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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

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.

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Verigin, M., Author
Kotova, G., Author
Shutte, N., Author
Remizov, A.1, Author              
Szegö, K., Author
Tátrallyay, M., Author
Apáthy, I., Author
Rosenbauer, H.2, Author              
Livi, S.2, Author              
Richter, A. K.2, Author              
Schwingenschuh, K., Author
Zhang, T.-L., Author
Slavin, J., Author
Lemaire, J., Author
Affiliations:
1Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832288              
2MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832291              

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 Dates: 1997
 Publication Status: Published in print
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Type: Peer
 Identifiers: BibTex Citekey: Verigin:1997-221
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Title: Journal Geophysical Research
Source Genre: Journal
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Publ. Info: -
Pages: - Volume / Issue: 102 Sequence Number: - Start / End Page: 2147 - 2155 Identifier: -