Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/27135
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | Ilyushin, Ya. A. | en_US |
dc.contributor.author | OROSEI, ROBERTO | en_US |
dc.contributor.author | Witasse, O. | en_US |
dc.contributor.author | Sánchez-Cano, B. | en_US |
dc.date.accessioned | 2020-09-04T10:18:13Z | - |
dc.date.available | 2020-09-04T10:18:13Z | - |
dc.date.issued | 2017 | en_US |
dc.identifier.issn | 0048-6604 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/27135 | - |
dc.description.abstract | In this paper we present the CLUtter SIMulator (CLUSIM), a special program simulating radar side echoes from rough planetary surfaces using realistic topography data sets. A numerical model of realistic topography of the Martian surface, based on Mars Orbiter Laser Altimeter data, is developed. A specially developed computer routine for evaluation of wideband radar echoes reflected from rough surfaces, capable of aperture synthesis simulation, is described. A synthetic radargram for a portion of Mars Express (MEX) orbit 9466 is computed and validated against experimental data obtained by the MARSIS radar instrument. Finally, a previously developed ionospheric phase correction procedure is numerically tested with new simulated echo signals. Impact of the surface clutter on the ionospheric correction procedure is investigated with a direct numerical comparison to a known benchmark result, which shows robustness of the correction algorithm with respect to the surface clutter. | en_US |
dc.language.iso | eng | en_US |
dc.title | CLUSIM: A Synthetic Aperture Radar Clutter Simulator for Planetary Exploration | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1002/2017RS006265 | en_US |
dc.identifier.scopus | 2-s2.0-85031732564 | en_US |
dc.identifier.isi | 000428024200013 | en_US |
dc.identifier.url | https://agupubs.onlinelibrary.wiley.com/doi/full/10.1002/2017RS006265 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 52 | en_US |
dc.relation.issue | 9 | en_US |
dc.relation.firstpage | 1200 | en_US |
dc.relation.lastpage | 1213 | en_US |
dc.relation.numberofpages | 14 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.numberofauthors | 4 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | FRA | en_US |
dc.contributor.country | ESP | en_US |
dc.contributor.country | RUS | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | RADIO SCIENCE | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2017RaSc...52.1200I | en_US |
dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.openairetype | Article | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | IRA Bologna | - |
crisitem.author.orcid | 0000-0003-1277-1294 | - |
crisitem.journal.journalissn | 0048-6604 | - |
crisitem.journal.ance | E140811 | - |
È visualizzato nelle collezioni: | 1.01 Articoli in rivista |
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File | Descrizione | Dimensioni | Formato | |
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ilyushin_et_al_2017.pdf | Pdf editoriale | 1.98 MB | Adobe PDF | Visualizza/apri |
Witasse2017RSfinal.pdf | preprint | 5.86 MB | Adobe PDF | Visualizza/apri |
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