Heber, B.; Kopp, A.; Fichtner, H.; Ferreira, S. E. S.: On the determination of energy spectra of MeV electrons by the Ulysses COSPIN/KET. Advances in Space Research 35 (4), pp. 605 - 610 (2005)
Kopp, A.; Ip, W.-H.: Resistive MHD simulations of Ganymede's magnetosphere 1: Time variabilities of the magnetic field topology. Journal Geophysical Research 107 (A12), 1490 (2002)
Ip, W.-H.; Kopp, A.; Lara, L. M.; Rodrigo, R.: Pluto's ionospheric models and solar wind interaction. Advances in Space Research 26 (10) (10), pp. 1559 - 1563 (2000)
Ip, W.-H.; Kopp, A.; Lara, L. M.; Rodrigo, R.: Pluto's ionospheric models and solar wind interaction. Advances in Space Research 26 (10) (10), pp. 1559 - 1563 (2000)
Ip, W.-H.; Kopp, A.; Williams, D. J.; McEntire, R. W.; Mauk, B. H.: Magnetospheric ion sputtering: The case of Europa and its surface age. Advances in Space Research 26 (10), pp. 1649 - 1652 (2000)
Schröer, A.; Kopp, A.: A three-fluid system of equations describing dusty magnetoplasmas with dynamically important dust and ion components. Physics of Plasmas 7 (8), pp. 3468 - 3471 (2000)
Kopp, A.: The influence of mass loading effects on the electrodynamical interaction between Jupiter and Io. Advances in Space Research 21 (11), pp. 1475 - 1478 (1998)
Kopp, A.; Birk, G. T.; Otto, A.: On the formation of Io-related Jovian discrete auroral phenomena. Advances in Space Research 21 (11), pp. 1469 - 1473 (1998)
Kopp, A.; Birk, G. T.; Otto, A.: On the formation of Io-induced acceleration regions related to Jovian aurora. Planetary and Space Science 46, pp. 405 - 415 (1998)
Shukla, P. K.; Birk, G. T.; Kopp, A.: Some remarks on the generation and dissipation of magnetic fields in dusty plasmas. Physica Scripta T74, pp. 82 - 85 (1998)
Kopp, A.; Schröer, A.; Birk, G. T.; Shukla, P. K.: Fluid equations governing the dynamics and energetics of partially ionized dusty magnetoplasmas. Physics of Plasmas 4, pp. 4414 - 4418 (1997)
Analyzing the high spatial resolution solar Ca II H and K emission data obtained by the SUNRISE mission and building a model of other stars more active than the Sun
For PhD students whose project is already funded and who are applying for admission to the IMPRS, or for applicants who want to bring their own funding and their own project idea to the IMPRS.