Stellar activity and its influence on planetary atmosphere evolution

Physics

Scientific paper

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Scientific paper

The evolution of planetary atmospheres can only be understood if one recognizes the fact that the radiation and particle environment of the Sun or a planet's host star were not always on the same activity level. New insights, the latest observations and research regarding the evolution of the solar radiation, plasma environment and solar/stellar magnetic field from the observations of solar proxies and their impact on planetary atmospheres with different ages will be given. We present also a new innovative idea how hydrogen coronae and energetic neutral atom (ENA) observations around transiting Earth-like exoplanets by space observatories such as the WSO-UV, can be used for testing the addressed atmospheric evolution studies.

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