Choukroun, M.; Altwegg, K.; Kührt, E.; Biver, N.; Bockelée-Morvan, D.; Drążkowska, J.; Hérique, A.; Hilchenbach, M.; Marschall, R.; Pätzold, M.et al.; Taylor, M. G. G. T.; Thomas, N.: Dust-to-Gas and Refractory-to-Ice Mass Ratios of Comet 67P/Churyumov-Gerasimenko from Rosetta Observations. Space Science Reviews 216, 44 (2020)
Czechowski, A.; Bzowski, M.; Sokół, J. M.; Kubiak, M. A.; Heerikhuisen, J.; Zirnstein, E. J.; Pogorelov, N. V.; Schwadron, N. A.; Hilchenbach, M.; Grygorczuk, J.et al.; Zank, G. P.: Heliospheric Structure as Revealed by the 3–88 keV H ENA Spectra. The Astrophysical Journal 888 (1), 1 (2020)
Gardner, E.; Lehto, H. J.; Lehto, K.; Fray, N.; Bardyn, A.; Lonnberg, T.; Merouane, S.; Isnard, R.; Cottin, H.; Hilchenbach, M.et al.; the Cosima Team: The detection of solid phosphorus and fluorine in the dust from the coma of comet 67P/Churyumov-Gerasimenko. Monthly Notices of the Royal Astronomical Society 499 (2), pp. 1870 - 1873 (2020)
Kimura, H.; Hilchenbach, M.; Merouane, S.; Paquette, J.; Stenzel, O. J.: The morphological, elastic, and electric properties of dust aggregates in comets: A close look at COSIMA/Rosetta’s data on dust in comet 67P/Churyumov-Gerasimenko. Planetary and Space Science 181, 104825 (2020)
Langevin, Y.; Merouane, S.; Hilchenbach, M.; Vincendon, M.; Hornung, K.; Engrand, C.; Schulz, R.; Kissel, J.; Ryno, J.: Optical properties of cometary particles collected by COSIMA: Assessing the differences between microscopic and macroscopic scales. Planetary and Space Science 182, 104815 (2020)
Ellerbroek, L. E.; Gundlach, B.; Landeck, A.; Dominik, C.; Blum, J.; Merouane, S.; Hilchenbach, M.; John , H.; van Veen, H. A.: The footprint of cometary dust analogues – II. Morphology as a tracer of tensile strength and application to dust collection by the Rosetta spacecraft. Monthly Notices of the Royal Astronomical Society 486 (3), pp. 3755 - 3765 (2019)
Czechowski, A.; Hilchenbach, M.; Hsieh, K. C.; Bzowski, M.; Grzedzielski, S.; Sokół, J. M.; Grygorczuk, J.: Structure of the heliosheath from HSTOF energetic neutral atoms measurements. Astronomy and Astrophysics 618, A26 (2018)
Paquette, J.; Engrand, C.; Hilchenbach, M.; Fray, N.; Stenzel, O. J.; Silen, J.; Rynö, J.; Kissel, J.; the COSIMA Team: The oxygen isotopic composition (18O/16O) in the dust of comet 67P/Churyumov-Gerasimenko measured by COSIMA on-board Rosetta. Monthly Notices of the Royal Astronomical Society 477 (3), pp. 3836 - 3844 (2018)
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.