Coronal Mass Ejection (CME) Activity of Low Mass M Stars as An Important Factor for The Habitability of Terrestrial Exoplanets. I. CME Impact on Expected Magnetospheres of Earth-Like Exoplanets in Close-In Habitable Zones-Reference-Cited by-同舟云学术

Coronal Mass Ejection (CME) Activity of Low Mass M Stars as An Important Factor for The Habitability of Terrestrial Exoplanets. I. CME Impact on Expected Magnetospheres of Earth-Like Exoplanets in Close-In Habitable Zones

Published:2007-02 Issue:1 Volume:7 Page:167-184
ISSN:1531-1074
Container-title:Astrobiology
language:en
Short-container-title:Astrobiology

Author:

Khodachenko Maxim L.¹,Ribas Ignasi²³,Lammer Helmut¹,Grießmeier Jean-Mathias⁴⁵,Leitner Martin¹,Selsis Franck⁶⁷,Eiroa Carlos⁸,Hanslmeier Arnold⁹,Biernat Helfried K.¹⁹,Farrugia Charles J.¹⁰¹¹,Rucker Helmut O.¹⁹

Affiliation:

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

2. Institut d'Estudis Espacials de Catalunya, Barcelona, Spain.

3. Instituto de Ciencias del Espacio, Barcelona, Spain.

4. Institute for Theoretical Physics, Technical University of Braunschweig, Mendelssohnstrasse 3, D-38106 Braunschweig, Germany.

5. Present address: LESIA, CNRS-Observatoire de Paris, Meudon, France.

6. Centre de Recherche Astronomique de Lyon, Lyon, France.

7. École Normale Supérieure, Lyon, France.

8. Departemento de Física Teórica, Facultad de Ciencias, Universidad Autónoma de Madrid, Cantoblanco, Madrid, Spain.

9. Institute for Physics, University of Graz, Graz, Austria.

10. Institute for the Study of Earth, Oceans, and Space, Durham, New Hampshire.

11. Department of Physics, University of New Hampshire, Durham, New Hampshire.

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.2006.0127

Reference66 articles.

1. A Model for Solar Coronal Mass Ejections

2. Interchange instability of the Venusian ionopause

3. Extreme‐Ultraviolet Flare Activity in Late‐Type Stars

4. The structure and origin of magnetic clouds in the solar wind

5. Magnetic loop behind an interplanetary shock: Voyager, Helios, and IMP 8 observations

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