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)
Heyminck, S.; Güsten, R.; Hartogh, P.; Hübers, H.-W.; Stutzki, J.; Graf, U. U.: GREAT: a first light instrument for SOFIA. Proceedings of the SPIE 7014, 701410 (2008)
Paganini, L.; Hartogh, P.; Reindl, L.: An improved method for nonlinearity detection applied to a new 400-MHz bandwidth Chirp transform spectrometer. Transactions on Systems, Signals & Devices 3 (4), pp. 1 - 15 (2008)
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)
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).
The MPS instruments on board ESA’s JUICE spacecraft have successfully completed their commissioning in space - and delivered their first observational data.
The launch was successful; the ESA’s space probe JUICE is now on its way to the Jupiter system. There, it will primarily study the gas giant's icy moons.
ESA's space probe is on the move: First it heads for the launch site in Kourou - and in April it will begin its long journey to Jupiter and its icy moons.