XUV-Exposed, Non-Hydrostatic Hydrogen-Rich Upper Atmospheres of Terrestrial Planets. Part I: Atmospheric Expansion and Thermal Escape-Reference-Cited by-同舟云学术

XUV-Exposed, Non-Hydrostatic Hydrogen-Rich Upper Atmospheres of Terrestrial Planets. Part I: Atmospheric Expansion and Thermal Escape

Published:2013-11 Issue:11 Volume:13 Page:1011-1029
ISSN:1531-1074
Container-title:Astrobiology
language:en
Short-container-title:Astrobiology

Author:

Erkaev Nikolai V.¹²,Lammer Helmut³,Odert Petra³⁴,Kulikov Yuri N.⁵,Kislyakova Kristina G.³⁴,Khodachenko Maxim L.³⁶,Güdel Manuel⁷,Hanslmeier Arnold⁴,Biernat Helfried³

Affiliation:

1. Institute of Computational Modelling, Siberian Division of the Russian Academy of Sciences, Krasnoyarsk, Russian Federation.

2. Siberian Federal University, Krasnoyarsk, Russian Federation.

3. Austrian Academy of Sciences, Space Research Institute, Graz, Austria.

4. Institute of Physics, University of Graz, Graz, Austria.

5. Polar Geophysical Institute (PGI), Russian Academy of Sciences, Murmansk, Russian Federation.

6. Institute of Nuclear Physics, Moscow State University, Moscow, Russian Federation.

7. Institute of Astrophysics, University of Vienna, Austria.

Publisher

Mary Ann Liebert Inc

Subject

Space and Planetary Science,Agricultural and Biological Sciences (miscellaneous)

Link

http://www.liebertpub.com/doi/pdf/10.1089/ast.2012.0957

Reference91 articles.

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2. Thermal and chemical evolution of the terrestrial magma ocean

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4. Photochemistry of Planetary Atmospheres

5. The effect of evaporation on the evolution of close-in giant planets

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