Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/16093
DC FieldValueLanguage
dc.date.accessioned2023-02-02T10:13:36Z-
dc.date.available2023-02-02T10:13:36Z-
dc.date.issued2022-
dc.identifier.urihttp://hdl.handle.net/2122/16093-
dc.description.abstractSpaceborne detection and measurements of high-temperature thermal anomalies enable monitoring and forecasts of lava flow propagation. The accuracy of such thermal estimates relies on the knowledge of input parameters, such as emissivity, which notably affects computation of temperature, radiant heat flux, and subsequent analyses (e.g., effusion rate and lava flow distance to run) that rely on the accuracy of observations. To address the deficit of field and laboratory-based emissivity data for inverse and forward modelling, we measured the emissivity of ‘a’a lava samples from the 2001 Mt. Etna eruption, over the wide range of temperatures (773 to 1373 K) and wavelengths (2.17 to 21.0 µm). The results show that emissivity is not only wavelength dependent, but it also increases non-linearly with cooling, revealing considerably lower values than those typically assumed for basalts. This new evidence showed the largest and smallest increase in average emissivity during cooling in the MIR and TIR regions (~30% and ~8% respectively), whereas the shorter wavelengths of the SWIR region showed a moderate increase (~15%). These results applied to spaceborne data confirm that the variable emissivity-derived radiant heat flux is greater than the constant emissivity assumption. For the differences between the radiant heat flux in the case of variable and constant emissivity, we found the median value is 0.06, whereas the 25th and the 75th percentiles are 0.014 and 0.161, respectively. This new evidence has significant impacts on the modelling of lava flow simulations, causing a dissimilarity between the two emissivity approaches of ~16% in the final area and ~7% in the maximum thickness. The multicomponent emissivity input provides means for ‘best practice’ scenario when accurate data required. The novel approach developed here can be used to test an improved version of existing multi-platform, multi-payload volcano monitoring systems.en_US
dc.language.isoEnglishen_US
dc.publisher.nameMDPIen_US
dc.relation.ispartofRemote Sensingen_US
dc.relation.ispartofseries/14 (2022)en_US
dc.rightsCC0 1.0 Universal*
dc.rights.urihttp://creativecommons.org/publicdomain/zero/1.0/*
dc.titleThe Impact of Dynamic Emissivity–Temperature Trends on Spaceborne Data: Applications to the 2001 Mount Etna Eruptionen_US
dc.typearticleen
dc.description.statusPublisheden_US
dc.type.QualityControlPeer-revieweden_US
dc.description.pagenumber1641en_US
dc.identifier.doi10.3390/rs14071641en_US
dc.description.obiettivoSpecifico3V. Proprietà chimico-fisiche dei magmi e dei prodotti vulcanicien_US
dc.description.obiettivoSpecifico5V. Processi eruttivi e post-eruttivien_US
dc.description.obiettivoSpecifico6V. Pericolosità vulcanica e contributi alla stima del rischioen_US
dc.description.journalTypeJCR Journalen_US
dc.relation.issn2072-4292en_US
dc.contributor.authorRogic, Nikola-
dc.contributor.authorBilotta, Giuseppe-
dc.contributor.authorGanci, Gaetana-
dc.contributor.authorThompson, James-
dc.contributor.authorCappello, Annalisa-
dc.contributor.authorRymer, Hazel-
dc.contributor.authorRamsey, Michael-
dc.contributor.authorFerrucci, Fabrizio-
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italiaen_US
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italiaen_US
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italiaen_US
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextopen-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italia-
crisitem.author.deptDepartment of Geology and Planetary Science, University of Pittsburgh, Pittsburgh, PA, USA-
crisitem.author.orcid0000-0002-2850-2358-
crisitem.author.orcid0000-0002-1406-4545-
crisitem.author.orcid0000-0002-9914-1107-
crisitem.author.orcid0000-0003-4540-5717-
crisitem.author.orcid0000-0002-9947-8789-
crisitem.author.orcid0000-0003-3949-1129-
crisitem.author.orcid0000-0002-8092-7409-
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.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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