Hauptseite > Publikationsdatenbank > Do cosmic-ray-driven electron-induced reactions impact stratospheric ozone depletion and global climate change? > print

001     13790
005     20240709074301.0
024 7 _ |2 DOI
|a 10.1016/j.atmosenv.2011.03.059
024 7 _ |2 WOS
|a WOS:000292809300020
024 7 _ |a altmetric:179839
|2 altmetric
037 _ _ |a PreJuSER-13790
041 _ _ |a eng
082 _ _ |a 550
084 _ _ |2 WoS
|a Environmental Sciences
084 _ _ |2 WoS
|a Meteorology & Atmospheric Sciences
100 1 _ |a Grooß, J.-U.
|0 P:(DE-Juel1)129122
|b 0
|u FZJ
245 _ _ |a Do cosmic-ray-driven electron-induced reactions impact stratospheric ozone depletion and global climate change?
260 _ _ |a Amsterdam [u.a.]
|b Elsevier Science
|c 2011
300 _ _ |a 3508 - 3514
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 Atmospheric Environment
|x 1352-2310
|0 697
|y 20
|v 45
500 _ _ |3 POF3_Assignment on 2016-02-29
500 _ _ |a Record converted from VDB: 12.11.2012
520 _ _ |a Recently, the cosmic-ray-driven electron-induced reaction mechanism (CRE) was introduced to explain polar ozone depletion and surface temperature change. It was proposed that the dissociation of chlorofluorocarbons (CFCs) on ice surfaces of polar stratospheric clouds plays the dominant role in forming the ozone hole. Efforts have been made to predict polar ozone loss in future years. It was further proposed that CFCs and cosmic-ray-driven ozone depletion may control global surface temperatures. These assertions challenge the fundamental understanding of Antarctic stratospheric ozone loss and global warming. Here we show that these arguments based on the CRE mechanism are inconclusive. First, correlations of satellite data of CFC-12, N2O and CH4 from ACE-FTS show no evidence of significant loss of CFC-12 as predicted by the CRE mechanism. Second, conclusions drawn about a possible CRE impact on the atmosphere, based on correlations of different observed atmospheric parameters, do not have a physical basis. Finally, predictions on the future development of the atmosphere based on these correlations are not reliable for either the ozone hole or global surface temperatures. (C) 2011 Elsevier Ltd. All rights reserved.
536 _ _ |a Atmosphäre und Klima
|c P23
|2 G:(DE-HGF)
|0 G:(DE-Juel1)FUEK491
|x 0
588 _ _ |a Dataset connected to Web of Science
650 _ 7 |a J
|2 WoSType
653 2 0 |2 Author
|a Ozone
653 2 0 |2 Author
|a Ozone depletion
653 2 0 |2 Author
|a Global warming
653 2 0 |2 Author
|a Cosmic rays
653 2 0 |2 Author
|a Dissociative electron attachment
700 1 _ |a Müller, R.
|0 P:(DE-Juel1)129138
|b 1
|u FZJ
773 _ _ |a 10.1016/j.atmosenv.2011.03.059
|g Vol. 45, p. 3508 - 3514
|p 3508 - 3514
|q 45<3508 - 3514
|0 PERI:(DE-600)1499889-0
|t Atmospheric environment
|v 45
|y 2011
|x 1352-2310
856 7 _ |u http://dx.doi.org/10.1016/j.atmosenv.2011.03.059
909 C O |o oai:juser.fz-juelich.de:13790
|p VDB
|p VDB:Earth_Environment
913 1 _ |k P23
|v Atmosphäre und Klima
|l Atmosphäre und Klima
|b Erde und Umwelt
|z vormals P22
|0 G:(DE-Juel1)FUEK491
|x 0
913 2 _ |a DE-HGF
|b Marine, Küsten- und Polare Systeme
|l Atmosphäre und Klima
|1 G:(DE-HGF)POF3-240
|0 G:(DE-HGF)POF3-249H
|2 G:(DE-HGF)POF3-200
|v Addenda
|x 0
914 1 _ |y 2011
915 _ _ |0 StatID:(DE-HGF)0010
|a JCR/ISI refereed
920 1 _ |k IEK-7
|l Stratosphäre
|g IEK
|0 I:(DE-Juel1)IEK-7-20101013
|x 0
970 _ _ |a VDB:(DE-Juel1)125497
980 _ _ |a VDB
980 _ _ |a ConvertedRecord
980 _ _ |a journal
980 _ _ |a I:(DE-Juel1)IEK-7-20101013
980 _ _ |a UNRESTRICTED
981 _ _ |a I:(DE-Juel1)ICE-4-20101013

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