Lühr, H.; Wicht, J.; Gilder, S. A.; Holschneider, M.: General Introduction and Scientific Summary of the German Priority Program “PlanetMag”. In: Magnetic Fields in the Solar System: Planets, Moons and Solar Wind Interactions, pp. 1 - 6 (Eds. Lühr, H.; Wicht, J.; Gilder, S. A.; Holschneider, M.). Springer, Cham (2018)
Wicht, J.; French, M.; Stellmach, S.; Nettelmann, N.; Gastine, T.; Duarte, L.; Redmer, R.: Modeling the Interior Dynamics of Gas Planets. In: Magnetic Fields in the Solar System: Planets, Moons and Solar Wind Interactions, pp. 7 - 81 (Eds. Lühr, H.; Wicht, J.; Gilder, S. A.; Holschneider, M.). Springer, Cham (2018)
Wicht, J.; Stellmach, S.; Harder, H.: From fundamental cartesian model to 3d simulations of field reversals. In: Geomagnetic field variations (Eds. Glassmeier, K.-H.; Soffel, H.; Negendank, J.). Springer (2008)
Wicht, J.; Mandea, M.; Takahashi, F.; Christensen, U. R.; Matsushima, M.; Langlais, B.: The origin of Mercury's internal magnetic field. In: Mercury, pp. 79 - 108 (Eds. Balogh, A.; Ksanfomality, L.; von Steiger, R.). Springer, Dordrecht/Boston/London (2007)
Bossmann, A. B.; Wicht, J.; Gastine, T.; Christensen, U. R.: Magnetic field morphology of the ice giants linked to their internal structure. 5th Meeting of the DFG-SPP Planetary Magnetism, Nördlingen, Germany (2015)
The Sun’s planets and small objects have undergone substantial evolution. Deciphering the history of our cosmic home is not a simple task even though we now have access to a multitude of data gathered by space missions, remote observations, and laboratory studies of diverse samples. A significant fraction of materials available for the study of planetary bodies come from meteorites.
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).
The Solar Lower Atmosphere and Magnetism (SLAM) group covers many exciting subjects in solar physics, focussing on the development and testing of highly novel solar instrumentation, reduction and analysis of highest quality solar observations, or improving and developing advanced techniques for the analysis of solar observations.
The MPS is one of the leading institutes worldwide in building instruments for solar research, both for ground based observatories as well as for balloon and space-borne missions. Scientists and engineers of MPS conceive new observing methods and develop novel instruments of highest technological complexity. These instruments are built in house, tested, calibrated, and used at the best solar observatories in the world, or delivered to NASA and ESA to be launched to space.