Wilken, B.; Zong, Q.-G.; Reeves, G. D.; Doke, T.; Yamamoto, T.: Geoactivity in response to CIR/CME events-a synoptic view. Physics and Chemistry of the Earth 24, pp. 113 - 117 (1999)
Zong, Q.-G.; Wilken, B.; Woch, J.; Büchner, J.; Reeves, G. D.; Doke, T.; Yamamoto, T.: Energetic particles bursts in the near-earth magnetosheath during a storm recovery phase. Physics and Chemistry of the Earth 24, pp. 293 - 298 (1999)
Aellig, M. R.; Grünwaldt, H.; Bochsler, P.; Wurz, P.; Hefti, S.; Kallenbach, R.; Ipavich, F. M.; Axford, W. I.; Balsiger, H.; Bürgi, A.et al.; Coplan, M. A.; Galvin, A. B.; Geiss, J.; Gliem, F.; Gloeckler, G.; Hilchenbach, M.; Hovestadt, D.; Hsieh, K. C.; Klecker, B.; Lee, M. A.; Livi, S.; Managadze, G. G.; Marsch, E.; Möbius, E.; Neugebauer, M.; Reiche, K.-U.; Scholer, M.; Verigin, M. I.; Wilken, B.: Iron freeze-in temperatures measured by SOHO/CELIAS/CTOF. Journal Geophysical Research 103, pp. 17215 - 17222 (1998)
Henke, T.; Woch, J.; Mall, U.; Livi, S.; Wilken, B.; Schwenn, R.; Gloeckler, G.; von Steiger, R.; Forsyth, R. J.; Balogh, A.: Differences in the O7+ /O6+ ratio of magnetic cloud and non-cloud coronal mass ejections. Geophysical Research Letters 25, pp. 3465 - 3468 (1998)
Ipavich, F. M.; Galvin, A. B.; Lasley, S. E.; Paquette, J. A.; Hefti, S.; Reiche, K.-U.; Coplan, M. A.; Gloeckler, G.; Bochsler, P.; Hovestadt, D.et al.; Grünwaldt, H.; Hilchenbach, M.; Gliem, F.; Axford, W. I.; Balsiger, H.; Bürgi, A.; Geiss, J.; Hsieh, K. C.; Kallenbach, R.; Klecker, B.; Lee, M. A.; Managadze, G. G.; Marsch, E.; Möbius, E.; Neugebauer, M.; Scholer, M.; Verigin, M. I.; Wilken, B.; Wurz, P.: Solar wind measurements with SOHO: The CELIAS/MTOF proton monitor. Journal Geophysical Research 103, pp. 17205 - 17213 (1998)
Jin, S. P.; Ma, N.; Zong, Q.-G.; Wilken, B.: A simulation study of multiple plasmoids in the magnetotail during substorm event (II). ACTA Geophysica Sinica 16, pp. 283 - 291 (1998)
Kucharek, H.; Ipavich, F. M.; Kallenbach, R.; Bochsler, P.; Hovestadt, D.; Grünwaldt, H.; Hilchenbach, M.; Axford, W. I.; Balsiger, H.; Bürgi, A.et al.; Coplan, M. A.; Galvin, A. B.; Geiss, J.; Gliem, F.; Gloeckler, G.; Hsieh, K. C.; Judge, D. L.; Klecker, B.; Lee, M. A.; Livi, S.; Managadze, G. G.; Marsch, E.; Möbius, E.; Neugebauer, M.; Ogawa, H. S.; Reiche, K.-U.; Scholer, M.; Verigin, M. I.; Wilken, B.; Wurz, P.: Magnesium isotopic composition as observed with the CELIAS/MTOF experiment on the SOHO spacecraft. Journal Geophysical Research 103, pp. 26805 - 26812 (1998)
Lagg, A.; Krupp, N.; Woch, J.; Livi, S.; Wilken, B.; Williams, D. J.: Determination of the neutral number density in the Io-torus from Galileo-EPD measurements. Geophysical Research Letters 25 (21), pp. 4039 - 4042 (1998)
Mauk, B. H.; McEntire, R. W.; Williams, D. J.; Lagg, A.; Roelof, E. C.; Krimigis, S. M.; Armstrong, T. P.; Fritz, T. A.; Lanzerotti, L. J.; Roederer, J. G.et al.; Wilken, B.: Galileo-measured depletion of near-Io hot ring current plasmas since the voyager epoch. Journal Geophysical Research 103, pp. 4715 - 4722 (1998)
Wilken, B.; Zong, Q.-G.; Doke, T.; Mukai, M.; Yamamoto, T.; Reeves, G. D.; Maezawa, K.; Kokubun, S.; Ullaland, S.: Substorm activity on January 11, 1994: Geotail observations in the distant tail during the leading phase of a corotating interaction region. Journal Geophysical Research 103, pp. 17671 - 17689 (1998)
Zong, Q.-G.; Wilken, B.: Energetic oxygen bursts in the distant tail as a result of substorms. Journal Geophysical Research 103, pp. 20339 - 20363 (1998)
Zong, Q.-G.; Wilken, B.: Layered structure of energetic oxygen ions in the dayside magnetosheath. Geophysical Research Letters 25, pp. 4121 - 4124 (1998)
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, ...