Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/12327
DC FieldValueLanguage
dc.date.accessioned2019-02-27T10:59:05Zen
dc.date.available2019-02-27T10:59:05Zen
dc.date.issued2018en
dc.identifier.urihttp://hdl.handle.net/2122/12327en
dc.description.abstractAn inversion methodology, named maximum likelihood (ML) volcanic ash light detection and ranging (Lidar) retrieval (VALR-ML), has been developed and applied to estimate volcanic ash particle size and ash mass concentration within volcanic plumes. Both estimations are based on the ML approach, trained by a polarimetric backscattering forward model coupled with a Monte Carlo ash microphysical model. The VALR-ML approach is applied to Lidar backscattering and depolarization profiles, measured at visible wavelength during two eruptions of Mt. Etna, Catania, Italy, in 2010 and 2011. The results are compared with those of ash products derived from other parametric retrieval algorithms. A detailed comparison among these different retrieval techniques highlights the potential of VALR-ML to determine, on the basis of a physically consistent approach, the ash cloud area that must be interdicted to flight operations. Moreover, the results confirm the usefulness of operating scanning Lidars near active volcanic vents.en
dc.language.isoEnglishen
dc.relation.ispartofIEEE Transactions on Geoscience and Remote Sensingen
dc.relation.ispartofseries/56 (2018)en
dc.titleMaximum-Likelihood Retrieval of Volcanic Ash Concentration and Particle Size From Ground-Based Scanning Lidaren
dc.typearticleen
dc.description.statusPublisheden
dc.description.pagenumber5824 - 5842en
dc.identifier.doi10.1109/TGRS.2018.2826839en
dc.description.obiettivoSpecifico5V. Processi eruttivi e post-eruttivien
dc.description.journalTypeJCR Journalen
dc.contributor.authorMereu, Luigien
dc.contributor.authorScollo, Simonaen
dc.contributor.authorMori, Saverioen
dc.contributor.authorBoselli, Antonellaen
dc.contributor.authorLeto, Giuseppeen
dc.contributor.authorMarzano, Frank S.en
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italiaen
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 Bologna, Bologna, Italia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italia-
crisitem.author.deptCNISM and IMAA-CNR-
crisitem.author.deptOsservatorio Astrofisico di Catania, INAF,-
crisitem.author.orcid0000-0003-0303-1171-
crisitem.author.orcid0000-0001-8704-8629-
crisitem.author.orcid0000-0002-3392-8687-
crisitem.author.orcid0000-0002-4996-7648-
crisitem.author.orcid0000-0002-0040-5011-
crisitem.author.orcid0000-0002-5873-204X-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
Appears in Collections:Article published / in press
Files in This Item:
File Description SizeFormat Existing users please Login
Mereuetal_2018.pdf40.72 MBAdobe PDF
Show simple item record

WEB OF SCIENCETM
Citations 50

5
checked on Feb 7, 2021

Page view(s)

215
checked on Apr 27, 2024

Download(s)

2
checked on Apr 27, 2024

Google ScholarTM

Check

Altmetric