On Jupiter's Rate of RotationSource: Journal of the Atmospheric Sciences:;1974:;Volume( 031 ):;issue: 005::page 1471Author:Stone, Peter H.
DOI: 10.1175/1520-0469(1974)031<1471:OJROR>2.0.CO;2Publisher: American Meteorological Society
Abstract: It is suggested that the apparent lag of Jupiter's mean rotation rate in extratropical latitudes (System II) behind the rotation rate of Jupiter's radio emissions (System III) is caused by the difference between phase speeds and true speeds in extratropical latitudes. An estimate of the difference based on the formula for the phase speed of Rossby waves agrees with the difference calculated from the two rotation rates.
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| contributor author | Stone, Peter H. | |
| date accessioned | 2017-06-09T14:17:38Z | |
| date available | 2017-06-09T14:17:38Z | |
| date copyright | 1974/07/01 | |
| date issued | 1974 | |
| identifier issn | 0022-4928 | |
| identifier other | ams-16617.pdf | |
| identifier uri | http://onlinelibrary.yabesh.ir/handle/yetl/4152420 | |
| description abstract | It is suggested that the apparent lag of Jupiter's mean rotation rate in extratropical latitudes (System II) behind the rotation rate of Jupiter's radio emissions (System III) is caused by the difference between phase speeds and true speeds in extratropical latitudes. An estimate of the difference based on the formula for the phase speed of Rossby waves agrees with the difference calculated from the two rotation rates. | |
| publisher | American Meteorological Society | |
| title | On Jupiter's Rate of Rotation | |
| type | Journal Paper | |
| journal volume | 31 | |
| journal issue | 5 | |
| journal title | Journal of the Atmospheric Sciences | |
| identifier doi | 10.1175/1520-0469(1974)031<1471:OJROR>2.0.CO;2 | |
| journal fristpage | 1471 | |
| journal lastpage | 1472 | |
| tree | Journal of the Atmospheric Sciences:;1974:;Volume( 031 ):;issue: 005 | |
| contenttype | Fulltext |