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)
Images from ESA’s Solar Orbiter offer the best look yet at a source region of the solar wind - and challenge our view of the continuous particle stream from the Sun.
Deciphering the magnetic origins of the Sun's hot corona: developing a framework for coronal heating by probing the elusive photosphere-corona connection
Using unique observational data and computer simulations, the MPS scientist is striving to understand the incredibly hot temperatures in the solar corona.
For the first time, images of the Sun have been taken from a distance of only 77 million kilometres enabling a completely new view of our star possible.
In his doctoral thesis, Sudip Mandal investigated how special pressure waves help maintain temperatures of several million degrees in the outermost solar atmosphere.