- Abstract:
-
The banded patterns of cloud and wind are among the most striking features of the atmospheres of Jupiter and Saturn, but their dynamical origin remains poorly understood. Most approaches towards understanding zonation so far (also in the terrestrial oceans) have used highly idealized models to show that it might originate from dynamical anisotropy in a shallow turbulent fluid layer due to the planetary β-effect. Here we report the results of laboratory experiments, conducted on a 14-m diamete...
Expand abstract - Publication status:
- Published
- Peer review status:
- Peer reviewed
- Publisher copy:
- 10.1029/2004GL020106
-
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- Publisher:
- American Geophysical Union Publisher's website
- Journal:
- Geophysical Research Letters Journal website
- Volume:
- 31
- Pages:
- Article: L22701
- Publication date:
- 2004-11-05
- DOI:
- ISSN:
-
0094–8276
- URN:
-
uuid:38f6aa19-95de-4155-af3f-3eba79b3540d
- Local pid:
- ora:4356
- Language:
- English
- Keywords:
- Subjects:
- Copyright holder:
- American Geophysical Union
- Copyright date:
- 2004
- Notes:
- The full-text of this article is not currently available in ORA, but you may be able to access the article via the publisher copy link on this record page. Citation: Read, P. L. et al. (2004). 'Jupiter's and Saturn's convectively driven banded jets in the laboratory', Geophysical Research Letters 31, L22701. [Available at http://www.agu.org/journals/gl/].
Journal article
Jupiter's and Saturn's convectively driven banded jets in the laboratory
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UK Particle Physics and Astronomy Research Council
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