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  1. OA@INAF
  2. PRODOTTI RICERCA INAF
  3. 1 CONTRIBUTI IN RIVISTE (Journal articles)
  4. 1.01 Articoli in rivista
Please use this identifier to cite or link to this item: http://hdl.handle.net/20.500.12386/30092
DC FieldValueLanguage
dc.contributor.authorWOLKENBERG, PAULINA MARIAen_US
dc.contributor.authorGIURANNA, MARCOen_US
dc.contributor.authorGRASSI, Davideen_US
dc.contributor.authorARONICA, Alessandroen_US
dc.contributor.authorAoki, Shoheien_US
dc.contributor.authorScaccabarozzi, Diegoen_US
dc.contributor.authorSaggin, Bortolinoen_US
dc.date.accessioned2021-01-28T17:09:15Z-
dc.date.available2021-01-28T17:09:15Z-
dc.date.issued2018en_US
dc.identifier.issn0019-1035en_US
dc.identifier.urihttp://hdl.handle.net/20.500.12386/30092-
dc.description.abstractWe present spatial and temporal distributions of dust on Mars from Ls = 331° in MY 26 until Ls = 80° in MY33 retrieved from the measurements taken by the Planetary Fourier Spectrometer (PFS) aboard Mars Express. In agreement with previous observations, large dust opacity is observed mostly in the southern hemisphere spring/summer and particularly over regions of higher terrain and large topographic variation. We present a comparison with dust opacities obtained from Thermal Emission Spectrometer (TES) - Mars Global Surveyor (MGS) measurements. We found good consistency between observations of two instruments during overlapping interval (Ls = 331° in MY 26 until Ls = 77° in MY 27). We found a different behavior of the dust opacity with latitude in the various Martian years (inter-annual variations). A global dust storm occurred in MY 28. We observe a different spatial distribution, a later occurrence and dissipation of the dust maximum activity in MY 28 than in other Martian years. A possible precursor signal to the global dust storm in MY 28 is observed at Ls = 200°-235° especially over west Hellas. Heavy dust loads alter atmospheric temperatures. Due to the absorption of solar radiation and emission of infrared radiation to space by dust vertically non-uniformly distributed, a strong heating of high atmospheric levels (40-50 km) and cooling below ∼30 km are observed.en_US
dc.language.isoengen_US
dc.titleCharacterization of dust activity on Mars from MY27 to MY32 by PFS-MEX observationsen_US
dc.typeArticle-
dc.identifier.doi10.1016/j.icarus.2017.10.045en_US
dc.identifier.scopus2-s2.0-85033395426en_US
dc.identifier.isi000432763100003en_US
dc.identifier.urlhttp://arxiv.org/abs/1802.02653v1en_US
dc.identifier.urlhttps://www.sciencedirect.com/science/article/abs/pii/S0019103517301926?via%3Dihuben_US
dc.relation.mediumSTAMPAen_US
dc.relation.volume310en_US
dc.relation.firstpage32en_US
dc.relation.lastpage47en_US
dc.type.refereeREF_1en_US
dc.description.internationalsìen_US
dc.contributor.countryITAen_US
dc.contributor.countryBELen_US
dc.contributor.countryJPNen_US
dc.contributor.countryPOLen_US
dc.relation.scientificsectorFIS/05 - ASTRONOMIA E ASTROFISICAen_US
dc.relation.journalICARUSen_US
dc.type.miur262 Articolo in rivista-
dc.identifier.adsbibcode2018Icar..310...32Wen_US
dc.relation.ercsectorERC 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::PE9_2 Planetary systems sciencesen_US
dc.description.apcnoen_US
dc.description.oa1 – prodotto con file in versione Open Access (allegare il file al passo  5-Carica)en_US
item.grantfulltextopen-
item.languageiso639-1en-
item.fulltextWith Fulltext-
item.openairetypeArticle-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.cerifentitytypePublications-
crisitem.journal.journalissn0019-1035-
crisitem.journal.anceE079353-
crisitem.author.deptIAPS Roma-
crisitem.author.deptIAPS Roma-
crisitem.author.deptIAPS Roma-
crisitem.author.deptIAPS Roma-
crisitem.author.orcid0000-0001-6769-3719-
crisitem.author.orcid0000-0001-8967-9184-
crisitem.author.orcid0000-0003-1653-3066-
crisitem.author.orcid0000-0003-3205-9472-
Appears in Collections:1.01 Articoli in rivista
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Dust_arxiv_with_figures.pdfpreprint8.23 MBAdobe PDFView/Open
Characterization-of-dust-activity-on-Mars-from-MY27-to-MY32-by-PFS_2018_Icar.pdf[Administrators only]8.79 MBAdobe PDF
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