Reference : The distributions of the OH (Δv=1) and (Δv=2) emissions on the Venus nightside

	Document type :	Scientific congresses and symposiums : Unpublished conference
	Discipline(s) :	Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics
	To cite this reference:	http://hdl.handle.net/2268/111307

Title :	The distributions of the OH (Δv=1) and (Δv=2) emissions on the Venus nightside
Language :	English
Author, co-author :	Soret, Lauriane [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Labo de physique atmosphérique et planétaire (LPAP) >]
	Gérard, Jean-Claude [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Département d'astrophys., géophysique et océanographie (AGO) >]
	Piccioni, Giuseppe [ > > ]
	Drossart, Pierre [ > > ]
Publication date :	Sep-2010
Audience :	International
Event name :	EPSC
Event place (city) :	Rome
Event country :	Italie
Keywords :	[en] Venus ; OH
Abstract :	[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.
Target :	Researchers ; Professionals ; Students
Permalink :	http://hdl.handle.net/2268/111307

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