Medvedev, A. S.; Yiğit, E.; Kuroda, T.; Hartogh, P.: Response of the Martian upper atmosphere to lower atmospheric dust storms: GCM study. Fifth international workshop on the Mars Atmosphere: Modelling and observations, Oxford, UK (2014)
Medvedev, A. S.; Yiğit, E.; Kuroda, T.; Hartogh, P.: Dynamical coupling between the lower Martian atmosphere and thermosphere. 40th COSPAR Scientific Assembly, Moscow, Russia (2014)
Medvedev, A.; Yiğit, E.; Kuroda, T.; Hartogh, P.: Influence of global dust storms on the mesosphere and lower thermosphere of Mars. European Planetary Science Congress 2014, Cascais, Portugal (2014)
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 the main-belt comet P/2012 T1 (PanSTARRS). Asteroids, Comets, Meteors, Helsinki, Finland (2014)
Orton, G.; Fletcher, L. N.; Feuchtgruber, H.; Lellouch, E.; Moreno, R.; Encrenaz, T.; Hartogh, P.; Jarchow, C.; Swinyard, B.; Cavalié, T.et al.; Moses, J.; Burgdorf, M.; Hammel, H.; Line, M.; Mainzer, A. K.; Hofstadter, M.; Sandell, G. H.; Dowell, C. D.; Pantin, E.; Fujiyoshi, T.: Models for Temperature and Composition in Uranus from Spitzer, Herschel and Ground-Based Infrared through Millimeter Observations. American Astronomical Society, DPS meeting #46, Tucson, AZ, USA (2014)
Orton, G.; Fletcher, L.; Feuchtgruber, H.; Lellouch, E.; Moreno, R.; Hartogh, P.; Jarchow, C.; Swinyard, B.; Moses, J.; Burgdorf, M.et al.; Hammel, H.; Line, M.; Mainzer, A.; Hofstadter, M.; Sandell, G.; Dowell, C.: Models for Temperature and Composition in Uranus from Spitzer, Herschel and Ground-Based Infrared through Millimeter Observations. EGU General Assembly, Vienna, Austria (2014)
Rengel, M.; Moreno, R.; Courtin, R.; Lellouch, E.; Sagawa, H.; Hartogh, P.; Swinyard, B.; Lara, L.; Feuchtgruber, H.; Jarchow, C.et al.; Fulton, T.; Cernicharo, J.; Bockelée-Morvan, D.; Biver, N.; Banaszkiewicz, M.; González, A.: Tracing the gas composition of Titan's atmosphere with Herschel: Advances and Discoveries. 46th Annual Meeting of the Division for Planetary Sciences, Tucson, AZ, USA (2014)
Rengel, M.; Sagawa, H.; Hartogh, P.: The HCN distribution in the stratosphere of Titan: an intercomparison between the HCN distributions obtained with Herschel/PACS and APEX-2. Asia Oceania Geosciences Society (AOGS) 11th Annual Meeting, Sapporo, Japan (2014)
Rezac, L.; Jarchow, C.; Hartogh, P.: Inversion simulations for the MIRO instrument on board of the Rosetta orbiter: characterizing the information content. 11th Annual Meeting, Asia Oceania Geosciences Society, Sapporo, Japan (2014)
Sagawa, H.; Hartogh, P.; Rengel, M.; Güsten, R.: Submillimeter Observations of Chlorine-bearing Molecules in Venus Middle Atmosphere. Asia Oceania Geosciences Society (AOGS) 11th Annual Meeting, Sapporo, Japan (2014)
Sethunadh, J. A.; Medvedev, A. S.; Hartogh, P.: General circulation modeling of the Jovian stratosphere. European Planetary Science Congress 2014, Cascais, Portugal (2014)
Villanueva, G. L.; Mumma, M. J.; Novak, R. E.; Käufl, H.-U.; Hartogh, P.; Encrenaz, T.; Tokunaga, A.; Khayat, A.: Revealing the water cycle on Mars via D/H isotopic measurements. American Astronomical Society, DPS meeting #46, Tucson, AZ, USA (2014)
Thomas, B.; Philipp, M.; Lichius, K.; Trasatti, M.; Maestrini, A.; Miettinen , E.P.; Hartogh, P.: Digitally tunable 150 GHz Local Oscillator chain for the Submillimeter Wave Instrument onboard the ESA JUICE mission. 30th International Symposium on Space Terahertz Technology, Gothenburg, Sweden (2019)
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".