Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/3229
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dc.contributor.authorallBruno, V.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Catania, Catania, Italiaen
dc.contributor.authorallAloisi, M.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Catania, Catania, Italiaen
dc.contributor.authorallBonforte, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Catania, Catania, Italiaen
dc.contributor.authorallImmè, G.; Università degli Studi di Catania, Dipartimento di Fisica e Astronomiaen
dc.contributor.authorallPuglisi, G.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Catania, Catania, Italiaen
dc.date.accessioned2007-12-13T14:59:27Zen
dc.date.available2007-12-13T14:59:27Zen
dc.date.issued2007-04-02en
dc.identifier.urihttp://hdl.handle.net/2122/3229en
dc.description.abstractDue to the prominent topography of Mt. Etna, the use of satellite geodetic techniques may significantly suffer from atmospheric heterogeneities. This problem mainly affects the DInSAR technique. To overcome these drawbacks the present study attempts to make headway in measuring and interpreting atmospheric anomalies. We used the GAMIT software to obtain the ZTD (Zenith Total Delay) values for the GPS sessions performed on 1996-97, during ERS-2 passes at Mt. Etna. GAMIT software also allows to characterize the statistical behaviour of the tropospheric effects, by using residuals for each station-satellite pair, and to locate the atmospheric anomalies, present mostly at low altitudes. The attempt at using these results to produce a tomography of radio waves velocity of the troposphere suggests that the number of GPS stations used to investigate atmosphere is a critical point in such a study. The three stations are too few to invert anomalies eventually existing in the lower atmosphere. This result is a good starting point for better direct future study to verify the applicability of this tomographic technique to a geodetic network with a higher number of stations, with the aim of characterizing the lower atmosphere of Mt. Etna for a more accurate monitoring of ground deformations.en
dc.language.isoEnglishen
dc.publisher.nameIstituto Nazionale di Geofisica e Vulcanologiaen
dc.relation.ispartofAnnals of Geophysicsen
dc.relation.ispartofseries2/50 (2007)en
dc.subjectGPSen
dc.subjectatmospheric anomaliesen
dc.subjecttropospheric delaysen
dc.subjecttomography of radio wave velocitiesen
dc.titleAtmospheric anomalies over Mt.Etna using GPS signal delays and tomography of radio wave velocitiesen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber267-282en
dc.subject.INGV04. Solid Earth::04.03. Geodesy::04.03.07. Satellite geodesyen
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CLARKE (2002): Atmospheric models, GPS and InSAR measurements of the tropospheric water vapour field over Mount Etna, Geophysical Research Letters, 29, no. 19, 1905. WEBLEY, P.W., R.M. BINGLEY, A.H. DODSON, G. WADGE, S.J. WAUGH, I.N. JAMES (2002): Atmospheric water vapour correction to InSAR surface motion measurements on mountains: results from a dense GPS network on Mount Etna, Physics and Chemistry of the Earth, 27, 363-370. WILLIAMS, S., Y. BOCH, P. FANG (1998): Integrated satellite interferometry: tropospheric noise, GPS estimates and implications for interferometric synthetic aperture radar products, Journal of Geophysical Research, 103, no. B11, 27, 051-27, 067.en
dc.description.obiettivoSpecifico1.3. TTC - Sorveglianza geodetica delle aree vulcaniche attiveen
dc.description.journalTypeJCR Journalen
dc.description.fulltextopenen
dc.contributor.authorBruno, V.en
dc.contributor.authorAloisi, M.en
dc.contributor.authorBonforte, A.en
dc.contributor.authorImmè, G.en
dc.contributor.authorPuglisi, G.en
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italiaen
dc.contributor.departmentUniversità degli Studi di Catania, Dipartimento di Fisica e Astronomiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italiaen
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.deptDipartimento di Fisica e Astronomia - Università degli studi di Catania – Via S. Sofia, 64, 95123 Catania-Italy-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italia-
crisitem.author.orcid0000-0001-7803-5404-
crisitem.author.orcid0000-0002-9945-4138-
crisitem.author.orcid0000-0003-0435-7763-
crisitem.author.orcid0000-0003-4503-5808-
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.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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