Saturn’s rotation period from its atmospheric planetary-wave configuration
Saturn’s rotation period from its atmospheric planetary-wave configuration
复制标题
土星的自转周期来自其大气行星波结构
DOI:
10.1038/nature08194
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发表时间:
2009
期刊:
影响因子:
64.8
通讯作者:
Gerald Schubert
中科院分区:
文献类型:
--
作者:
P. L. Read;T. Dowling;Gerald Schubert
The rotation period of a gas giant's magnetic field (called the System III reference frame) is commonly used to infer its bulk rotation. Saturn's dipole magnetic field is not tilted relative to its rotation axis (unlike Jupiter, Uranus and Neptune), so the surrogate measure of its long-wavelength (kilometric) radiation is currently used to fix the System III rotation period. The period as measured now by the Cassini spacecraft is up to ∼7 min longer than the value of 10 h 39 min 24 s measured 28 years ago by Voyager. Here we report a determination of Saturn's rotation period based on an analysis of potential vorticity. The resulting reference frame (which we call System IIIw) rotates with a period of 10 h 34 min 13 ± 20 s. This shifted reference frame is consistent with a pattern of alternating jets on Saturn that is more symmetrical between eastward and westward flow. This suggests that Saturn's winds are much more like those of Jupiter than hitherto believed.