A three-dimensional MHD model of plasma flow around Titan

Planetary and Space Science

Volumn 46, Issue 9-10, 1998, Pages 1175-1191

  Ledvina, S A ^a   Cravens, T E ^a  

^a UNIVERSITY OF KANSAS   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0001578727     PISSN: 00320633     EISSN: None     Source Type: Journal    
DOI: 10.1016/S0032-0633(98)00052-X     Document Type: Article

References (14)

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9. Luhmann, J. G. and Cravens, T. E. (1991) Magnetic fields in the ionosphere of Venus. Space Sci. Rev. 55, 201.
10. Luhmann, J. G., Russell, C. T., Schwingenschuh, K. and Yeroshenko, Ye. (1991) A comparison of induced magnetotails of planetary bodies: Venus, Mars, and Titan. J. Geophys. Res. 96, 11199.
11. Ness, N. F., Acuna, M. H., Behannon, K. W. and Neubauer, F. M. (1982) The induced magnetosphere of Titan. J. Geophys. Res. 87, 1369.
12. Neubauer, F. M., Gurnett, D. A., Scudder, J. D. and Hartle, R. E. (1984) Titan's magnetospheric interaction. In Saturn, ed. T. Gehrels and M. S. Matthews, Univ. of Arizona Press, Tucson, pp. 760-787.
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14. Stone, J. M. and Norman, M. L. (1992) ZEUS-2D: A radiation magneto-hydrodynamical code for astrophysical flows in two dimensions II. The magnetohydrodynamical algorithms and tests. Astrophys. J. 80, (Suppl.), 791.