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)
Images from ESA’s Solar Orbiter offer the best look yet at a source region of the solar wind - and challenge our view of the continuous particle stream from the Sun.
Deciphering the magnetic origins of the Sun's hot corona: developing a framework for coronal heating by probing the elusive photosphere-corona connection
Using unique observational data and computer simulations, the MPS scientist is striving to understand the incredibly hot temperatures in the solar corona.
For the first time, images of the Sun have been taken from a distance of only 77 million kilometres enabling a completely new view of our star possible.
In his doctoral thesis, Sudip Mandal investigated how special pressure waves help maintain temperatures of several million degrees in the outermost solar atmosphere.