Lellouch, E.; Moreno, R.; Orton, G. S.; Feuchtgruber, H.; Cavalié, T.; Moses, J. I.; Hartogh, P.; Jarchow, C.; Sagawa, H.: New constraints on the CH4 vertical profile in Uranus and Neptune from Herschel observations. Astronomy and Astrophysics 579, A121 (2015)
Mandt, K. E.; Mousis, O.; Marty, B.; Cavalié, T.; Harris, W.; Hartogh, P.; Willacy, K.: Constraints from Comets on the Formation and Volatile Acquisition of the Planets and Satellites. Space Science Reviews 197, pp. 297 - 342 (2015)
Medvedev, A. S.; Gonzalez-Galindo, F.; Yigit, E.; Feofilov, A. G.; Forget, F.; Hartogh, P.: Cooling of the Martian thermosphere by CO2 radiation and gravity waves: An intercomparison study with two general circulation models. Journal Geophysical Research 120, pp. 913 - 927 (2015)
Rezac, L.; Hartogh, P.; Gusten, R.; Wiesemeyer, H.; Hubers, H.-W.; Jarchow, C.; Richter, H.; Klein, B.; Honingh, N.: First detection of the 63um atomic oxygen line in the thermosphere of Mars with GREAT/SOFIA. Astronomy and Astrophysics 580, L10 (2015)
Sonnemann, G. R.; Hartogh, P.; Berger, U.; Grygalashvyly, M.: Hydroxyl layer: trend of number density and intra-annual variability. Annales Geophysicae 33, pp. 749 - 767 (2015)
Villanueva, G. L.; Mumma, M. J.; Novak, R. E.; Käufl, H. U.; Hartogh, P.; Encrenaz, T.; Tokunaga, A.; Khayat, A.; Smith, M. D.: Strong water isotopic anomalies in the martian atmosphere: Probing current and ancient reservoirs. Science 348, aaa3630 (2015)
Yiğit, E.; Medvedev, A. S.; Hartogh, P.: Gravity waves and high-altitude CO2 ice cloud formation in the Martian atmosphere. Geophysical Research Letters 42, pp. 4294 - 4300 (2015)
Bockelée-Morvan, D.; Biver, N.; Crovisier, J.; Lis, D. C.; Hartogh, P.; Moreno, R.; de Val-Borro, M.; Blake, G. A.; Szutowicz, S.; Boissier, J.et al.; Cernicharo, J.; Charnley, S. B.; Combi, M.; Cordiner, M. A.; de Graauw, T.; Encrenaz, P.; Jarchow, C.; Kidger, M.; Küppers, M.; Milam, S. N.; Müller, H. S. P.; Phillips, T. G.; Rengel, M.: Searches for HCl and HF in comets 103P/Hartley 2 and C/2009 P1 (Garradd) with the Herschel Space Observatory. Astronomy and Astrophysics 562, A5 (2014)
Cavalié, T.; Moreno, R.; Lellouch, E.; Hartogh, P.; Venot, O.; Orton, G.; Jarchow, C.; Encrenaz, T.; Selsis, F.; Hersant, F.et al.; Fletcher, L.: The first submillimeter observation of CO in the stratosphere of Uranus. Astronomy and Astrophysics 562, A33 (2014)
de Val-Borro, M.; Bockelée-Morvan, D.; Jehin, E.; Hartogh, P.; Opitom, C.; Szutowicz, S.; Biver, N.; Crovisier, J.; Lis, D. C.; Rezac, L.et al.; de Graauw, T.; Hutsemékers, D.; Jarchow, C.; Kidger, M.; Küppers, M.; Lara, L. M.; Manfroid, J.; Rengel, M.; Swinyard, B. M.; Teyssier, D.; Vandenbussche, B.; Waelkens, C.: Herschel observations of gas and dust in comet C/2006 W3 (Christensen) at 5 AU from the Sun. Astronomy and Astrophysics 564, A124 (2014)
Grygalashvyly, M.; Sonnemann, G. R.; Lübken, F.-J.; Hartogh, P.; Berger, U.: Hydroxyl layer: Mean state and trends at midlatitudes. Journal Geophysical Research 119 (21), pp. 12391 - 12419 (2014)
Kuroda, T.; Medvedev, A. S.; Hartogh, P.: Parameterization of radiative heating and cooling rates in the stratosphere of Jupiter. Icarus 242, pp. 149 - 157 (2014)
Peters, D. H. W.; Hallgren, K.; Lübken, F.-J.; Hartogh, P.: Subseasonal variability of water vapor in the upper stratosphere/lower mesosphere over Northern Europe in winter 2009/2010. Journal of Atmospheric and Solar-Terrestrial Physics 114, pp. 9 - 18 (2014)
Rezac, L.; de Val-Borro, M.; Hartogh, P.; Cavalié, T.; Jarchow, C.; Rengel, M.; Dobrijevic, M.: New determination of the HCN profile in the stratosphere of Neptune from millimeter-wave spectroscopy. Astronomy and Astrophysics 563, A4 (2014)
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".