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Observations and models of the wind system in Jupiter's atmosphere

机译:木星大气中风系统的观测和模型

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With this Ph.D. Thesis work we have used the information provided by HST observations to improve our knowledge of the long-term behaviour of Jupiter's zonal winds, and numerical simulations to explore the wind structure of the planet's upper troposphere. The deduced high velocity at the 6 bar level is difficult to understand under the hypothesis that solar insolation alone drives Jupiter's circulation. The internal heat source may play a significant role. If so, the jovian jets may extend deeply, which can help to explain their long term stability.
机译:拥有博士学位论文工作中,我们使用了HST观测提供的信息来提高对木星纬向风长期行为的了解,并利用数值模拟来探索行星对流层的风结构。在仅靠太阳直射驱动木星环流的假设下,很难理解6 bar级推论得出的高速。内部热源可能起重要作用。如果是这样,木星喷气机可能会延伸得很深,这有助于解释它们的长期稳定性。

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