Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/6032
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dc.contributor.authorallCorradini, S.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione CNT, Roma, Italiaen
dc.contributor.authorallTirelli, C.; Università La Sapienza Romaen
dc.contributor.authorallGangale, G.; Università di Modena e Reggio Emiliaen
dc.contributor.authorallPugnaghi, Sergio; Università di Modena e Reggio Emiliaen
dc.contributor.authorallCarboni, E.; Atmospheric, Oceanic, and Planetary Physics, Atmospheric, Oceanic, and Planetary Physics, Clarendon Laboratory, University of Oxforden
dc.date.accessioned2010-06-08T12:00:40Zen
dc.date.available2010-06-08T12:00:40Zen
dc.date.issued2010-03en
dc.identifier.urihttp://hdl.handle.net/2122/6032en
dc.description.abstractIn this paper, a sensitivity analysis and procedure development for volcanic-plume sulfur dioxide and ash retrievals using ground thermal infrared camera have been carried out. The semiconductor device camera, considered as a reference, has a spectral range of 8–14 μm with noise equivalent temperature difference that is better than 100 mK at 300 K. The camera will be used to monitor and assess the hazards of Mt. Etna volcano to mitigate the risk and impact of volcanic eruptions on the civil society and transports. A minimum number of filters have been selected for sulfur dioxide (SO2) and volcanic ash retrievals. The sensitivity study has been carried out to determine the SO2 and volcanic ash minimum concentration detectable by the system varying the camera geometry and the atmospheric profiles. Results show a meaningful sensitivity increase considering high instrument altitudes and low camera-elevation angles. For all geometry configurations and monthly profiles, the sensitivity limit varies between 0.5 and 2 g · m−2 for SO2 columnar abundance and between 0.02 and 1 for ash optical depth. Two procedures to detect SO2 and ash, based on the least square fit method and on the brightness temperature difference (BTD) algorithm, respectively, have also been proposed. Results show that high concentration of atmospheric water vapor columnar content significantly reduces the ash-plume effect on the BTD. A water vapor-correction procedure introduced improves the ash retrievals and the cloud discrimination in every season, considering all the camera geometries.en
dc.language.isoEnglishen
dc.publisher.nameIEEE Geoscience and Remote Sensing Societyen
dc.relation.ispartofIEEE Transactions on Geoscience and Remote Sensingen
dc.relation.ispartofseries3/48 (2010)en
dc.subjectRemote sensingen
dc.subjectTIR-cameraen
dc.subjectground measurementsen
dc.subjectsulphur dioxideen
dc.subjectvolcanic ashen
dc.subjectMt. Etna Mt. Etna volcanoen
dc.titleTheoretical study on SO2 and ash volcanic plume retrievals using ground TIR camera. Sensitivity analysis and retrieval procedure developmentsen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber1619-1628en
dc.subject.INGV04. Solid Earth::04.08. Volcanology::04.08.01. Gasesen
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.subject.INGV04. Solid Earth::04.08. Volcanology::04.08.08. Volcanic risken
dc.subject.INGV05. General::05.02. Data dissemination::05.02.03. Volcanic eruptionsen
dc.identifier.doi10.1109/TGRS.2009.2032242en
dc.description.obiettivoSpecifico1.5. TTC - Sorveglianza dell'attività eruttiva dei vulcanien
dc.description.obiettivoSpecifico1.10. TTC - Telerilevamentoen
dc.description.journalTypeJCR Journalen
dc.description.fulltextreserveden
dc.contributor.authorCorradini, S.en
dc.contributor.authorTirelli, C.en
dc.contributor.authorGangale, G.en
dc.contributor.authorPugnaghi, Sergioen
dc.contributor.authorCarboni, E.en
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione ONT, Roma, Italiaen
dc.contributor.departmentUniversità La Sapienza Romaen
dc.contributor.departmentUniversità di Modena e Reggio Emiliaen
dc.contributor.departmentUniversità di Modena e Reggio Emiliaen
dc.contributor.departmentAtmospheric, Oceanic, and Planetary Physics, Atmospheric, Oceanic, and Planetary Physics, Clarendon Laboratory, University of Oxforden
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.deptUniversità La Sapienza Roma-
crisitem.author.deptUniversità di Modena e Reggio Emilia-
crisitem.author.deptUniversità di Modena e Reggio Emilia-
crisitem.author.orcid0000-0001-9432-3246-
crisitem.author.orcid0000-0002-0236-7856-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.classification.parent04. Solid Earth-
crisitem.classification.parent04. Solid Earth-
crisitem.classification.parent04. Solid Earth-
crisitem.classification.parent04. Solid Earth-
crisitem.classification.parent05. General-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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