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Quantitative model of the Martian magnetopause shape and its variation with the solar wind ram pressure based on Phobos 2 observations

MPS-Authors
http://pubman.mpdl.mpg.de/cone/persons/resource/persons104147

Remizov,  A.
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;

http://pubman.mpdl.mpg.de/cone/persons/resource/persons104165

Rosenbauer,  H.
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

http://pubman.mpdl.mpg.de/cone/persons/resource/persons104054

Livi,  S.
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

http://pubman.mpdl.mpg.de/cone/persons/resource/persons104153

Richter,  A. K.
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

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Citation

Verigin, M., Kotova, G., Shutte, N., Remizov, A., Szegö, K., Tátrallyay, M., et al. (1997). Quantitative model of the Martian magnetopause shape and its variation with the solar wind ram pressure based on Phobos 2 observations. Journal Geophysical Research, 102, 2147-2155.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0014-D8C6-8
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