001     40885
005     20240911115615.0
024 7 _ |2 DOI
|a 10.1016/j.asr.2003.02.041
024 7 _ |2 WOS
|a WOS:000225594400012
037 _ _ |a PreJuSER-40885
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 Grossmann, K. U.
|b 0
|0 P:(DE-HGF)0
245 _ _ |a A review of the scientific results from the CRISTA missions
260 _ _ |a Amsterdam [u.a.]
|b Elsevier Science
|c 2004
300 _ _ |a 1715 - 1721
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 8
|v 34
500 _ _ |a Record converted from VDB: 12.11.2012
520 _ _ |a The CRyogenic Infrared Spectrometers and Telescopes for the Atmosphere (CRISTA) experiment measured atmospheric limb infrared emissions in the altitude regime from the upper troposphere to the lower thermosphere during two Shuttle missions in November 1994 and August 1997. From the recorded spectra trace gas densities and temperature fields were derived on a very dense spatial grid. In the mesosphere and lower thermosphere trace gas and temperature retrievals were carried out with the help of a state of the art non-LTE (non-local thermodynamic equilibrium) model coupled to a line-by-line radiative transfer code. The upper atmosphere data include densities of carbon dioxide, ozone, atomic oxygen, and temperature. All parameters were derived for day and night with the exception of CO2 which is available for daytime only. Additional trace gases in the mesosphere include water vapor, methane, and carbon monoxide. The main findings are a substantial depletion of CO2 between 80 and 100 km, high ozone concentrations in the secondary maximum (upper mesosphere) during night, a tertiary ozone maximum near the winter polar terminator in the middle mesosphere and well developed dynamically induced structures in latitude as well as in longitude. Such structures are also observed in the lower thermosphere where the distribution of atomic oxygen was measured up to about 180 km altitude. The atomic oxygen concentrations encountered in the thermosphere during solar minimum are much lower than predicted by MSIS. (C) 2004 COSPAR. Published by Elsevier Ltd. All rights reserved.
536 _ _ |a Chemie und Dynamik der Geo-Biosphäre
|c U01
|2 G:(DE-HGF)
|0 G:(DE-Juel1)FUEK257
|x 0
588 _ _ |a Dataset connected to Web of Science
650 _ 7 |a S
|2 WoSType
653 2 0 |2 Author
|a CRISTA missions
653 2 0 |2 Author
|a atmospheric limb infrared emission
653 2 0 |2 Author
|a mesospheric trace gases and temperatures
700 1 _ |a Gusev, O.
|b 1
|0 P:(DE-HGF)0
700 1 _ |a Kaufmann, M.
|b 2
|u FZJ
|0 P:(DE-Juel1)129128
700 1 _ |a Kutepov, A.
|b 3
|0 P:(DE-HGF)0
700 1 _ |a Knieling, P.
|b 4
|0 P:(DE-HGF)0
773 _ _ |a 10.1016/j.asr.2003.02.041
|g Vol. 34, p. 1715 - 1721
|p 1715 - 1721
|q 34<1715 - 1721
|0 PERI:(DE-600)2023311-5
|t Advances in space research
|v 34
|y 2004
|x 0273-1177
856 7 _ |u http://dx.doi.org/10.1016/j.asr.2003.02.041
909 C O |o oai:juser.fz-juelich.de:40885
|p VDB
913 1 _ |k U01
|v Chemie und Dynamik der Geo-Biosphäre
|l Chemie und Dynamik der Geo-Biosphäre
|b Environment (Umwelt)
|0 G:(DE-Juel1)FUEK257
|x 0
914 1 _ |y 2004
915 _ _ |0 StatID:(DE-HGF)0010
|a JCR/ISI refereed
920 1 _ |k ICG-I
|l Stratosphäre
|d 31.12.2006
|g ICG
|0 I:(DE-Juel1)VDB47
|x 0
970 _ _ |a VDB:(DE-Juel1)55688
980 _ _ |a VDB
980 _ _ |a ConvertedRecord
980 _ _ |a journal
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980 _ _ |a UNRESTRICTED
981 _ _ |a I:(DE-Juel1)ICE-4-20101013
981 _ _ |a I:(DE-Juel1)IEK-7-20101013


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