Combi, M.; Shou, Y.; Fougere, N.; Tenishev, V.; Altwegg, K.; Rubin, M.; Bockelée-Morvan, D.; Capaccioni, F.; Cheng, Y.-C.; Fink, U.et al.; Gombosi, T.; C.Hansen, K.; Huang, Z.; Marshall, D. W.; Totha, G.: The surface distributions of the production of the major volatile species, H2O, CO2, CO and O2, from the nucleus of comet 67P/Churyumov-Gerasimenko throughout the Rosetta Mission as measured by the ROSINA double focusing mass spectrometer. Icarus 335, 113421 (2020)
Marshall, D. W.; Rezac, L.; Hartogh, P.; Zhao, Y.; Attree, N.: Interpretation of heliocentric water production rates of comets. Astronomy and Astrophysics 623, A120 (2019)
Rezac, L.; Zhao, Y.; Hartogh, P.; Ji, J.; Marshall, D. W.; Shi, X.: Three-dimensional analysis of spatial resolution of MIRO/Rosetta measurements at 67P/Churyumov-Gersimenko. Astronomy and Astrophysics 630, A34 (2019)
Marshall, D. W.; Hartogh, P.; Rezac, L.; von Allmen, P.; Biver, N.; Bockelée-Morvan, D.; Crovisier, J.; Encrenaz, P.; Gulkis, S.; Hofstadter, M.et al.; Ip, W.-H.; Jarchow, C.; Lee, S.; Lellouch, E.: Spatially resolved evolution of the local H2O production rates of comet 67P/Churyumov-Gerasimenko from the MIRO instrument on Rosetta. Astronomy and Astrophysics 603, A87 (2017)
Marshall, D. W.; Sadeghpour, H. R.: Simulating the formation of carbon-rich molecules on an idealized graphitic surface. Mon. Not. Roy. Astron. Soc. 455 (3), pp. 2889 - 2900 (2016)
Marshall, D. W.; Rezac, L.; Hartogh, P.: The inner coma of 67P/Churyumov-Gerasimenko as seen by MIRO. Asia Oceania Geosciences Society (AOGS) 15th Annual Meeting, Honolulu, Hawaii (2018)
Christou, C.; Dadzie, S. K.; Marschall, R.; Marshall, D. W.; Thomas, N.; Hartogh, P.; Jorda, L.; Kührt, E.; Wright, I.; Zarnecki, J.: Gas flow in near surface comet like porous structures: application to 67P/Churyumov-Gerasimenko. European Geosciences Union General Assembly, Vienna, Austria (2017)
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.