Reference : The distributions of the OH (Δv=1) and (Δv=2) emissions on the Venus nightside
Scientific congresses and symposiums : Unpublished conference
Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics
http://hdl.handle.net/2268/111307
The distributions of the OH (Δv=1) and (Δv=2) emissions on the Venus nightside
English
Soret, Lauriane mailto [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Labo de physique atmosphérique et planétaire (LPAP) >]
Gérard, Jean-Claude mailto [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Département d'astrophys., géophysique et océanographie (AGO) >]
Piccioni, Giuseppe [ > > ]
Drossart, Pierre [ > > ]
Sep-2010
No
International
EPSC
Rome
Italie
[en] Venus ; OH
[en] The presence of OH was detected in the spectrum of the Venus mesosphere observed at the limb with the VIRTIS instrument on board the Venus Express spacecraft [3]. The (1-0) and (2-1) transitions at 2.80 and 2.94 mm, respectively and the (2-0) band at 1.43 mm were clearly identified. The results of this study show that a correlation is observed between the emissions associated to the Δv=1 and the Δv=2 sequences.
Researchers ; Professionals ; Students
http://hdl.handle.net/2268/111307

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