期刊论文

He, HQ

英文

ASTROPHYSICAL JOURNAL

0004-637X

2023

951

2

10.3847/1538-4357/acd330

This work was partially supported by the B-type Strategic Priority Program of the Chinese Academy of Sciences under grant XDB41000000, the National Natural Science Foundation of China under grants 41874207 and 41474154, the Chinese Academy of Sciences under grant KZZD-EW-01-2, the Natural Science Foundation of Hunan Province under grants 2022JJ40461 and 2021JJ30734, the Education Department of Hunan Province under grant 21B0301, and the Postgraduate Scientific Research Innovation Project of Hunan Province (No. CX20210819). H.-Q.H. gratefully acknowledges the partial support of the Youth Innovation Promotion Association of the Chinese Academy of Sciences (No. 2017091). We benefited from the data of exoplanets provided by exoplanet TEAM of Observatoire de Paris ( http://exoplanet.eu ).

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The habitability of Earth-like planets is an increasingly important subject in astrophysics and in planetary sciences. Atmospheric escape plays a vital role in the evolution of the habitability of Earth-like planets. By systematically analyzing the numerical simulation results of the interactions between the planetary atmospheres and the stellar winds, in this work, we evaluate various factors related to the atmospheric nonthermal ion escape rates, including planetary parameters (e.g., mass, density, radius, semimajor axis, etc.) and stellar wi...