A new axisymmetric MHD model of the interaction of the solar wind with Venus

Journal of Geophysical Research: Planets

Volumn 101, Issue E2, 1996, Pages 4547-4556

  De Zeeuw, Darren L ^a  

^a UNIVERSITY OF MICHIGAN   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0005352415     PISSN: 01480227     EISSN: None     Source Type: Journal    
DOI: 10.1029/95JE03363     Document Type: Article

References (5)

1. Alexander, C.J., J.G. Luhmann, and C.T. Russell, Interplanetary field control of the location of the Venus bow shock: Evidence for comet-like ion pickup, Geophys. Res. Lett., 13, 917, 1986.
2. Belotserkovskii, O.M., T.K. Breus, A.M.Krymskii, V.Y. Mitnitskii, A.F. Nagy, and T.I.Gombosi, The effect of hot oxygen corona on the interaction of the solar wind with Venus., Geophys. Res. Lett., 14, 503, 1987.
3. Brecht, S.H., Magnetic asymmetries of unmagnetized planets., Geophys. Res. Lett., 17, 1243, 1990.
4. Brecht, S.H., and J.R. Ferrante, Global hybrid simulation of unmagnetized planets: Comparison of Venus and Mars., J. Geophys. Res., 96, 11209, 1991.
5. Brecht, S.H., J.R. Ferrante, and J.G. Luhmann, Three-dimensional simulation of the solar wind interaction with Mars., J. Geophys. Res., 98, 1345, 1993.