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Variability of Martian water ice and dust vertical profiles with TGO/NOMAD

dc.contributor.authorLiuzzi, G.
dc.contributor.authorVillanueva, G.L.
dc.contributor.authorCrismani, M.M.J.
dc.contributor.authorSmith, M.D.
dc.contributor.authorMumma, M.J.
dc.contributor.authorVandaele, A.C.
dc.contributor.authorAoki, S.
dc.contributor.authorDaerden, F.
dc.contributor.authorThomas, I.R.
dc.contributor.authorLopez-Valverde, M.A.
dc.contributor.authorRistic, B.
dc.contributor.authorDepiesse, C.
dc.contributor.authorWillame, Y.
dc.contributor.authorHolmes, J.A.
dc.contributor.authorLewis, S.
dc.contributor.authorOliva, F.
dc.contributor.authorHewson, W.
dc.contributor.authorPatel, M.R.
dc.contributor.authorBellucci, G.
dc.contributor.authorLopez-Moreno, J.J.
dc.contributor.authorthe NOMAD Science team
dc.date2019
dc.date.accessioned2020-03-29T16:11:57Z
dc.date.available2020-03-29T16:11:57Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/7488
dc.descriptionWe present the first results of water ice and dust microphysical properties derived from the Nadir and Occultation for Mars Discovery (NOMAD) instrument, onboard ExoMars Trace Gas Orbiter (TGO). These retrievals are derived from vertical profiles that span the entire science phase so far, which began April 21st, 2018.
dc.languageeng
dc.titleVariability of Martian water ice and dust vertical profiles with TGO/NOMAD
dc.typeConference
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.source.titleEPSC-DPS Joint Meeting 2019, 15-20 September 2019, Geneva, Switzerland
dc.source.volume13
dc.source.pageEPSC-DPS2019-743-1
Orfeo.peerreviewedNo


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