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Radiative forcing of the stratosphere of Jupiter, Part I: Atmospheric cooling rates from Voyager to Cassini

Abstract:

We developed a line-by-line heating and cooling rate model for the stratosphere of Jupiter, based on two complete sets of global maps of temperature, CH and CH, retrieved from the Cassini and Voyager observations in the latitude and vertical plane, with a careful error analysis. The non-LTE effect is found unimportant on the thermal cooling rate below the 0.01 mbar pressure level. The most important coolants are molecular hydrogen between 10 and 100 mbar, and hydrocarbons, including ethane (C...

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Publication status:
Published

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Publisher copy:
10.1016/j.pss.2013.07.005

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Journal:
PLANETARY AND SPACE SCIENCE More from this journal
Volume:
88
Pages:
3-25
Publication date:
2013-11-01
DOI:
ISSN:
0032-0633
Keywords:
Pubs id:
pubs:425706
UUID:
uuid:d5f5a9aa-18d4-4edb-829b-8dfabffee4d1
Local pid:
pubs:425706
Source identifiers:
425706
Deposit date:
2013-11-17

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