data. The pumice of these two events was analyzed and the data used in a two-step computer model in order to investigate the pre-explosive conditions.

The explosive-effusive transition often occurs at arc volcanoes. The parameters driving this transition (overpressure, eruptive volume, . . .) are known but the relative importance of each parameter remains unclear. This study demonstrates the primacy of overpressure in determining the eruptive mode of the volcano, with volume and other parameters contributing only to the magnitude rather than the character of the event.

3. Results

5. Possible Eruptive Sequence

Before the explosive event of October 26, a cryptodome was growing in the south flank of the volcano. The pressure induced by this growth and the plug sealing the conduit generated a large overpressure (5- 20 MPa assuming elastic conduit walls) that led to the explosion. The explo-sion sampled the conduit to 11 km depth. The pyroclastic flow associated with this event was pumice-rich and ran up to 7 km from the summit.

On November 5, after several events, the system was probably semi-open to degassing. The ex-plosion sampled the conduit to a much shallower depth (up to 3 km) than on October 26. The pyroclastic flow associated ran up to 15.5 km from the summit.

It is interesting to consider why there were no stable eruptive columns for either event. The eruptive volumes were fairly small (6-10x106

m3). Small eruptive volumes can’t feed a stable

eruptive column, so this led to an early collapse. Eruptive volume is a key parameter for the crea-tion of a stable eruptive column, but does not in-fluence the explosive-effusive transition. The overpressure on the other hand has a major role. With a system closed to gas, it is possible to induce a large overpressure leading to an explo-sive eruption even at volcanoes that normally have effusive activity, such as Merapi.

Carbonate Assimilation ?

1. Analytical Study

4. Preliminary Source Depths

Reservoir depth: Costa et al. (2013) 2 mm 25 µm 0 50 100 150 200 250 300 350 400 450 0 1 2 3 4 5 6 7 P ( M P a ) % porosity

Pumice samples Max porosity if the total H2O= 7wt%

Minimal Syn-explosive expansion and no gass loss Maximal Syn-explosive expansion and gass loss

October 26, 2010

0 20 40 60 80 100 0 10 20 30 40 P ( M P a ) % porosity

Pumice Samples Max porosity if the total H2O= 7wt%

Minimal Syn-explosive expansion and no gass loss Maximal Syn-explosive expansion and gass loss

November 5, 2010

0 1 2 3 4 5 6 7 8 -13 -8 -3 2 7 12 17 D ep th s (k m )

Delta O18 ( ‰) AME 10 A (bulk) AME 10 B (bulk) AME 10 C (bulk) AME 10 E (bulk) AME 10 F (bulk) AME 10 G (bulk) AME 19 A (bulk) MER 13-01 (bulk) AME 10 F (magnetite) AME 10 G (magnetite) AME 19 A (magnetite) sea water

magmatic water / Merapi lavas (Troll et al, 2013)

Local Crust (limestone &

volcanoclastics_ Troll et al, 2003) Meteoric water (Cobb et al, 2007)

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