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Sremcevic, M.; Krivov, A. V.; Krüger, H.; Spahn, F.: Impact-generated dust clouds around planetary satellites: model versus Galileo data. Planetary and Space Science 53, pp. 625 - 641 (2005)
Willis, M.; Burchell, M. J.; Ahrens, T. J.; Krüger, H.; Grün, E.: Decreased values of cosmic dust number density estimates in the solar system. Icarus 176, pp. 440 - 452 (2005)
Altobelli, N.; Krüger, H.; Moissl, R.; Landgraf, M.; Grün, E.: Influence of wall impacts on the Ulysses dust detector in modelling the interstellar dust flux. Planetary and Space Science 52, pp. 1287 - 1295 (2004)
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First Light for Sunrise III: the first tests with real sunlight were successful. The balloon-borne solar observatory should be ready for launch at the end of May.
First icy cold, then midnight sun: at the Arctic Circle, the team will prepare the next flight of the balloon-borne solar observatory - and hopes for solar fireworks.
Astronomical teamwork: By combining data from Solar Orbiter and SDO, a group of researchers has unambiguously determined the magnetic field at the solar surface.
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.