On the formation of Io-related Jovian discrete auroral phenomena

Advances in Space Research

Volumn 21, Issue 11, 1998, Pages 1469-1473

  Kopp, A ^a   Birk, G T ^b   Otto, A ^c  

^a MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

^b UNIVERSITY OF MUNICH   (Germany)

^c UNIVERSITY OF ALASKA FAIRBANKS   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0040577247     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/S0273-1177(98)00024-6     Document Type: Article

References (10)

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4. Kopp, A, The influence of mass loading effects on the electrodynamic interaction between Jupiter and Io, Adv. Space Res., this issue (1997)
5. Kopp, A., G.T. Birk and A. Otto, On the formation of Io-induced acceleration regions related to Jovian aurora, Planet. Space Sci., in press (1997)
6. Linker, J.A., M.G. Kivelson and R.J. Walker, A three-dimensional MHD simulation of plasma flow past Io, J. Geophys. Res. 96, 21037 (1991)
7. Neubauer, F.M., Nonlinear standing Alfvén wave current system at Io: Theory, J. Geophys. Res. 85, 1171 (1980)
8. Otto, A., 3D resistive MHD computations of magnetospheric physics, Comput. Phys. Commun. 59, 185, 1990.
9. Schindler, K., M. Hesse and J. Birn, Magnetic field-aligned electric potentials in nonideal plasma flows, Astrophys. J. 380, 293 (1991)
10. Wilson, J.K. and N.M. Schneider, Io's sodium directional features: evidence for ionospheric escape, J. Geophys. Res., in press, (1997)