Rengel, M.; Sagawa, H.; Hartogh, P.: Venusian Mesospheric thermal structure and winds from May 2009 SMT CO spectral- line observations. 40th COSPAR Scientific Assembly, Moscow, Russia (2014)
Rezac, L.; de Val-Borro, M.; Hartogh, P.; Cavalié, T.; Jarchow, C.; Rengel, M.; Dobrijevic, M.: New Determination of the HCN Profile in the Stratosphere of Neptune from Millimeter-wave Spectroscopy. Asia Oceania Geosciences Society (AOGS) 11th Annual Meeting, Sapporo, Japan (2014)
Hartogh, P.: Chirptransformations-Spektrometer für die passive Millimeterwellenradiometrie: Messungen der 142 GHz Emissionslinie des atmosphärischen Ozons. Dissertation, Georg-August-Universität Göttingen (1989)
Hartogh, P.: Raumflugtauglicher FM-Pulskompressionsempfänger mit Oberflächenwellenfiltern für die Millimeter- und Submillimeterwellenspektroskopie. Diploma, Georg-August-Universität Göttingen (1985)
Biver, N.; Bockelée-Morvan, D.; Moreno, R.; Crovisier, J.; Hartogh, P.; de Val-Borro, M.; Kidger, M.; Kueppers, M.; Szutowicz, S.; Lis, D. C.et al.; Blake, G. A.; Gonzalez, J. J.; Seargent, D. A. J.; Mattiazzo, M.: Comet C/2011 L4 (Panstarrs). Central Bureau Electronic Telegrams 3230, 1 (2012)
Meister, C.-V.; Hartogh, P.; Villanueva, G.; Berger, U.: Hydrodynamic model of the Martian atmosphere between near-surface layers and an altitude of about 130 km. Max-Planck-Institut für Aeronomie, Katlenburg-Lindau, Germany (2002)
Gulkis, S.; Forget, F.; Janssen, M.; Riley, L.; Hartogh, P.; Clancy, T.; Allen, M.; Frerking, M.: Microwave Investigation of the Martian Atmosphere and Surface. JPL, California Institute of Technology, Pasadena, CA, USA (2000)
Gurevich, A. V.; Borison, N. D.; Montecinos-Geisse, S. E.; Hartogh, P.: Artificial ozone layer. Max-Planck-Institut für Aeronomie, Katlenburg-Lindau, Germany (1995)
Lopez, J. E.; Montecinos, S. E.; Hartogh, P.: A photochemical model of the atmosphere. Max-Planck-Institut für Aeronomie, Katlenburg-Lindau, Germany (1995)
Hartogh, P.; Hartmann, G. K.; Heimesaat, G.: The use of Chirp-transform-spectrometers for real time Fouriertransform of stochastic signals. Max-Planck-Institut für Aeronomie, Katlenburg-Lindau, Germany (1989)
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).
Application deadline 1 October 2024. PhD projects in planetary science, solar and stellar physics, solar magnetism, heliophysics, helioseismology, asteroseismology, ...
Two scientific associations have awarded Prof. Dr. Thorsten Kleine the title "Geochemistry Fellow" for his contributions to the understanding of how the Solar System was formed.