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木星的大气喷流可以延伸数千公里
Y Kaspi1, E Galanti1, W B Hubbard2
1Department of Earth and Planetary Sciences, Weizmann Institute of Science, Rehovot 76100, Israel.
Nature
|March 9, 2018
概括
强大的喷流可以达到数千公里的深度, 延伸到行星的磁散射区域. 朱诺航天器的重力数据揭示了动态的大气层
科学领域:
- 星球科学
- 流体动力学
- 地质学
背景情况:
- 木星的东西喷流是一个突出的特征, 但它们的垂直范围仍然未知.
- 了解深层大气和内部流动对于理解木星的结构和演变至关重要.
研究的目的:
- 为了确定木星观察到的喷流的深度.
- 研究木星的重力场及其大气/内部动态之间的关系.
主要方法:
- 来自朱诺航天器的重力测量分析.
- 重力数据的反转以推导风场和大气流形状.
- 模拟内部结构对重力波的贡献.
主要成果:
- 奇特的重力波 (J3,J5,J7,J9) 表示喷流延伸到数千公里的深度.
- 喷流深度可能达到3000公里左右的磁散射区域.
- 即使是重力波 (J8,J10) 也与导出的流量形状和内部结构一致.
- 木星的动态大气构成了大约百分之一的行星的总质量.
结论:
- 星的强大喷流比之前认为的更深入.
- 朱诺任务的重力数据提供了前所未有的洞察力,
- 这些发现完善了气态巨星的组成和循环模型.
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