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Simulating spectra of Jupiter’s atmosphere based on MAJIS VIS-NIR characteristics

dc.contributor.authorCisneros González, M.E.
dc.contributor.authorRobert, S.
dc.contributor.authorErwin, J.
dc.contributor.authorVandaele, A.C.
dc.contributor.authorLauzin, C.
dc.contributor.authorPoulet, F.
dc.contributor.authorPiccioni, G.
dc.date2021
dc.date.accessioned2021-10-13T05:29:36Z
dc.date.available2021-10-13T05:29:36Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/8041
dc.languageeng
dc.titleSimulating spectra of Jupiter’s atmosphere based on MAJIS VIS-NIR characteristics
dc.typeConference
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.source.titleEPSC Abstracts: Europlanet Science Congress 2021, 13 to 24 September 2021
dc.source.volume15
dc.source.pageEPSC2021-764
Orfeo.peerreviewedNo
dc.identifier.doi10.5194/epsc2021-764
dc.identifier.scopus


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