Widiyantoro S. auteur aut IRD Ramdhan M. auteur aut IRD Métaxian Jean-Philippe auteur aut IRD Cummins P. R. auteur aut IRD Martel C. auteur aut IRD Erdmann S. auteur aut IRD Nugraha A. D. auteur aut IRD Budi-Santoso A. auteur aut IRD Laurin Antoine auteur aut IRD Fahmi A. A. auteur aut IRD text journalArticle eng text/pdf reformatted digital access Our seismic tomographic images characterize, for the first time, spatial and volumetric details of the subvertical magma plumbing system of Merapi Volcano. We present P-and S-wave arrival time data, which were collected in a dense seismic network, known as DOMERAPI, installed around the volcano for 18 months. The P-and S-wave arrival time data with similar path coverage reveal a high Vp/Vs structure extending from a depth of >= 20 km below mean sea level (MSL) up to the summit of the volcano. Combined with results of petrological studies, our seismic tomography data allow us to propose: (1) the existence of a shallow zone of intense fluid percolation, directly below the summit of the volcano; (2) a main, pre-eruptive magma reservoir at >= 10 to 20 km below MSL that is orders of magnitude larger than erupted magma volumes; (3) a deep magma reservoir at MOHO depth which supplies the main reservoir; and (4) an extensive, subvertical fluid-magma-transfer zone from the mantle to the surface. Such high-resolution spatial constraints on the volcano plumbing system as shown are an important advance in our ability to forecast and to mitigate the hazard potential of Merapi's future eruptions. specialized INDONESIE 066 064 8 art. 13656 [7p.] 2018 2045-2322 https://www.documentation.ird.fr/hor/fdi:010074033 10.1038/s41598-018-31293-w 2045-2322 [F B010074033] https://www.documentation.ird.fr/hor/fdi:010074033 https://horizon.documentation.ird.fr/exl-doc/pleins_textes/divers18-09/010074033.pdf IRD - Base Horizon / Pleins textes 2018-10-03 2023-07-11 fdi:010074033 fre