- Abstract:
-
The zonal jets on the giant planets have been thought to be stable in time1-3. A decline in the velocity of Saturn's equatorial jet has been identified, on the basis of a comparison of cloud-tracking data across two decades4, but the differences in cloud speeds have since been suggested to stem from changes in cloud altitude in combination with vertical wind shear, rather than from temporal changes in wind strength at a given height5. Here, we combine observations of cloud tracks and of atmos...
Expand abstract - Publication status:
- Published
- Publisher copy:
- 10.1038/NGEO1292
-
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- Journal:
- NATURE GEOSCIENCE
- Volume:
- 4
- Issue:
- 11
- Pages:
- 750-752
- Publication date:
- 2011-11-05
- DOI:
- EISSN:
-
1752-0908
- ISSN:
-
1752-0894
- URN:
-
uuid:45a91032-8372-4b73-9873-7c25a81c1b46
- Source identifiers:
-
206326
- Local pid:
- pubs:206326
- Language:
- English
- Copyright date:
- 2011
Journal article
Equatorial winds on Saturn and the stratospheric oscillation
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