Cavalié, T.; Benmahi, B.; Hue, V.; Moreno, R.; Lellouch, E.; Fouchet, T.; Hartogh, P.; Rezac, L.; Greathouse, T. K.; Gladstone, G. R.et al.; Sinclair, J. A.; Dobrijevic, M.; Billebaud, F.; Jarchow, C.: First direct measurement of auroral and equatorial jets in the stratosphere of Jupiter. Astronomy and Astrophysics 647, L8 (2021)
Benmahi, B.; Cavalié, T.; Dobrijevic, M.; Biver, N.; Bermudez-Diaz, K.; Sandqvist, A.; Lellouch, E.; Moreno, R.; Fouchet, T.; Hue, V.et al.; Hartogh, P.; Billebaud, F.; Lecacheux, A.; Hjalmarson, Å.; Frisk, U.; Olberg, M.: Monitoring of the evolution of H2O vapor in the stratosphere of Jupiter over an 18-yr period with the Odin space telescope. Astronomy and Astrophysics 641, A140 (2020)
Ilyushin, Y. A.; Hartogh, P.: Submillimeter Wave Instrument radiometry of the Jovian icy moons: Numerical simulation of the microwave thermal radiative transfer and Bayesian retrieval of the physical properties. Astronomy and Astrophysics 644, A24 (2020)
Skorov, Y. V.; Keller, H. U.; Mottola, S.; Hartogh, P.: Near-perihelion activity of comet 67P/Churyumov–Gerasimenko. A first attempt of non-static analysis. Monthly Notices of the Royal Astronomical Society 494 (3), pp. 3310 - 3316 (2020)
Zhao, Y.; Rezac, L.; Hartogh, P.; Ji, J.; Marschall, R.; Keller, H. U.: Constraining spatial pattern of early activity of comet 67P/C–G with 3D modelling of the MIRO observations. Monthly Notices of the Royal Astronomical Society 494 (2), pp. 2374 - 2384 (2020)
Biver, N.; Bockelée-Morvan, D.; Hofstadter, M.; Lellouch, E.; Choukroun, M.; Gulkis, S.; Crovisier, J.; Schloerb, F. P.; Rezac, L.; von Allmen, P.et al.; Lee, S.; Leyrat, C.; Ip, W. H.; Hartogh, P.; Encrenaz, P.; Beaudin, G.; the MIRO Team: Long-term monitoring of the outgassing and composition of comet 67P/Churyumov-Gerasimenko with the Rosetta/MIRO instrument. Astronomy and Astrophysics 630, A19 (2019)
Jesch, D.; Medvedev, A. S.; Castellini, F.; Yiğit, E.; Hartogh, P.: Density Fluctuations in the Lower Thermosphere of Mars Retrieved From the ExoMars Trace Gas Orbiter (TGO) Aerobraking. Atmosphere 10 (10), 620 (2019)
Rezac, L.; Zhao, Y.; Hartogh, P.; Ji, J.; Marshall, D. W.; Shi, X.: Three-dimensional analysis of spatial resolution of MIRO/Rosetta measurements at 67P/Churyumov-Gersimenko. Astronomy and Astrophysics 630, A34 (2019)
Shaposhnikov, D. S.; Medvedev, A. S.; Rodin, A. V.; Hartogh, P.: Seasonal Water “Pump” in the Atmosphere of Mars: Vertical Transport to the Thermosphere. Geophysical Research Letters 46 (8), pp. 4161 - 4169 (2019)
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.