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)
The dwarf planet is a bizarre, cryovolcanic world. However, the organic deposits discovered on its surface so far are unlikely to originate from its interior.
The Uranian magnetic field is more expansive than previously thought, according to newly analyzed data from Voyager 2, making it easier to search for moons with oceans.
The Planetary Plasma Environments group (PPE) has a strong heritage in the exploration of planetary magnetospheres and space plasma interactions throughout the solar system. It has contributed instruments to several past missions that flew-by or orbited Jupiter (Galileo, Cassini, Ulysses). The PPE participates in the JUICE mission by contributing hardware and scientific expertise to the Particle Environment Package (PEP).