Hauptseite > Publikationsdatenbank > Zonal Asymmetries in Middle Atmosphere Temperatures > print

001     35332
005     20240911115615.0
024 7 _ |2 DOI
|a 10.1016/S0273-1177(03)90475-3
024 7 _ |2 WOS
|a WOS:000188280600016
037 _ _ |a PreJuSER-35332
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 Offermann, D.
|b 0
|0 P:(DE-HGF)0
245 _ _ |a Zonal Asymmetries in Middle Atmosphere Temperatures
260 _ _ |a Amsterdam [u.a.]
|b Elsevier Science
|c 2003
300 _ _ |a 1771 - 1780
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 9
|v 32
500 _ _ |a Record converted from VDB: 12.11.2012
520 _ _ |a Zonal asymmetries axe frequently seen in stratospheric temperature or trace gas fields as surf zones, streamers, filaments etc. They axe also seen as very small-scale fluctuations, the intensity of which varies with longitude. Similar structures might be expected in the mesosphere as well, and several examples have recently been found. CRISTA 1 large-scale data are presented that indicate a surf zone in the middle mesosphere at the beginning of winter. Very small-scale data are shown from the CRISTA 2 mission. Mesospheric variability is found to be high at all altitudes, latitudes, and longitudes. There axe considerable non-zonal structures in these fluctuations. (The duration of the Crista missions was about one week each.)Zonal asymmetries have been known for a long time from comparisons of ground stations measuring the same parameter in the mesosphere / lower thermosphere As an example, upper mesosphere temperatures derived from OH* emissions are compaxed here for Wuppertal and Moscow (Zvenigorod), which are about 2000 km apart. A systematic and substantial difference in temperature is obtained, with higher temperatures at Wuppertal than at Moscow. The difference appears to follow the solar cycle: it is small at solar maximum and large (up to 28 K) at solar minimum. The reason for this surprising behavior is as yet unknown.The Moscow and Wuppertal temperatures have also been analyzed for long-term trends: a trend discrepancy between the two stations is not seen in the data interval common to the two stations. (C) 2003 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
700 1 _ |a Donner, M.
|b 1
|0 P:(DE-HGF)0
700 1 _ |a Grossmann, K. U.
|b 2
|0 P:(DE-HGF)0
700 1 _ |a Gusev, O.
|b 3
|0 P:(DE-HGF)0
700 1 _ |a Jarisch, M.
|b 4
|0 P:(DE-HGF)0
700 1 _ |a Kaufmann, M.
|b 5
|u FZJ
|0 P:(DE-Juel1)129128
700 1 _ |a Oberheide, J.
|b 6
|0 P:(DE-HGF)0
700 1 _ |a Semenov, A. I.
|b 7
|u FZJ
|0 P:(DE-Juel1)VDB32783
773 _ _ |a 10.1016/S0273-1177(03)90475-3
|g Vol. 32, p. 1771 - 1780
|p 1771 - 1780
|q 32<1771 - 1780
|0 PERI:(DE-600)2023311-5
|t Advances in space research
|v 32
|y 2003
|x 0273-1177
856 7 _ |u http://dx.doi.org/10.1016/S0273-1177(03)90475-3
909 C O |o oai:juser.fz-juelich.de:35332
|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 _ |a Nachtrag
|y 2003
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)42355
980 _ _ |a VDB
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980 _ _ |a journal
980 _ _ |a I:(DE-Juel1)IEK-7-20101013
980 _ _ |a UNRESTRICTED
981 _ _ |a I:(DE-Juel1)ICE-4-20101013
981 _ _ |a I:(DE-Juel1)IEK-7-20101013

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