XUV-Exposed, Non-Hydrostatic Hydrogen-Rich Upper Atmospheres of Terrestrial Planets. Part II: Hydrogen Coronae and Ion Escape

We studied the interactions between the stellar wind plasma flow of a typical M star, such as GJ 436, and the hydrogen-rich upper atmosphere of an Earth-like planet and a “super-Earth” with a radius of 2 R(Earth) and a mass of 10 M(Earth), located within the habitable zone at ∼0.24 AU. We investigat...

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Bibliographic Details
Main Authors: Kislyakova, Kristina G., Lammer, Helmut, Holmström, Mats, Panchenko, Mykhaylo, Odert, Petra, Erkaev, Nikolai V., Leitzinger, Martin, Khodachenko, Maxim L., Kulikov, Yuri N., Güdel, Manuel, Hanslmeier, Arnold
Format: Artigo
Language:Inglês
Published: Mary Ann Liebert, Inc. 2013
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Research Articles
Online Access:https://ncbi.nlm.nih.gov/pmc/articles/PMC3865724/
https://ncbi.nlm.nih.gov/pubmed/24283926
https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1089/ast.2012.0958
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