Rengel, M.; Shulyak, D.; Hartogh, P.; Sagawa, H.; Moreno, R.; Jarchow, C.: Ground-based HCN submillimetre measurements in Titan's atmosphere: an intercomparison with Herschel observations. Astronomy and Astrophysics 658, p. A88 (2022)
Hartogh, P.; Jarchow, C.; Lellouch, E.; de Val-Borro, M.; Rengel, M.; Moreno, R.; Medvedev, A. S.; Sagawa, H.; Swinyard, B. M.; Cavalié, T.et al.; Lis, D. C.; Błecka, M. I.; Banaszkiewicz, M.; Bockelée-Morvan, D.; Crovisier, J.; Encrenaz, T.; Küppers, M.; Lara, L.-M.; Szutowicz, S.; Vandenbussche, B.; Bensch, F.; Bergin, E. A.; Billebaud, F.; Biver, N.; Blake, G. A.; Blommaert, J. A. D. L.; Cernicharo, J.; Decin, L.; Encrenaz, P.; Feuchtgruber, H.; Fulton, T.; de Graauw, T.; Jehin, E.; Kidger, M.; Lorente, R.; Naylor, D. A.; Portyankina, G.; Sánchez-Portal, M.; Schieder, R.; Sidher, S.; Thomas, N.; Verdugo, E.; Waelkens, C.; Whyborn, N.; Teyssier, D.; Helmich, F.; Roelfsema, P.; Stutzki, J.; Leduc, H. G.; Stern, J. A.: Herschel/HIFI observations of Mars: First detection of O2 at submillimetre wavelengths and upper limits on HCl and H2O2. Astronomy and Astrophysics 521, L49 (2010)
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)
Takagi, M.; Suzuki, K.; Sagawa, H.; Baron, P.; Mendrok, J.; Kasai, Y.; Matsuda, Y.: Influence of CO2 line profiles on radiative and radiative-convective equilibrium states of the Venus lower atmosphere. Journal Geophysical Research 115, E06014 (2010)
Rengel, M.; Shulyak, D.; Hartogh, P.; Sagawa, H.; Moreno, R.; Jarchow, C.; Breitschwerdt, D.: Ground-based measurements of HCN abundances in the stratosphere of Titan: an inter-comparison with Herschel observations. Asia Oceania Geosciences Society 18th Annual Meeting (AOGS2021), Online (2021)
Hartogh, P.; Sagawa, H.; Rengel, M.: APEX submillimetre observations of HCl and HDO in the mesosphere of Venus. 40th COSPAR Scientific Assembly, Moscow, Russia (2014)
Lellouch, E.; Hartogh, P.; Moreno, R.; Billebaud, F.; Bockelée-Morvan, D.; Biver, N.; Cassidy, T.; Courtin, R.; Crovisier, J.; Dobrijevic, M.et al.; Feuchtgruber, H.; González, A.; Greathouse, T.; Jarchow, C.; Kidger, M.; Lara, L. M.; Rengel, M.; Orton, G.; Sagawa, H.; de Val-Borro, M.; Cavalié, T.: The origin of external oxygen in Jupiter and Saturn's environments. Semaine de l'Astrophysique Francaise, Paris, France (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)
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".
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.