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)
Cavalié, T.; Billebaud, F.; Dobrijevic, M.; Fouchet, T.; Lellouch, E.; Encrenaz, T.; Brillet, J.; Moriarty-Schieven, G. H.; Wouterloot, J. G. A.; Hartogh, P.: First observation of CO at 345 GHz in the atmosphere of Saturn with the JCMT. New constraints on its origin. Icarus 203, pp. 531 - 540 (2009)
Grygalashvyly, M.; Sonnemann, G. R.; Hartogh, P.: Long-term behavior of the concentration of minor constituents in the mesosphere-a model study. Atmos. Chem. Phys. 9, pp. 2779 - 2792 (2009)
Kuroda, T.; Medvedev, A. S.; Hartogh, P.; Takahashi, M.: Correction to Semiannual oscillations in the atmosphere of Mars. Geophysical Research Letters 36, L01202 (2009)
Kuroda, T.; Medvedev, A. S.; Hartogh, P.; Takahashi, M.: On Forcing the Winter Polar Warmings in the Martian Middle Atmosphere during Dust storms. J. Meteorol. Soc. Japan 87, pp. 913 - 921 (2009)
Sonnemann, G. R.; Hartogh, P.: Upper stratospheric ozone decrease events due to a positive feedback between ozone and the ozone dissociation rate. Nonlinear Processes in Geophysics 16, pp. 409 - 418 (2009)
Sonnemann, G. R.; Hartogh, P.; Li, S.; Grygalashvyly, M.; Berger, U.: A QBO-signal in mesospheric water vapor measurements at ALOMAR (69.29 N, 16.03 E) and in model calculations by LIMA over a solar cycle. Atmos. Chem. Phys. Discuss. 9, pp. 883 - 903 (2009)
Yiğit, E.; Medvedev, A. S.; Aylward, A. D.; Hartogh, P.; Harris, M. J.: Modeling the effects of gravity wave momentum deposition on the general circulation above the turbopause. Journal Geophysical Research 114, D07101 (2009)
Bhardwaj, A.; Hartogh, P.; Kasaba, Y.; Wu, R. C. Y.: Advances in Planetary Sciences: AOGS 2007 (based on the Forth Annual Meeting of the AOGS, Bangkok, Thailand). Planetary and Space Science 56, p. 1675 (2008)
Analyzing the high spatial resolution solar Ca II H and K emission data obtained by the SUNRISE mission and building a model of other stars more active than the Sun
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).
First Light for Sunrise III: the first tests with real sunlight were successful. The balloon-borne solar observatory should be ready for launch at the end of May.