001     40890
005     20240709074439.0
024 7 _ |2 DOI
|a 10.1016/j.asr.2005.07.031
024 7 _ |2 WOS
|a WOS:000240088800018
037 _ _ |a PreJuSER-40890
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 Wu, D. L.
|b 0
|0 P:(DE-HGF)0
245 _ _ |a Remote sounding of atmospheric gravity waves with satellite limb and nadir techniques
260 _ _ |a Amsterdam [u.a.]
|b Elsevier Science
|c 2006
300 _ _ |a 2269 - 2277
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 12
|v 37
500 _ _ |a Record converted from VDB: 12.11.2012
520 _ _ |a Recent advances in satellite techniques hold great potential for mapping global gravity wave (GW) processes at various altitudes. Poor understanding of small-scale GWs has been a major limitation to numerical climate and weather models for making reliable forecasts. Observations of short-scale features have important implication for validating and improving future high-resolution numerical models. This paper summarizes recent GW observations and sensitivities from several satellite instruments, including MLS, AMSU-A, AIRS, GPS, and CLAES. It is shown in an example that mountain waves with horizontal wavelengths as short as similar to 30 km now can be observed by AIRS, reflecting the superior horizontal resolution in these modern satellite instruments. Our studies show that MLS, AMSU-A and AIRS observations reveal similar GW characteristics, with the observed variances correlated well with background winds. As a complementary technique, limb sounding instruments like CRISTA, CLAES, and GPS can detect GWs with better vertical but poorer horizontal resolutions. To resolve different parts of the broad GW spectrum, both satellite limb and nadir observing techniques are needed, and a better understanding of GW complexities requires joint analyses of these data and dedicated hieh-resolution model simulations. (c) 2005 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 S
|2 WoSType
653 2 0 |2 Author
|a gravity waves
653 2 0 |2 Author
|a satellite observations
653 2 0 |2 Author
|a instrument filter
653 2 0 |2 Author
|a wave sources
700 1 _ |a Preusse, P.
|b 1
|u FZJ
|0 P:(DE-Juel1)VDB12001
700 1 _ |a Eckermann, S. D.
|b 2
|0 P:(DE-HGF)0
700 1 _ |a Jiang, J. H.
|b 3
|0 P:(DE-HGF)0
700 1 _ |a de la Torre, M.
|b 4
|0 P:(DE-HGF)0
700 1 _ |a Juarez, L. C.
|b 5
|0 P:(DE-HGF)0
700 1 _ |a Wang, D. Y.
|b 6
|0 P:(DE-HGF)0
773 _ _ |a 10.1016/j.asr.2005.07.031
|g Vol. 37, p. 2269 - 2277
|p 2269 - 2277
|q 37<2269 - 2277
|0 PERI:(DE-600)2023311-5
|t Advances in space research
|v 37
|y 2006
|x 0273-1177
856 7 _ |u http://dx.doi.org/10.1016/j.asr.2005.07.031
909 C O |o oai:juser.fz-juelich.de:40890
|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 2006
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)55692
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980 _ _ |a ConvertedRecord
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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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