Krivov, A. V.; Mann, I.; Krivova, N. A.: Size distribution of dust in circumstellar debris disks. Astronomy and Astrophysics 362, pp. 1127 - 1137 (2000)
Mann, I.; Kimura, H.: Interstellar dust properties derived from mass density, mass distribution, and flux rates in the heliosphere. Journal Geophysical Research 105, pp. 10317 - 10328 (2000)
Kimura, H.; Mann, I.: Filtering of the interstellar dust flow near the heliopause: the importance of secondary electron emission for the grain charging. Earth Planets Space 51, pp. 1223 - 1232 (1999)
Krüger, H.; Grün, E.; Hamilton, D. P.; Baguhl, M.; Dermott, S.; Fechtig, H.; Gustafson, B. A.; Hanner, M. S.; Horányi, M.; Kissel, J.et al.; Lindblad, B. A.; Linkert, D.; Linkert, G.; Mann, I.; McDonnell, J. A. M.; Morfill, G. E.; Polanskey, C.; Riemann, R.; Schwehm, G.; Srama, R.; Zook, H. A.: Three years of Galileo dust data: II. 1993-1995. Planetary and Space Science 47, pp. 85 - 106 (1999)
Krüger, H.; Grün, E.; Landgraf, M.; Baguhl, M.; Dermott, S.; Fechtig, H.; Gustafson, B. A.; Hamilton, D. P.; Hanner, M. S.; Horányi, 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.; Zook, H. A.: Three years of Ulysses dust data: 1993-1995. Planetary and Space Science 47, pp. 363 - 383 (1999)
Kuhn, J. R.; MacQueen, R. M.; Streete, J.; Tansey, G.; Mann, I.; Hillebrand, P.; Coulter, R.; Lin, H.: Probable detection of a bright infrared coronal emission line of SI IX near 3.93 microns. Astrophysical Journal 521, pp. 478 - 482 (1999)
Mann, I.; Kuhn, J. R.; MacQueen, R. M.; Streete, J.; Tansey, G.; Hillebrand, P.; Colter, R.; Lin, H.; Edmund, D.; Judge, P.: Probable detection of a bright infrared coronal emission line of Si IX near 3.93 microns. Astrophysical Journal 521, pp. 478 - 482 (1999)
Wehry, A.; Mann, I.: Identification of β-meteoroids from measurements of the dust detector onboard the Ulysses spacecraft. Astronomy and Astrophysics 341, pp. 296 - 303 (1999)
Grün, E.; Krüger, H.; Graps, A. L.; Hamilton, D. P.; Heck, A.; Linkert, G.; Zook, H. A.; Dermott, S.; Fechtig, H.; Gustafson, B. A.et al.; Hanner, M. S.; Horányi, M.; Kissel, J.; Lindblad, B. A.; Linkert, D.; Mann, I.; McDonnell, J. A. M.; Morfill, G. E.; Polanskey, C.; Schwehm, G.; Srama, R.: Galileo observes electromagnetically coupled dust in the Jovian magnetosphere. Journal Geophysical Research 103, p. 20011 (1998)
Kimura, H.; Mann, I.: The electric charging of interstellar dust in the solar system and consequences for its dynamics. Astrophysical Journal 499, pp. 454 - 462 (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".