Schäfer, M.; Schäfer, T.; Izawa, M. R. M.; Cloutis, E. A.; Schröder, S. E.; Roatsch, T.; Preusker, F.; Stephan, K.; Matz, K.; Raymond, C. A.et al.; Russell, C. T.: Ceres’ spectral link to carbonaceous chondrites - Analysis of the dark background materials. Meteoritics and Planetary Science 53 (9), pp. 1925 - 1945 (2018)
Schäfer, T.; Nathues, A.; Mengel, K.; Izawa, M. R. M.; Cloutis, E. A.; Schäfer, M.; Hoffmann, M.: Spectral parameters for Dawn FC color data: Carbonaceous chondrites and aqueous alteration products as potential cerean analog materials. Icarus 265, pp. 149 - 160 (2016)
Izawa, M. R. M.; Schäfer, T.; Pietrasz, V. B.; Cloutis, E. A.; Mann, P.; Nathues, A.; Mengel, K.; Schäfer, M.; Thangjam, G.; Hoffmann, M.et al.; Tait, K. T.; Applin, D. M.: Effects of viewing geometry, aggregation state, and particle size on reflectance spectra of the Murchison CM2 chondrite deconvolved to Dawn FC band passes. Icarus 266, pp. 235 - 248 (2015)
Schäfer, M.; Nathues, A.; Williams, D. A.; Mittlefehldt, D. W.; Le Corre, L.; Buczkowski, D. L.; Kneissl, T.; Thangjam, G. S.; Hoffmann, M.; Schmedemann, N.et al.; Schäfer, T.; Scully, J. E. C.; Li, J.-Y.; Reddy, V.; Garry, W. B.; Krohn, K.; Yingst, R. A.; Gaskell, R. W.; Russell, C. T.: Imprint of the Rheasilvia impact on Vesta - Geologic mapping of quadrangles Gegania and Lucaria. Icarus 244, pp. 60 - 73 (2014)
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.