Journal article

The origin of belt/zone contrasts in the atmosphere of Jupiter and their correlation with 5-mu m opacity

Publication status:: Published

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APA Style

Irwin, P., Weir, A., Taylor, F., Calcutt, S., & Carlson, R. (2001). The origin of belt/zone contrasts in the atmosphere of Jupiter and their correlation with 5-mu m opacity. ICARUS, 149(2), 397–415.

MLA Style

Irwin, P, et al. “The Origin of Belt/Zone Contrasts in the Atmosphere of Jupiter and Their Correlation with 5-Mu m Opacity.” ICARUS, vol. 149, no. 2, 2001, pp. 397–415.

Chicago Style

Irwin, P, A Weir, F Taylor, S Calcutt, and R Carlson. 2001. “The Origin of Belt/Zone Contrasts in the Atmosphere of Jupiter and Their Correlation with 5-Mu m Opacity.” ICARUS 149 (2): 397–415.
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Publisher copy:: 10.1006/icar.2000.6542

Authors

+ Irwin, P More by this author

Role:: Author

+ Weir, A More by this author

Role:: Author

+ Taylor, F More by this author

Institution:: University of Oxford
Division:: MPLS
Department:: Physics
Sub department:: Atmos Ocean & Planet Physics
Role:: Author

+ Calcutt, S More by this author

Institution:: University of Oxford
Division:: MPLS
Department:: Physics
Sub department:: Atmos Ocean & Planet Physics
Role:: Author

+ Carlson, R More by this author

Role:: Author

Journal:: ICARUS More from this journal
Volume:: 149
Issue:: 2
Pages:: 397-415
Publication date:: 2001-02-01
DOI:: 10.1006/icar.2000.6542
ISSN:: 0019-1035

Keywords:: Jupiter

clouds

atmosphere
Pubs id:: pubs:28883
UUID:: uuid:0b345227-2f70-405f-a2f5-3e2987c8b9af
Local pid:: pubs:28883
Source identifiers:: 28883
Deposit date:: 2012-12-19
ARK identifier:: ark:/29072/ora_0b3452272f70405fa2f53e2987c8b9af

Terms of use

Copyright date:: 2001

Licence:: Terms and Conditions of Use for Oxford University Research Archive

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