Mann, I.; Kuhn, J. R.; Penn, M.: Infrared spectroscopic observations of neutral helium during the 1994 eclipse. In: Physics, Chemistry and Dynamics of Interplanetary Dust, pp. 345 - 348 (Eds. Gustafson, B. A. S.; Hanner, M. S.). Astron. Soc. Pacific, San Francisco (1996)
Mann, I.; MacQueen, R. M.: Ground-based observations of dust in the solar environment. In: Proc. First US-Russian Workshop on the FIRE Environment, pp. 161 - 163 (Eds. Vaisberg, O.; Tsurutani, B. T.). Space Research Institute, Moscow (1996)
Mann, I.; Skalsky, A. A.; Andreev, V. E.; Efimov, A. I.; Bogomolov, V. B.; Kuzienova, O. M.: Working group summary on circumsolar dust. In: Proc. First US-Russian Workshop on the FIRE Environment, pp. 259 - 261 (Eds. Vaisberg, O.; Tsurutani, B. T.). Space Research Institute, Moscow (1996)
Mann, I.; Wilck, M.; Grün, E.: Analysis of the Ulysses dust measurements in the Asteroid Belt. In: Physics, Chemistry and Dynamics of Interplanetary Dust, pp. 19 - 22 (Eds. Gustafson, B. A. S.; Hanner, M. S.). Astron. Soc. Pacific, San Francisco (1996)
Scherer, K.; Mann, I.; Reaves, G.: On the dnyamics of the zodiacal dust cloud close to the Sun. In: From Stardust to Planetesimals, pp. 209 - 212 (Eds. Kress, M. E.; Tielens, A. G. G. M.; Pendleton, Y. J.). Ames Research Center, Moffett Field (1996)
Mann, I.: Spatial distribution and orbital properties of interplanetary dust at high latitudes. In: Proc. 28th ESLAB Symp. on The High Latitude Heliosphere, pp. 477 - 482 (Ed. Marsden, R.). ESTEC, Noordwijk (1995)
Hartwig, H.; Mann, I.: The F-Korona Instrument-Design of a rocket-borne twin coronagraph. In: Proc. 11. ESA Symp. on European Rockets and Balloon Programmes and Related Research, Montreux 1993, pp. 283 - 286. ESA Publ. Div., Noordwijk (1994)
Mann, I.: F-corona experiment: Study of dust in circum-solar space. In: Proc. 11. ESA Symp. on European Rocket and Balloon Programmes and Related Research, Montreux 1993, pp. 259 - 261. ESA Publ. Div., Noordwijk (1994)
Mann, I.: Eigenschaften und Verteilung kosmischer Staubteilchen als Komponente der kleinen Körper im Sonnensystem. Habilitation, Technische Universität Braunschweig (1998)
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.
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".