Korth, A.; Friedel, R. H. W.; Frutos-Alfaro, F.; Mouikis, C. G.; Zong, Q.-G.: Ion composition of substorms during storm-time and non-storm-time periods. Journal of Atmospheric and Solar-Terrestrial Physics 64, pp. 561 - 566 (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)
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)
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)
Pu, Z. Y.; Kang, K. B.; Korth, A.; Fu, S. Y.; Zong, Q.-G.; Chen, Z. X.; Hong, M. H.; Liu, Z. X.; Mouikis, C. G.; Friedel, R. H. W.et al.; Pulkkinen, T.: Ballooning instability in the presence of a plasma flow: A synthesis of tail reconnection and current disruption models for the initiation of substorms. Journal Geophysical Research 104 (A5), pp. 10235 - 10248 (1999)
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)
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)
Pu, Z. Y.; Friedel, R. H. W.; Korth, A.; Zong, Q.-G.; Chen, Z. X.; Roux, A.; Perraut, S.: Evaluation of energetic particle parameters in the near-earth magnetotail derived from flux asymmetry observations. Annales Geophysicae 16 (3), pp. 283 - 291 (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)
Zong, Q.-G.; Wilken, B.; Woch, J.; Mukai, T.; Yamamoto, T.; Reeves, G. D.; Doke, T.; Maezawa, K.; Williams, D. J.; Kokubun, S.et al.; Ullaland, S.: Energetic oxygen ion bursts in the distant magnetotail as a product of intense substorms: Three case studies. Journal Geophysical Research 103, pp. 20339 - 20363 (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, ...