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Simulating Jupiter's weather layer. Part II: Passive ammonia and water cycles

Abstract:

We examine the ammonia and water cycles in Jupiter's upper troposphere and lower stratosphere during spin-up of a multiple zonal jet circulation using the Oxford Jupiter GCM. Jupiter's atmosphere is simulated at 512 x 256 horizontal resolution with 33 vertical levels between 0.01 and 18 bar, putting the lowest level well below the expected water cloud base. Simulations with and without a 5.7 W/m2 interior heat source were run for 130000-150000d to allow the deep atmosphere to come into radiat...

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Publication status:
Published
Peer review status:
Peer reviewed
Version:
Publisher's Version

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Publisher copy:
10.1016/j.icarus.2018.12.002

Authors


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Institution:
University of Oxford
Division:
MPLS Division
Department:
Physics
Subgroup:
Atmos Ocean & Planet Physics
Role:
Author
ORCID:
0000-0002-7241-8954
More by this author
Institution:
University of Oxford
Division:
MPLS Division
Department:
Physics
Subgroup:
Atmos Ocean & Planet Physics
Oxford college:
Trinity College
Role:
Author
More by this author
Institution:
University of Oxford
Division:
MPLS Division
Department:
Physics
Subgroup:
Atmos Ocean & Planet Physics
Role:
Author
More from this funder
Grant:
ST/I001948/1
ST/K00106X/1
ST/F003145/1
ST/K00087X/1
ST/K003267/1
Durham University More from this funder
Publisher:
Elsevier Publisher's website
Journal:
Icarus Journal website
Volume:
326
Pages:
253-268
Publication date:
2018-12-11
Acceptance date:
2018-12-03
DOI:
ISSN:
0019-1035
Pubs id:
pubs:949914
URN:
uri:b583fa89-eef7-4b24-994c-a1f0e270bb19
UUID:
uuid:b583fa89-eef7-4b24-994c-a1f0e270bb19
Local pid:
pubs:949914
Language:
English
Keywords:

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