探测冰巨星磁层系统的科学回报

Xin Cao, Xiangning Chu, Hsiang-Wen Hsu, Hao Cao, Weijie Sun, Lucas Liuzzo, Jasper Halekas, Carol Paty, Feng Chu, O. Agiwal, Lauren Blum, F. Crary, Ian Cohen, P. Delamere, M. Hofstadter, G. Hospodarsky, Cooper John, P. Kollmann, E. Kronberg, William Kurth, L. Lamy, Dong Lin, Wen Li, Xuanye Ma, D. Malaspina, Michiko Morooka, Tom A. Nordheim, F. Postberg, Andrew Poppe, Cartwright Richard, S. Ruhunusiri, Krista Soderlund, James O'Donoghue, Ferdinand Plaschke
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摘要

冰巨星的磁层系统是典型系外行星的理想和独特模板,但在过去十年中却没有得到充分的研究。这些不对称且极富动态的磁层的复杂性为我们提供了一个很好的机会,可以系统地研究宇宙中这类常见系外行星磁层的一般驱动机制,以及影响这类行星全局和局部磁层结构的关键因素。在本文中,我们讨论了为未来飞行任务探测冰巨星磁层系统的科学回报,包括从与上游太阳风的相互作用到磁尾下游区域的不同磁层区域。我们强调在未来几十年探测冰巨星磁层系统的重要性,这使我们能够深入了解冰巨星本身以及广泛分布在宇宙中的类似系外行星的空间环境和宜居性。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Science return of probing magnetospheric systems of ice giants
The magnetospheric systems of ice giants, as the ideal and the unique template of a typical class of exoplanets, have not been sufficiently studied in the past decade. The complexity of these asymmetric and extremely dynamic magnetospheres provides us a great chance to systematically investigate the general mechanism of driving the magnetospheres of such common exoplanets in the Universe, and the key factors of influencing the global and local magnetospheric structures of this type of planets. In this paper, we discuss the science return of probing magnetospheric systems of ice giants for the future missions, throughout different magnetospheric regions, across from the interaction with upstream solar wind to the downstream region of the magnetotail. We emphasize the importance of detecting the magnetospheric systems of ice giants in the next decades, which enables us to deeply understand the space enviroNMent and habitability of not only the ice giants themselves but also the analogous exoplanets which are widely distributed in the Universe.
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