Rengel, M.: La extraña química de la atmósfera de Titán vista con el Observatorio Espacial Herschel. Seminar at the Center of Physics, Caracas, Venezuela (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)
de Val-Borro, M.; Bockelée-Morvan, D.; Jehin, E.; Hartogh, P.; Opitom, C.; Szutowicz, S.; Biver, N.; Crovisier, J.; Lis, D.; Rezac, L.et al.; de Graauw, T.; Hutsemékers, D.; Jarchow, C.; Kidger, M. R.; Küppers, M.; Lara, L. M.; Manfroid, J.; Rengel, M.; Swinyard, B. M.; Teyssier, D.; Vandenbussche, B.; Waelkens, C.: Distant activity of comet C/2006 W3 (Christensen) as observed with Herschel. Asteroids, Comets, Meteors, Helsinki, Finland (2014)
Hartogh, P.; Rezac, L.; Moreno, R.; Lellouch, E.; Rengel, M.; Jarchow, C.; de Val-Borro, M.; Crovisier, J.; Biver, N.; Bockeleé-Morvan: Detection and characterization of Ganymede's and Callisto's water atmospheres. 11th Annual Meeting, Asia Oceania Geosciences Society, Sapporo, Japan (2014)
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)
Lara, L.-M.; Lellouch, E.; González, M.; Moreno, R.; Rengel, M.: Exploring external time-dependent sources of H2O into Titan's atmosphere. European Geosciences Union General Assembly 2014, Vienna, Austria (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)
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)
Rengel, M.; Reiners, A.; Shulyak, D.; Yan, F.; Khaimova, J.; Cont, D.; Gapp, C.: Investigating Physical and Chemical Mechanisms in Planetary Atmospheres and their impacts on the observables. Exoplanet III online, Heidelberg, Germany (2020)
Rengel, M.; Reiners, A.; Shulyak, D.; Yan, F.; Khaimova, J.; Cont, D.; Gapp, C.: Investigating Physical and Chemical Mechanisms of Planetary Atmospheres: A DFG Project Characterizing Planetary Atmospheres Inside and Outside Our Solar System. Tackling the Complexities of Substellar Objects: From Brown Dwarfs to (exo-)Planets, Leiden, The Netherlands (2020)
Rengel, M.: Chemical compositions of atmospheres of planets of the Solar System from spectroscopy. ARIEL Science, Mission and Community Conference 2020, Noordwijk, Netherlands (2020)
First Light! The spectro-polarimeter of the world's largest solar telescope in Hawaii looks at the Sun for the first time. The instrument was developed in Germany.
Dr. Theodosios Chatzistergos receives award by the European Space Weather and Space Climate Association for his research findings on the historical activity of the Sun.
The Zdenĕk Švetska Senior Prize of the Solar Physics Division of the European Physical Society (EPS) recognizes Solanki’s pioneering contributions to solar research.
The magnetic field in the solar atmosphere exceeds the geomagnetic field strength by four orders of magnitude. It greatly influences the processes of energy transport within the solar atmosphere, and dominates the morphology of the solar chromosphere and corona. Kinetic energy from convective motions in the Sun can be efficiently stored in magnetic fields and subsequently released - to heat the solar corona to several million degrees or to blast off coronal mass ejections.
Application deadline 1 October 2024. PhD projects in planetary science, solar and stellar physics, solar magnetism, heliophysics, helioseismology, asteroseismology, ...