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)
First Light! The spectro-polarimeter of the world's largest solar telescope in Hawaii looks at the Sun for the first time. The instrument was developed in Germany.
Dr. Theodosios Chatzistergos receives award by the European Space Weather and Space Climate Association for his research findings on the historical activity of the Sun.
The Zdenĕk Švetska Senior Prize of the Solar Physics Division of the European Physical Society (EPS) recognizes Solanki’s pioneering contributions to solar research.
The magnetic field in the solar atmosphere exceeds the geomagnetic field strength by four orders of magnitude. It greatly influences the processes of energy transport within the solar atmosphere, and dominates the morphology of the solar chromosphere and corona. Kinetic energy from convective motions in the Sun can be efficiently stored in magnetic fields and subsequently released - to heat the solar corona to several million degrees or to blast off coronal mass ejections.
Application deadline 1 October 2024. PhD projects in planetary science, solar and stellar physics, solar magnetism, heliophysics, helioseismology, asteroseismology, ...