Kimura, H.; Mann, I.; Mukai, T.: Influence of dust shape and material composition on the solar F-corona. Planetary and Space Science 46, pp. 911 - 919 (1998)
Grün, E.; Krüger, H.; Dermott, S.; Fechtig, H.; Graps, A. L.; Zook, H. A.; Gustafson, B. A.; Hamilton, D. P.; Hanner, M. S.; Heck, A.et al.; Horányi, M.; Kissel, J.; Lindblad, B. A.; Linkert, D.; Linkert, G.; Mann, I.; McDonnell, J. A. M.; Morfill, G. E.; Polanskey, C.; Schwehm, G.; Srama, R.: Dust measurements in the Jovian magnetosphere. Geophysical Research Letters 24, pp. 2171 - 2174 (1997)
Grün, E.; Staubach, P.; Baguhl, M.; Hamilton, D. P.; Zook, H. A.; Dermott, S.; Fechtig, H.; Gustafson, B. A.; Hanner, M. S.; Horanyi, M.et al.; Kissel, J.; Lindblad, B. A.; Linkert, D.; Linkert, G.; Mann, I.; McDonnell, J. A. M.; Morfill, G. E.; Polanskey, C.; Schwehm, G.; Srama, R.: South-north and radial traverses through the interplanetary dust cloud. Icarus 129, pp. 270 - 288 (1997)
Mann, I.; Kuhn, J.: Near infrared solar coronal observations: A perspective for future investigations? Physics and Chemistry of the Earth 22, pp. 493 - 494 (1997)
Grün, E.; Baguhl, M.; Hamilton, D. P.; Riemann, R.; Zook, H. A.; Dermott, S.; Fechtig, H.; Gustafson, B. A.; Hanner, M. S.; Horanyi, M.et al.; Khurana, K. K.; Kissel, J.; Kivelson, M.; Lindblad, B.-A.; Linkert, D.; Linkert, G.; Mann, I.; McDonnell, J. A. M.; Morfill, G. E.; Polanskey, C.; Schwehm, G.; Srama, R.: Constraints from Galileo observations on the origin of Jovian dust streams. Nature 381, pp. L395 - L398 (1996)
Grün, E.; Hamilton, D. P.; Riemann, R.; Dermott, S.; Fechtig, H.; Gustafson, B. A.; Hanner, M. S.; Heck, A.; Horanyi, M.; Kissel, J.et al.; Krüger, H.; Lindblad, B. A.; Linkert, D.; Linkert, G.; Mann, I.; McDonnell, J. A. M.; Morfill, G. E.; Polanskey, C.; Schwehm, G.; Srama, R.; Zook, H. A.: Dust measurements during Galileo's approach to Jupiter and Io encounter. Science 274, pp. 399 - 401 (1996)
Leese, M. R.; McDonnell, J. A. M.; Green, S. F.; Busoletti, E.; Clark, B. C.; Colangeli, L.; Crifo, J. F.; Eberhardt, P.; Giovane, F.; Grün, E.et al.; Gustafson, B.; Hughes, D. W.; Jackson, D.; Lamy, P.; Langevin, Y.; Mann, I.; McKenna-Lawlor, S.; Tanner, W. G.; Weissman, P. R.; Zarnecki, J. C.: Dust flux analyser experiment for the Rosetta mission. Advances in Space Research 17, pp. (12)137 - (12)140 (1996)
Mann, I.; Grün, E.; Wilck, M.: The contribution of asteroid dust to the interplanetary dust cloud: The impact of Ulysses results on the understanding of dust production in the Asteroid Belt and of the formation of the IRAS dust bands. Icarus 120, pp. 399 - 407 (1996)
Davidson, W. C.; MacQueen, R. M.; Mann, I.: Scattering models for the solar infrared F-corona brightness. Planetary and Space Science 43, pp. 1395 - 1400 (1995)
Grün, E.; Baguhl, M.; Divine, N.; Fechtig, H.; Hanner, M. S.; Kissel, J.; Lindblad, B.-A.; Linkert, D.; Linkert, G.; Mann, I.et al.; McDonnell, J. A. M.; Morfill, G. E.; Polanskey, C.; Riemann, R.; Schwehm, G.; Siddique, N.; Staubach, P.; Zook, H. A.: Two years of ULYSSES data. Planetary and Space Science 43, pp. 971 - 999 (1995)
Grün, E.; Baguhl, M.; Divine, N.; Fechtig, H.; Hanner, M. S.; Kissel, J.; Lindblad, B.-A.; Linkert, D.; Linkert, G.; Mann, I.et al.; McDonnell, J. A. M.; Morfill, G. E.; Polanskey, C.; Riemann, R.; Schwehm, G.; Siddique, N.; Staubach, P.; Zook, H. A.: Three years of Galileo dust data. Planetary and Space Science 43, pp. 953 - 969 (1995)
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.
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.