Atmospheric Escape Processes and Planetary Atmospheric Evolution

The habitability of the surface of any planet is determined by a complex evolution of its interior, surface, and atmosphere. The electromagnetic and particle radiation of stars drive thermal, chemical, and physical alteration of planetary atmospheres, including escape. Many known extrasolar planets...

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Bibliographic Details
Published in:	Journal of geophysical research. Space physics Vol. 125; no. 8
Main Authors:	Gronoff, G., Arras, P., Baraka, S., Bell, J. M., Cessateur, G., Cohen, O., Curry, S. M., Drake, J. J., Elrod, M., Erwin, J., Garcia‐Sage, K., Garraffo, C., Glocer, A., Heavens, N. G., Lovato, K., Maggiolo, R., Parkinson, C. D., Simon Wedlund, C., Weimer, D. R., Moore, W. B.
Format:	Journal Article
Language:	English
Published:	Washington Blackwell Publishing Ltd 01.08.2020 American Geophysical Union/Wiley
Subjects:	Astrophysics Atmosphere Atmospheric evolution Earth and Planetary Astrophysics Earth atmosphere Extrasolar planets Habitability Hypotheses Magnetic fields Physics Planetary atmospheres Planetary evolution Planetary magnetic fields Planets Radiation Solar system Stars Stellar evolution Stellar magnetic fields Stellar winds Surface temperature Target detection Temperature range Thermosphere Water Xenon
ISSN:	2169-9380, 2169-9402
Online Access:	Get full text
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