Rengel, M.; Sagawa, H.; Hartogh, P.: Retrieval Simulations of Atmospheric Gases from Herschel Observations of Titan. Advances in Geosciences, pp. 335 - 348 (2010)
Sagawa, H.; Hartogh, P.; Rengel, M.; de Lange, A.; Cavalié, T.: Preparation for the solar system observations with Herschel: Simulation of Jupiter observations with PACS. Planetary and Space Science 58, pp. 1692 - 1698 (2010)
Sagawa, H.; Hartogh, P.; Rengel, M.; Lange, A.; Cavalié, T.: Preparation for the solar system observations with Herschel: Simulation of Jupiter observations with PACS. Planetary and Space Science 58 (13), pp. 1692 - 1698 (2010)
Rengel, M.; Hartogh, P.; Jarchow, C.: HHSMT observations of the Venusian mesospheric temperature, winds, and CO abundance around the MESSENGER flyby. Planetary and Space Science 56, pp. 1688 - 1695 (2008)
Rengel, M.; Hartogh, P.; Jarchow, C.: Mesospheric vertical thermal structure and winds on Venus from HHSMT CO spectral-line observations. Planetary and Space Science 56, pp. 1368 - 1384 (2008)
Tachihara, K.; Rengel, M.; Nakajima, Y.; Yamaguchi, N.; André, P.; Neuhäuser, R.; Onishi, T.; Fukui, Y.; Mizuno, A.: Gas and Dust Condensations and a Peculiar Class 0 Object in the Lupus 3 Star-Forming Cloud. Astrophysical Journal 659, pp. 1382 - 1393 (2007)
Limaye, S.; Rengel, M.: 5 - Atmospheric circulation and dynamics - Observations and knowledge gaps. In: Towards understanding the climate of Venus: Applications of terrestrial models to our sister planet, pp. 55 - 72 (Eds. Bengtsson, L.; Bonnet, R.-M.; Grinspoon, D.; Koumoutsaris, S.; Lebonnois, S. et al.). Springer-Verlag, Berlin (2012)
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Rengel, M.; Küppers, M.; Keller, H. U.; Gutierrez, P.: Modeling of the Terminal Velocities of the Dust Ejected Material by the Impact. In: Deep Impact as a World Observatory Event - Synergies in Space, Time (Eds. Kaeufl, H. U.; Sterken, C.). Springer Verlag (2007)
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The Uranian magnetic field is more expansive than previously thought, according to newly analyzed data from Voyager 2, making it easier to search for moons with oceans.
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).