Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/9795
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dc.contributor.authorallBignami, C.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione CNT, Roma, Italiaen
dc.contributor.authorallRuch, J.; Università Roma Treen
dc.contributor.authorallChini, M.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione CNT, Roma, Italiaen
dc.contributor.authorallNeri, M.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Catania, Catania, Italiaen
dc.contributor.authorallBuongiorno, M. F.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione CNT, Roma, Italiaen
dc.contributor.authorallHidayati, S.; CVGHMen
dc.contributor.authorallSayudi, D. S.; CVGHMen
dc.contributor.authorallSurono, N.; CVGHMen
dc.date.accessioned2015-06-08T08:23:05Zen
dc.date.available2015-06-08T08:23:05Zen
dc.date.issued2013en
dc.identifier.urihttp://hdl.handle.net/2122/9795en
dc.description.abstractPyroclastic density current deposits remobilized by water during periods of heavy rainfall trigger lahars (volcanic mudflows) that affect inhabited areas at considerable distance from volcanoes, even years after an eruption.Here we present an innovative approach to detect and estimate the thickness and volume of pyroclastic density current (PDC) deposits as well as erosional versus depositional environments. We use SAR interferometry to compare an airborne digital surface model (DSM) acquired in 2004 to a post eruption 2010 DSM created using COSMO-SkyMed satellite data to estimate the volume of 2010 Merapi eruption PDC deposits along the Gendol river (Kali Gendol, KG). Results show PDC thicknesses of up to 75 m in canyons and a volume of about 40 × 10^6 m3, mainly along KG, and at distances of up to 16 km from the volcano summit. This volume estimate corresponds mainly to the 2010 pyroclastic deposits along the KG — material that is potentially available to produce lahars. Our volume estimate is approximately twice that estimated by field studies, a difference we consider acceptable given the uncertainties involved in both satellite- and field-based methods. Our technique can be used to rapidly evaluate volumes of PDC deposits at active volcanoes, in remote settings and where continuous activity may prevent field observations.en
dc.language.isoEnglishen
dc.relation.ispartofJournal of Volcanology and Geothermal Researchen
dc.relation.ispartofseries/261 (2013)en
dc.subjectSAR interferometryen
dc.subjectDSM changeen
dc.subjectPyroclastic density currenten
dc.titlePyroclastic density current volume estimation after the 2010 Merapi volcano eruption using X-band SARen
dc.typearticleen
dc.description.statusPublisheden
dc.description.pagenumber236-243en
dc.subject.INGV04. Solid Earth::04.08. Volcanology::04.08.06. Volcano monitoringen
dc.subject.INGV04. Solid Earth::04.08. Volcanology::04.08.07. Instruments and techniquesen
dc.identifier.doi10.1016/j.jvolgeores.2013.03.023en
dc.description.obiettivoSpecifico5V. Sorveglianza vulcanica ed emergenzeen
dc.description.journalTypeJCR Journalen
dc.description.fulltextrestricteden
dc.contributor.authorBignami, C.en
dc.contributor.authorRuch, J.en
dc.contributor.authorChini, M.en
dc.contributor.authorNeri, M.en
dc.contributor.authorBuongiorno, M. F.en
dc.contributor.authorHidayati, S.en
dc.contributor.authorSayudi, D. S.en
dc.contributor.authorSurono, N.en
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione ONT, Roma, Italiaen
dc.contributor.departmentUniversità Roma Treen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione ONT, Roma, Italiaen
dc.contributor.departmentCVGHMen
dc.contributor.departmentCVGHMen
dc.contributor.departmentCVGHMen
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextrestricted-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione ONT, Roma, Italia-
crisitem.author.deptDipartimento Scienze Geologiche, Università Roma Tre, Roma, Italy-
crisitem.author.deptLuxembourg Institute of Science and Technology (LIST)-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione ONT, Roma, Italia-
crisitem.author.deptCVGHM-
crisitem.author.deptCVGHM-
crisitem.author.deptCVGHM-
crisitem.author.orcid0000-0002-8632-9979-
crisitem.author.orcid0000-0002-5890-3398-
crisitem.author.orcid0000-0002-6095-6974-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.classification.parent04. Solid Earth-
crisitem.classification.parent04. Solid Earth-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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