- 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...
Expand abstract - Publication status:
- Published
- Peer review status:
- Peer reviewed
- Version:
- Publisher's Version
- Files:
-
-
(pdf, 5.2MB)
-
- Publisher copy:
- 10.1016/j.icarus.2018.12.002
-
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- Grant:
- ST/I001948/1
- ST/K00106X/1
- ST/F003145/1
- ST/K00087X/1
- ST/K003267/1
- Grant:
- ST/K00042X/1
- ST/K001590/1
- 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:
- Copyright holder:
- Young et al.
- Copyright date:
- 2018
- Notes:
- © 2018 The Authors. Published by Elsevier Inc. Under a Creative Commons license
Journal article
Simulating Jupiter's weather layer. Part II: Passive ammonia and water cycles
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+ Science and Technology Facilities Council
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Durham University
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