Rengel, M.; Hodapp, K.; Eisloeffel, J.: SK 1: A Possible Case of Triggered Star Formation in Perseus. In: Triggered Star Formation in a Turbulent Interstellar Medium (IAU S237) (Eds. Elmegreen, B.; Palous, J.). Cambridge University Press (2007)
Rengel, M.; Froebrich, D.; Eislöffel, J.; Hodapp, K.: Submillimetre Imaging of Deeply Embedded Outflow Sources and Class 0 Sources. In: Abstracts of Contributed Talks and Posters presented at the Annual Scientific Meeting of the Astronomische Gesellschaft at the Joint European and National Meeting JENAM 2001. (2001)
Rengel, M.: Caracterizando las atmósferas de los planetas: espectros, procesos y estructura. BrainGain-PWF Venezuelan Physics School 2022, Online (2022)
Rengel, M.: Atmospheric Characterization of (Exo)Planets: Spectra, Processes and Structure. Maynooth University, Department of Experimental Physics, Ireland, Online (2021)
Rengel, M.: Júpiter y sus lunas heladas: lo que nos enseñará la misión espacial JUICE. Parque Explora y Planetario de Medellín, Colombia, Online (2021)
Rengel, M.: Investigating physico-chemical mechanisms in (exo)planetary atmospheres and their impact on the observables. DFG SPP1992 virtual all-hands-on-deck meeting, Online (2021)
Gapp, C.; Rengel, M.; Hartogh, P.; Sagawa, H.; Feuchtgruber, H.; Lellouch, E.; Villanueva, G.: Deciphering Jupiter’s atmospheric chemistry as a benchmark for extrasolar gas giants using Herschel/PACS. Virtual Annual Meeting of the German Astronomical Society, Online (2021)
Gapp, C.; Rengel, M.; Hartogh, P.; Sagawa, H.; Feuchtgruber, H.; Lellouch, E.; Villanueva, G.: Characterization of Jupiter’s Atmosphere Using Far Infrared Spectra Measured with PACS Onboard the Herschel Space Observatory. Asia Oceania Geosciences Society 18th Annual Meeting (AOGS2021), Online (2021)
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)
Rengel, M.: Tracing the gas composition of Titan´s stratosphere from space, ground and airborne-based observatories. Workshop: "The Future of Airborne Infrared/Submm Astronomy: Prospects and Opportunities", online (2021)
Gapp, C.; Rengel, M.; Hartogh, P.; Sagawa, H.; Feuchtgruber, H.; Lellouch, E.; Villanueva, G.: Characterisation of Jupiter´s atmosphere with Herschel/PACS. 2nd Teleconference for the Ariel Working Group “Synergies with Solar System Planets, Online (2021)
Rengel, M.: Atmospheric characterisation of exoplanets through interpretation of their spectra. Online Seminar at Thüringer Landessternwarte , Tautenburg, Germany (2020)
Gapp, C.; Rengel, M.; Hartogh, P.; Sagawa, H.; Feuchtgruber, H.; Lellouch, E.: Retrieval of Jupiter’s atmospheric parameters using far infrared spectra measured with PACS onboard the Herschel Space Observatory. Europlanet Science Congress 2020, online (2020)
Rengel, M.: Key physico-chemical mechanisms in (exo)planetary atmospheres and their impacts on the observables. "Exploring the diversity of extrasolar planets", Virtual Annual Meeting of the German Astronomical Society (2020)
Rengel, M.; Reiners, A.; Cont, D.; Gapp, C.; Khaimova, J.; Lara, L. M.; Shulyak, D.; Yan, F.: Investigating physical and chemical mechanisms in planetary atmospheres and their impacts on the observables. Europlanet Science Congress 2020, online (2020)
Rengel, M.; Shulyak, D.; Hartogh, P.; Sagawa, H.; Moreno, R.; Jarchow, C.: Observing atmospheric HCN on Titan from space and ground-based observatories: an inter-comparison study from Herschel, APEX and IRAM 30m telescopes. Europlanet Science Congress 2020, online (2020)
Shulyak, D.; Rengel, M.; Lara, L.; Nèmec, N.-E.: Studying physics and chemistry in atmospheres of hot Jupiters from future ground-based and space facilities. Europlanet Science Congress 2020, online (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.