Variability of Martian water ice and dust vertical profiles with TGO/NOMAD
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Authors
Liuzzi, G.
Villanueva, G.L.
Crismani, M.M.J.
Smith, M.D.
Mumma, M.J.
Vandaele, A.C.
Aoki, S.
Daerden, F.
Thomas, I.R.
Lopez-Valverde, M.A.
Ristic, B.
Depiesse, C.
Willame, Y.
Holmes, J.A.
Lewis, S.
Oliva, F.
Hewson, W.
Patel, M.R.
Bellucci, G.
Lopez-Moreno, J.J.
the NOMAD Science team
Discipline
Physical sciences
Audience
Scientific
Date
2019Metadata
Show full item recordDescription
We 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.
Citation
Liuzzi, G.; Villanueva, G.L.; Crismani, M.M.J.; Smith, M.D.; Mumma, M.J.; Vandaele, A.C.; Aoki, S.; Daerden, F.; Thomas, I.R.; Lopez-Valverde, M.A.; Ristic, B.; Depiesse, C.; Willame, Y.; Holmes, J.A.; Lewis, S.; Oliva, F.; Hewson, W.; Patel, M.R.; Bellucci, G.; Lopez-Moreno, J.J.; the NOMAD Science team (2019). Variability of Martian water ice and dust vertical profiles with TGO/NOMAD. , EPSC-DPS Joint Meeting 2019, 15-20 September 2019, Geneva, Switzerland, Vol. 13, EPSC-DPS2019-743-1,Identifiers
Type
Conference
Peer-Review
No
Language
eng