Observation of HD18O, CH3OH and vibrationally-excited N2O from Odin/SMR measurements

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dc.contributor.author Zelinger, Zdeněk
dc.contributor.author Barret, Brice
dc.contributor.author Kubát, Pavel
dc.contributor.author Ricaud, Philippe
dc.contributor.author Attie, Jean-Luc
dc.contributor.author Le Flochmoën, Eric
dc.contributor.author Urban, Joachim
dc.contributor.author Murtagh, Donal
dc.contributor.author Střižík, Michal
dc.date.accessioned 2006-09-25T05:58:32Z
dc.date.available 2006-09-25T05:58:32Z
dc.date.issued 2006
dc.identifier.citation Molecular physics. 2006, vol. 104, no. 16-17, p. 2815 - 2820. en
dc.identifier.issn 0026-8976
dc.identifier.issn 1362-3028
dc.identifier.uri http://hdl.handle.net/10084/56449
dc.description.abstract The sub-millimetre radiometer (SMR) instrument aboard the Odin satellite launched in February 2001 is dedicated to the observation of trace gas profiles in the stratosphere and in the mesosphere, in particular water vapour and its isotopic species HDO, H217O and H218O. By averaging more than 400 000 Odin/SMR spectra over the period from November 2002 to March 2003, weak lines have been detected in the atmosphere. These weak lines have been attributed to water isotopic species HD18O, to a vibrationally-excited N2O, and to CH3OH. en
dc.language.iso en en
dc.publisher Taylor & Francis en
dc.relation.ispartofseries Molecular physics en
dc.relation.uri http://dx.doi.org/10.1080/00268970600875380 en
dc.title Observation of HD18O, CH3OH and vibrationally-excited N2O from Odin/SMR measurements en
dc.type Article en
dc.identifier.location Není ve fondu ÚK en
dc.identifier.doi 10.1080/00268970600875380
dc.identifier.wos 000240109000022

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