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)
How does our star heat its outer atmosphere, the solar corona, to unimaginable temperatures of up to 10 million degrees Celsius? With unprecedented observational data from ESA's Solar Orbiter spacecraft and powerful computer simulations, ERC starting grant awardee Pradeep Chitta intends to bring new momentum to the search for the coronal heating mechanism.
The research group “Solar Lower Atmosphere and Magnetism” (SLAM) studies the conditions and dynamic processes in the atmospheric layer between the solar surface (photosphere) and the overlying chromosphere, an approximately 2000 km thick gas layer.
The main research fields of the department "Sun and Heliosphere" are covered by the research groups "Solar and Stellar Coronae", "Solar Lower Atmosphere and Magnetism", "Solar and Stellar Magnetohydrodynamics" and "Solar Variability and Climate".