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dc.contributor.authorZelinger, Zdeněk
dc.contributor.authorBarret, Brice
dc.contributor.authorKubát, Pavel
dc.contributor.authorRicaud, Philippe
dc.contributor.authorAttie, Jean-Luc
dc.contributor.authorLe Flochmoën, Eric
dc.contributor.authorUrban, Joachim
dc.contributor.authorMurtagh, Donal
dc.contributor.authorStřižík, Michal
dc.date.accessioned2006-09-25T05:58:32Z
dc.date.available2006-09-25T05:58:32Z
dc.date.issued2006
dc.identifier.citationMolecular physics. 2006, vol. 104, no. 16-17, p. 2815 - 2820.en
dc.identifier.issn0026-8976
dc.identifier.issn1362-3028
dc.identifier.urihttp://hdl.handle.net/10084/56449
dc.description.abstractThe 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.isoenen
dc.publisherTaylor & Francisen
dc.relation.ispartofseriesMolecular physicsen
dc.relation.urihttp://dx.doi.org/10.1080/00268970600875380en
dc.titleObservation of HD18O, CH3OH and vibrationally-excited N2O from Odin/SMR measurementsen
dc.typearticleen
dc.identifier.locationNení ve fondu ÚKen
dc.identifier.doi10.1080/00268970600875380
dc.identifier.wos000240109000022


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