Birk, G. T.; Kopp, A.; Shukla, P. K.: Generalized magnetohydrodynamic equations for partially ionized dusty magnetoplasmas. Physics of Plasmas 3, pp. 3564 - 3572 (1996)
Birk, G. T.; Kopp, A.; Shukla, P. K.; Morfill, G.: Nonlinear fluid equations for low-frequency phenomena in partially ionized dusty magnetoplasmas. Physica Scripta 54, pp. 625 - 626 (1996)
Kopp, A.: Modifications of the electrodynamic interaction between Jupiter and Io due to mass loading effects. Journal Geophysical Research 101, pp. 24943 - 24954 (1996)
Preusse, S.; Kopp, A.; Büchner, J.; Motschmann, U.: Magnetic communication scenarios for close-in extrasolar planets. In: Status and prospects for hot Jupiter studies, Haute Provence Observatory Colloquium, August 22-25, 2005, pp. 1 - 8. (2005)
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