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Stellar winds and planetary atmospheres

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arxiv 2105.11243 v1 pith:YPQWZW7O submitted 2021-05-24 astro-ph.EP astro-ph.SR

classification astro-ph.EPastro-ph.SR
keywords atmospheresprocesseswindsactivityplanetaryatmosphereevolutioninteractions
verification ladder T0 review T1 audit T2 compute T3 formal
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Interactions between the winds of stars and the magnetospheres and atmospheres of planets involve many processes, including the acceleration of particles, heating of upper atmospheres, and a diverse range of atmospheric loss processes. Winds remove angular momentum from their host stars causing rotational spin-down and a decay in magnetic activity, which protects atmospheres from erosion. While wind interactions are strongly influenced by the X-ray and ultraviolet activity of the star and the chemical composition of the atmosphere, the role of planetary magnetic fields is unclear. In this chapter, I review our knowledge of the properties and evolution of stellar activity and winds and discuss the influences of these processes on the long term evolution of planetary atmospheres. I do not consider the large number of important processes taking place at the surfaces of planets that cause exchanges between the atmosphere and the planet's interior.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. OpenAlex reports about 107 citations worldwide. Full citation record

  1. Magnetic activity in cool stars: manifestations and relevance to exoplanets

    astro-ph.SR 2026-06 unverdicted novelty 3.0 of 10

    A review synthesizing manifestations of magnetic activity in cool stars and its relevance to exoplanet science via the solar-stellar connection.

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