001     29689
005     20240911115609.0
024 7 _ |a 10.1029/2002JD002800
|2 DOI
024 7 _ |a WOS:000182874800002
|2 WOS
024 7 _ |a 0022-1406
|2 ISSN
024 7 _ |a 0148-0227
|2 ISSN
024 7 _ |a 2128/20866
|2 Handle
037 _ _ |a PreJuSER-29689
041 _ _ |a eng
082 _ _ |a 550
082 _ _ |a 550
084 _ _ |2 WoS
|a Meteorology & Atmospheric Sciences
100 1 _ |a Kaufmann, M.
|b 0
|u FZJ
|0 P:(DE-Juel1)129128
245 _ _ |a Satellite observations of daytime and nighttime ozone in the mesosphere and lower thermosphere
260 _ _ |a Washington, DC
|b Union
|c 2003
|a Washington, DC
|b Union
300 _ _ |a D9
336 7 _ |a Journal Article
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336 7 _ |a Journal Article
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336 7 _ |a ARTICLE
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336 7 _ |a JOURNAL_ARTICLE
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336 7 _ |a article
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440 _ 0 |a Journal of Geophysical Research
|x 0022-1406
|0 3369
|v 108
500 _ _ |a Record converted from VDB: 12.11.2012
520 _ _ |a [1] The global distribution of mesospheric and lower thermospheric ozone 9.6 mum infrared emissions was measured by the Cryogenic Infrared Spectrometers and Telescopes for the Atmosphere (CRISTA) experiment during two Space Shuttle missions in November 1994 and August 1997. The radiances measured by CRISTA have been inverted to O-3 number densities in the 50-95 km range by using a nonlocal thermodynamic equilibrium model. A detailed sensitivity study of retrieved O-3 number densities has been carried out. The ozone abundance profiles show volume mixing ratios of 1-2 ppmv at the stratopause, 0.5 ppmv or less around 80 km, and typically 1 ppmv during daytime and 10 ppmv during nighttime at the secondary maximum. The agreement with other experiments is typically better than 25%. The global distribution of upper mesospheric ozone shows significant latitudinal gradients and an enhancement in the equatorial upper mesosphere. At the polar night terminator a third ozone maximum is observed. Three-dimensional model results indicate that the latitudinal gradients are significantly influenced by solar tides.
536 _ _ |a Chemie und Dynamik der Geo-Biosphäre
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588 _ _ |a Dataset connected to Web of Science
650 _ 7 |a J
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653 2 0 |2 Author
|a mesosphere
653 2 0 |2 Author
|a ozone
653 2 0 |2 Author
|a CRISTA
653 2 0 |2 Author
|a lower thermosphere
653 2 0 |2 Author
|a ROSE
653 2 0 |2 Author
|a non-LTE
700 1 _ |a Gusev, O. A.
|b 1
|0 P:(DE-HGF)0
700 1 _ |a Grossmann, K. U.
|b 2
|0 P:(DE-HGF)0
700 1 _ |a Martín-Torres, F. J.
|b 3
|u FZJ
|0 P:(DE-Juel1)VDB21257
700 1 _ |a Marsh, D. R.
|b 4
|0 P:(DE-HGF)0
700 1 _ |a Kutepov, A. A.
|b 5
|0 P:(DE-HGF)0
773 _ _ |0 PERI:(DE-600)2016800-7
|a 10.1029/2002JD002800
|g Vol. 108, p. D9
|p D9
|q 108|t Journal of geophysical research / Atmospheres
|v 108
|x 0022-1406
|y 2003
856 7 _ |u http://dx.doi.org/10.1029/2002JD002800
856 4 _ |u https://juser.fz-juelich.de/record/29689/files/2002JD002800.pdf
|y OpenAccess
856 4 _ |u https://juser.fz-juelich.de/record/29689/files/2002JD002800.pdf?subformat=pdfa
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909 C O |o oai:juser.fz-juelich.de:29689
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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 2003
915 _ _ |a OpenAccess
|0 StatID:(DE-HGF)0510
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915 _ _ |a JCR/ISI refereed
|0 StatID:(DE-HGF)0010
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)26607
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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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