Home > Publications database > Chemical heating rates derived from SCIAMACHY vibrationally excited OH limb emission spectra > print

001     62638
005     20240911115604.0
024 7 _ |2 DOI
|a 10.1016/j.asr.2007.07.045
024 7 _ |2 WOS
|a WOS:000256847100022
037 _ _ |a PreJuSER-62638
041 _ _ |a eng
082 _ _ |a 520
084 _ _ |2 WoS
|a Engineering, Aerospace
084 _ _ |2 WoS
|a Astronomy & Astrophysics
084 _ _ |2 WoS
|a Geosciences, Multidisciplinary
084 _ _ |2 WoS
|a Meteorology & Atmospheric Sciences
100 1 _ |a Kaufmann, M.
|b 0
|u FZJ
|0 P:(DE-Juel1)129128
245 _ _ |a Chemical heating rates derived from SCIAMACHY vibrationally excited OH limb emission spectra
260 _ _ |a Amsterdam [u.a.]
|b Elsevier Science
|c 2008
300 _ _ |a 1914 - 1920
336 7 _ |a Journal Article
|0 PUB:(DE-HGF)16
|2 PUB:(DE-HGF)
336 7 _ |a Output Types/Journal article
|2 DataCite
336 7 _ |a Journal Article
|0 0
|2 EndNote
336 7 _ |a ARTICLE
|2 BibTeX
336 7 _ |a JOURNAL_ARTICLE
|2 ORCID
336 7 _ |a article
|2 DRIVER
440 _ 0 |a Advances in Space Research
|x 0273-1177
|0 9884
|y 11
|v 41
500 _ _ |a Record converted from VDB: 12.11.2012
520 _ _ |a The SCIAMACHY instrument on board Envisat is able to measure nearly all vibrational transitions of mesospheric hydroxyl-from the ultraviolet to the near infrared spectral region.In this paper, we analyze SCIAMACHY limb emission data in the 1000-1750 nm spectral region by means of a new vibrational non-LTE model of OH. Several hydroxyl hotbands are identified. Vibrational non-LTE model calculations applying different collisional relaxation models are able to reproduce the measured spectra. Best agreement between model calculations and measured spectra is obtained, if a combination of multiquantum and step ladder single-quantum relaxation model is applied. Emissions from the OH(nu = 9) vibrational state are used to derive chemical heating rates from the SCIAMACHY spectra. Instantaneous heating rates are in the order of 10 K/day. (c) 2007 COSPAR. Published by Elsevier Ltd. All rights reserved.
536 _ _ |a Atmosphäre und Klima
|c P22
|2 G:(DE-HGF)
|0 G:(DE-Juel1)FUEK406
|x 0
588 _ _ |a Dataset connected to Web of Science
650 _ 7 |a J
|2 WoSType
653 2 0 |2 Author
|a hydroxyl
653 2 0 |2 Author
|a mesosphere
653 2 0 |2 Author
|a SCIAMACHY
653 2 0 |2 Author
|a OH
653 2 0 |2 Author
|a heating rates
700 1 _ |a Lehmann, C.
|b 1
|u FZJ
|0 P:(DE-Juel1)156465
700 1 _ |a Hoffmann, L.
|b 2
|u FZJ
|0 P:(DE-Juel1)129125
700 1 _ |a Funke, B.
|b 3
|0 P:(DE-HGF)0
700 1 _ |a López-Puertas, M.
|b 4
|0 P:(DE-HGF)0
700 1 _ |a von Savigny, C.
|b 5
|0 P:(DE-HGF)0
700 1 _ |a Riese, M.
|b 6
|u FZJ
|0 P:(DE-Juel1)129145
773 _ _ |a 10.1016/j.asr.2007.07.045
|g Vol. 41, p. 1914 - 1920
|p 1914 - 1920
|q 41<1914 - 1920
|0 PERI:(DE-600)2023311-5
|t Advances in Space Research
|v 41
|y 2008
|x 0273-1177
856 7 _ |u http://dx.doi.org/10.1016/j.asr.2007.07.045
909 C O |o oai:juser.fz-juelich.de:62638
|p VDB
913 1 _ |k P22
|v Atmosphäre und Klima
|l Atmosphäre und Klima
|b Umwelt
|z fortgesetzt als P23
|0 G:(DE-Juel1)FUEK406
|x 0
914 1 _ |y 2008
915 _ _ |0 StatID:(DE-HGF)0010
|a JCR/ISI refereed
920 1 _ |k ICG-1
|l Stratosphäre
|d 30.09.2010
|g ICG
|0 I:(DE-Juel1)VDB790
|x 1
920 1 _ |k JARA-SIM
|l Jülich-Aachen Research Alliance - Simulation Sciences
|g JARA
|0 I:(DE-Juel1)VDB1045
|x 2
970 _ _ |a VDB:(DE-Juel1)99174
980 _ _ |a VDB
980 _ _ |a ConvertedRecord
980 _ _ |a journal
980 _ _ |a I:(DE-Juel1)IEK-7-20101013
980 _ _ |a I:(DE-Juel1)VDB1045
980 _ _ |a UNRESTRICTED
981 _ _ |a I:(DE-Juel1)ICE-4-20101013
981 _ _ |a I:(DE-Juel1)IEK-7-20101013
981 _ _ |a I:(DE-Juel1)VDB1045

LibraryCollectionCLSMajorCLSMinorLanguageAuthor
Marc 21