He2+transport in the Martian upper atmosphere with an induced magnetic field

Author:

Shematovich V. I.1,Bisikalo D. V.1,Stenberg G.2,Barabash S.2,Diéval C.23,Gérard J.-C.4

Affiliation:

1. Institute of Astronomy; Russian Academy of Sciences; Moscow Russian Federation

2. Swedish Institute of Space Physics; Kiruna Sweden

3. Division of Space Technology, Department of Computer Science, Electrical and Space Engineering; Luleå University of Technology; Kiruna Sweden

4. LPAP; Université de Liège; Liège Belgium

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Reference37 articles.

1. Dayside induced magnetic field in the ionosphere of Mars;Akalin;Icarus,2010

2. Martian magnetic morphology: Contributions from the solar wind and crust;Brain;J. Geophys. Res.,2003

3. Indirect detection of the Martian helium corona;Barabash;Geophys. Res. Lett.,1994

4. Measurements of the nonthermal helium escape from Mars;Barabash;J. Geophys. Res.,1995

5. The analyzer of space plasmas and energetic atoms (ASPERA-3) for the Mars Express mission;Barabash;Space Sci. Rev.,2006

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