Larsson, R.; Mendrok, J.; Kasai, Y.; Buehler, S. A.; Dieval, C.; Brain, D.; Hartogh, P.: Using Zeeman effect on molecular oxygen to measure Mars' crustal magnetism: Sensor requirements from simulated signal strengths. European Geosciences Union General Assembly, Vienna, Austria (2015)
Lee, S.; von Allmen, P.; Hofstadter, M.; Beaudin, G.; Biver, N.; Bockelee-Morvan, D.; Choukroun, M.; Crovisier, J.; Encrenaz, P.; Encrenaz, T.et al.; Frerking, M.; Gulkis, S.; Hartogh, P.; Ip, W. H.; Janssen, M.; Jarchow, C.; Keihm, S.; Lellouch, E.; Leyrat, C.; Rezac, L.; Schloerb, F. P.: Local and Diurnal Variation of Water Outgassing on Comet 67P/Churuymov-Gerasimenko Nucleus Observed from Rosetta/MIRO. 46th Lunar and Planetary Science Conference , The Woodlands, Texas (2015)
Mendrok, J.; Eriksson, P.; Buehler, S.; Perrin, A.; Hartogh, P.; Rezac, L.; Lemke, O.: Atmospheric radiative transfer generalised for use on Earth and other planets: ARTS 2.2. European Geosciences Union General Assembly, Vienna, Austria (2015)
O'Rourke, L.; Snodgrass, C.; de Val-Borro, M.; Biver, N.; Bockelée-Morvan, D.; Hsieh, H.; Teyssier, D.; Fernandez, Y.; Küppers, M.; Micheli, M.et al.; Hartogh, P.: Determination of an upper limit for the water outgassing rate of main-belt comet P/2012 T1 (PANSTARRS). European Geosciences Union General Assembly, Vienna, Austria (2015)
Rengel, M.; Sagawa, H.; Hartogh, P.: Hydrogen Cyanide in the Stratosphere of Titan. 12th Annual Meeting Asia Oceania Geosciences Society, Singapore (2015)
Rengel, M.; Sagawa, H.; Hartogh, P.: Hydrogen Cyanide in the Stratosphere of Titan. 12th Annual Meeting Asia Oceania Geosciences Society, Singapore (2015)
Rezac, L.; Hartogh, P.; Wiesemeyer, H.; Güsten, R.; Jarchow, C.: First Detection of the 63 Micron Oxygen Line in the Thermosphere of Mars with the GREAT Instrument. 12th Annual Meeting Asia Oceania Geosciences Society, Singapore (2015)
Villanueva, G. L.; Mumma, M. J.; Novak, R. E.; Kaufl, H. U.; Hartogh, P.; Encrenaz, T.; Tokunaga, A. T.; Khayat, A.; Smith, M. D.: The Evolution of the Water Reservoirs on Mars Revealed via D/H Isotopic Mapping. 46th Lunar and Planetary Science Conference, The Woodlands, Texas, USA (2015)
von Allem, P.; Lee, S.; Hofstadter, M.; Biver, N.; Bockelee-Morvan, D.; Choukroun, M.; Gulkis, S.; Hartogh, P.; Janssen, M.; Jarchow, C.et al.; Keihm, S.; Lellouch, E.; Leyrat, C.; Rezac, L.; Schloerb, P.; Crovisier, J.; Encrenaz, P.; Ip, W.: Spatial and Temporal Variations of the Near-Surface Thermal Properties of 67P/Churyumov-Gerasimenko Obtained from Continuum Observations with Microwave Instrument on the Rosetta Orbiter (MIRO). 46th Lunar and Planetary Science Conference, The Woodlands, Texas, USA (2015)
von Allmen, P.; Lee, S.; Gulkis, S.; Hofstadter, M.; Schloerb, P.; Biver, N.; Bockelée-Morvan, D.; Choukroun, M.; Hartogh, P.; Janssen, M.et al.; Jarchow, C.; Keihm, S.; Lellouch, E.; Leyrat, C.; Rezac, L.; Crovisier, J.; Encrenaz, P.; Encrenaz, T.; Ip, W.: Line Shape Analysis and Abundance Quantification for Methanol in the Comet 67P/Churuymov-Gerasimenko Coma Derived from Microwave Instrument on the Rosetta Orbiter (MIRO) Observations. European Geosciences Union General Assembly, Vienna, Austria (2015)
Becker, E.; Grygalashvyly, M.; Sonnemann, G. R.; Hartogh, P.; Jarchow, C.: GWS mixing and effective diffusivity concept for minor chemical constituents in the MLT. 11th Annual, Meeting Asia Oceania Geosciences Society, Sapporo, Japan (2014)
Biver, N.; Bockelée-Morvan, D.; Hartogh, P.; de Crovisier J.and Val-Borro, M.; Kidger, M.; Küppers, M.; Lis, D.; Moreno, R.; Szutowicz, S.; The HssO Team: Observations of ammonia in comets with Herschel. Asteroids, Comets, Meteors , Helsinki, Finland (2014)
Cavalié, T.; Hue, V.; Hartogh, P.; Lellouch, E.; Cassidy, T.; Dobrijevic, M.; Jarchow, C.; Moreno, R.: Is Enceladus Saturn's source of water? European Planetary Science Congress , Cascais, Portugal (2014)
Cavalié, T.; Venot, O.; Selsis, F.; Hersant, F.; Hartogh, P.: The Deep O/H Ratio in Uranus and Neptune from CO Spectroscopy and Thermochemical Modeling. Workshop on the Study of the Ice Giant Planets, Laurel, Maryland, USA (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".