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)
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)
Sonnemann, G. R.; Hartogh, P.; Grygalashvyly, M.; Song, L.; Berger, U.: The quasi 5-day signal in the mesospheric water vapor concentration at high latitudes in 2003 - A comparison between observations at ALOMAR and calculations. Journal Geophysical Research 113, D04101 (2008)
Grygalashvyly, M.; Sonnemann, G. R.; Hartogh, P.: Long-term trends of the concentration of the minor constituents in the mesosphere - a model study. Atmos. Chem. Phys. Discuss. 7, pp. 15453 - 15494 (2007)
Hartogh, P.; Medvedev, A. S.; Jarchow, C.: Middle atmosphere polar warmings on Mars: Simulations and study on the validation with submillimeter observations. Planetary and Space Science 55, pp. 1103 - 1112 (2007)
Kuroda, T.; Medvedev, A. S.; Hartogh, P.; Takahashi, M.: Seasonal changes of the baroclinic wave activity in the northern hemisphere of Mars simulated with a GCM. Geophysical Research Letters 34, L09203 (2007)
Kutepov, A. A.; Feofilov, A. G.; Medvedev, A. S.; Pauldrach, A. W. A.; Hartogh, P.: Small-scale temperature fluctuations associated with gravity waves cause additional radiative cooling of the mesopause region. Geophysical Research Letters 34, L24807 (2007)
Medvedev, A. S.; Hartogh, P.: Winter polar warmings and the meridional transport on Mars simulated with a general circulation model. Icarus 186, pp. 97 - 110 (2007)
Sonnemann, G. R.; Hartogh, P.; Jarchow, C.; Grygalashvyly, M.; Berger, U.: On the winter anomaly of the night-to-day ratio of ozone in the middle to upper mesosphere in middle to high latitudes. Advances in Space Research 40, pp. 846 - 854 (2007)
Graf, U.; Heyminck, S.; Güsten, R.; Hartogh, P.; Hübers, H.-W.; Jacobs, K.; Phillip, M.; Rabanus, D.; Röser, H.-P.; Stutzki, J.et al.; van der Wal, P.; Wagner-Gentner, A.: GREAT: the German first light heterodyne instrument for SOFIA. Proceedings of the SPIE 6275, 62750K (2006)
Sonnemann, G. R.; Grygalashvyly, M.; Hartogh, P.; Jarchow, C.: Behaviour of mesospheric ozone under nearly polar night conditions. Advances in Space Research 38, pp. 2402 - 2406 (2006)
Villanueva, G.; Hartogh, P.: The high resolution chirp transform spectrometer for the SOFIA-GREAT instrument. Experimental Astronomy 18, pp. 77 - 91 (2006)
Villanueva, G. L.; Hartogh, P.; Reindl, L.: A Digital Dispersive Matching Network for SAW Devices in Chirp Transform Spectrometers. IEEE Trans. Microw. Theory Tech. 54 (4), pp. 1415 - 1424 (2006)
Hartogh, P.; Medvedev, A. S.; Kuroda, T.; Saito, R.; Villanueva, G.; Feofilov, A. G.; Kutepov, A. A.; Berger, U.: Description and climatology of a new general circulation model of the Martian atmosphere. Journal Geophysical Research 110, E11008 (2005)
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.