Fu, S. Y.; Zong, Q.-G.; Fritz, T. A.; Pu, Z. Y.; Wilken, B.: Composition signatures in ion injections and its dependence on geomagnetic conditions. Journal Geophysical Research 107 (A10), 1299 (2002)
Krimigis, S. M.; Mitchell, D. G.; Hamilton, D. C.; Dandouras, J.; Armstrong, T. P.; Bolton, S. J.; Cheng, A. F.; Gloeckler, G.; Hsieh, K. C.; Keath, E. P.et al.; Krupp, N.; Lagg, A.; Lanzerotti, L. J.; Livi, S.; Mauk, B. H.; McEntire, R. W.; Roelof, E. C.; Wilken, B.; Williams, D. J.: A nebula of gases from Io surrounding Jupiter. Nature 415, pp. 994 - 996 (2002)
Oksavik, K.; Fritz, T. A.; Zong, Q.-G.; Søraas, F.; Wilken, B.: Three-dimensional energetic ion sounding of the magnetopause using Cluster/RAPID. Geophysical Research Letters 29 (9), 1347 (2002)
Fu, S. Y.; Wilken, B.; Zong, Q.-G.; Pu, Z. Y.: Ion composition variations in the inner magnetosphere: Individual and collective storm effects in 1991. Journal Geophysical Research 106, p. 29683 (2001)
Jin, S.-P.; Hu, X.-P.; Zong, Q.-G.; Fu, S.-Y.; Wilken, B.; Büchner, J.: 2.5 dimensional MHD simulation of multiple-plasmoids-like structures in the course of a substorm. Journal Geophysical Research 106 (A12), pp. 29807 - 29830 (2001)
Krupp, N.; Woch, J.; Lagg, A.; Roelof, E. C.; Williams, D. J.; Livi, S.; Wilken, B.: Local time asymmetry of energetic ion anisotropies in the Jovian magnetosphere. Planetary and Space Science 49 (3-4), pp. 283 - 289 (2001)
Zong, Q.-G.; Wilken, B.; Fu, S. Y.; Fritz, T. A.; Korth, A.; Hasebe, N.; Williams, D. J.; Pu, Z. Y.: Ring Current Oxygen Ions Excaping into the Magnetosheath. Journal Geophysical Research 106 (A11), pp. 25541 - 25556 (2001)
Kirsch, E.; Mall, U.; Cierpka, K.; Wilken, B.; Gloeckler, G.; Galvin, A. B.: Composition of low energy solar particles (0.5-225 keV/e) measured by the WIND-S/C during impulsive and gradual flares. Advances in Space Research 26, pp. 833 - 837 (2000)
Perry, C. H.; Grande, M.; Zurbuchen, T. H.; Hefti, S.; Gloeckler, G.; Fennell, J. F.; Wilken, B.; Fritz, T.: Use of Fe charge state changes as a tracer for solar wind entry to the Magnetosphere. Geophysical Research Letters 27, p. 2441 (2000)
von Steiger, R.; Schwadron, N. A.; Fisk, L. A.; Geiss, J.; Gloeckler, G.; Hefti, S.; Wilken, B.; Wimmer-Schweingruber, R. F.; Zurbuchen, T. H.: Composition of quasi-stationary solar wind flows from Ulysses/Solar Wind Ion Composition Spectrometer. Journal Geophysical Research 105, p. 27217 (2000)
Wilken, B.; Zong, Q.-G.; Doke, T.; Kokubun, S.; Mukai, T.; Reeves, G. D.: Distribution of Energetic Oxygen Events in the Tail Region - a view from HEP-LD/GEOTAIL. Advances in Space Research 25 (7/8), pp. 1603 - 1606 (2000)
Zong, Q.-G.; Wilken, B.; Fu, S. Y.; Doke, T.; Kokubun, S.: Energetic oxygen ions in the magnetosheath during the passage of a CME event. Advances in Space Research 25 (12), pp. 2421 - 2424 (2000)
Daglis, I. A.; Kasotakis, G.; Sarris, E. T.; Kamide, Y.; Dialetis, D.; Livi, S.; Wilken, B.: Variation of the ion composition during an intense magnetic storm and their consequences. Physics and Chemistry of the Earth 24, pp. 229 - 232 (1999)
Håland, S.; Østgaard, N.; Bjordal, J.; Stadsnes, J.; Ullaland, S.; Wilken, B.; Yamamoto, T.; Doke, T.; Chenette, D. L.; Parks, G. K.et al.; Brittnacher, M. J.; Reeves, G. D.: Magnetospheric and ionospheric response to a substorm: Geotail HEP-LD and Polar PIXIE observations. Journal Geophysical Research 104, p. 28459 (1999)
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, ...