Hicks, M. D.; Buratti, B. J.; Lawrence, K. J.; Hillier, J.; Li, J.-Y.; Reddy, V.; Schröder, S.; Nathues, A.; Hoffmann, M.; Le Corre, L.et al.; Duffard, R.; Zhao, H.-B.; Raymond, C.; Russell, C.; Roatsch, T.; Jaumann, R.; Rhoades, H.; Mayes, D.; Barajas, T.; Truong, T.-T.; Foster, J.; McAuley, A.: Spectral diversity and photometric behavior of main-belt and near-Earth vestoids and (4) Vesta: A study in preparation for the Dawn encounter. Icarus 235, pp. 60 - 74 (2014)
Karkoschka, E.; Schröder, S. E.; Tomasko, M. G.; Keller, H. U.: The reflectivity spectrum and opposition effect of Titan's surface observed by Huygens' DISR spectrometers. Planetary and Space Science 60, pp. 342 - 355 (2012)
McCord, T. B.; Li, J.-Y.; Combe, J.-P.; McSween, H. Y.; Jaumann, R.; Reddy, V.; Tosi, F.; Williams, D. A.; Blewett, D. T.; Turrini, D.et al.; Palomba, E.; Pieters, C. M.; De Sanctis, M. C.; Ammannito, E.; Capria, M. T.; Le Corre, L.; Longobardo, A.; Nathues, A.; Mittlefehldt, D. W.; Schroeder, S. E.; Hiesinger, H.; Beck, A. W.; Capaccioni, F.; Carsenty, U.; Keller, H. U.; Denevi, B. W.; Sunshine, J. M.; Raymond, C. A.; Russell, C. T.: Dark material on Vesta from the infall of carbonaceous volatile-rich material. Nature 491, pp. 83 - 86 (2012)
Mittlefehldt, D. W.; Beck, A. W.; Ammannito, E.; Carsenty, U.; De Sanctis, M. C.; Le Corre, L.; McCoy, T. J.; Reddy, V.; Schröder, S. E.: Geologic structures in crater walls on Vesta. Meteorit. Planet. Sci. 47, p. A275 - A275 (2012)
Schröder, S. E.; Keller, H.-U.: The reflectance spectrum of Titan's surface at the Huygens landing site determined by the Descent Imager/Spectral Radiometer. Planetary and Space Science 56, pp. 753 - 769 (2008)
Karkoschka, E.; Tomasko, M. G.; Doose, L. R.; See, C.; McFarlane, E. A.; Schröder, S. E.; Rizk, B.: DISR imaging and the geometry of the descent of the Huygens probe within Titan's atmosphere. Planetary and Space Science 55 (13), pp. 1896 - 1935 (2007)
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).
Inversion codes are used to aid the detailed interpretation of solar spectro-polarimetric data. This computer code attempts to find the atmospheric structure that produced an observed spectrum by minimizing the difference between the observed spectrum and a Stokes spectrum.
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.
Karen Harvey solar physics prize 2020 for Prof. Dr. Tian who studies dynamic phenomena in the Sun’s atmosphere; his research group is a partner group of the Max Planck Institute for Solar System Research.
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.