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)
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".