ATMOSPHERIC ESCAPE OF CLOSE-IN NEPTUNES

Proceedings of the 48-th International student's conferences "Physics of Space" Pub Date : 1900-01-01 DOI:10.15826/b978-5-7996-2935-9.52

E. Kalinicheva, V. Shematovich, Y. Pavlyuchenkov

引用次数: 0

Abstract

We used the previously developed self-consistent 1D model of hydrogen-helium atmosphere with suprathermal electrons accounted [1] to calculate the rate of close-in Naeptune atmospheric loss. The two-scale structure of the close-in (hot) Neptune atmosphere was found.

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近距离海王星的大气逃逸

我们使用先前建立的氢氦大气自洽一维模型，超热电子占[1]，计算近地海王星大气损失率。发现了近距离(热)海王星大气的双尺度结构。

本文章由计算机程序翻译，如有差异，请以英文原文为准。

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Proceedings of the 48-th International student's conferences "Physics of Space"

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