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Understanding the variability of nightside temperatures, NO UV and O 2 IR nightglow emissions in the Venus upper atmosphere
dc.contributor.authorBrecht, A. S.en_US
dc.contributor.authorBougher, S. W.en_US
dc.contributor.authorGérard, J. ‐c.en_US
dc.contributor.authorParkinson, C. D.en_US
dc.contributor.authorRafkin, S.en_US
dc.contributor.authorFoster, B.en_US
dc.date.accessioned2013-01-03T19:42:08Z
dc.date.available2013-01-03T19:42:08Z
dc.date.issued2011-08en_US
dc.identifier.citationBrecht, A. S.; Bougher, S. W.; Gérard, J. ‐c. ; Parkinson, C. D.; Rafkin, S.; Foster, B. (2011). "Understanding the variability of nightside temperatures, NO UV and O 2 IR nightglow emissions in the Venus upper atmosphere." Journal of Geophysical Research: Planets 116(E8): n/a-n/a. <http://hdl.handle.net/2027.42/95269>en_US
dc.identifier.issn0148-0227en_US
dc.identifier.issn2156-2202en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/95269
dc.publisherWiley Periodicals, Inc.en_US
dc.publisherChem. Rubber Co. Pressen_US
dc.subject.otherThermosphereen_US
dc.subject.otherVenusen_US
dc.subject.otherAirglowen_US
dc.subject.otherAtmosphereen_US
dc.subject.otherCompositionen_US
dc.titleUnderstanding the variability of nightside temperatures, NO UV and O 2 IR nightglow emissions in the Venus upper atmosphereen_US
dc.typeArticleen_US
dc.rights.robotsIndexNoFollowen_US
dc.subject.hlbsecondlevelGeological Sciencesen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/95269/1/jgre2911.pdf
dc.identifier.doi10.1029/2010JE003770en_US
dc.identifier.sourceJournal of Geophysical Research: Planetsen_US
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