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)
The Planetary Plasma Environments group (PPE) has a strong heritage in the exploration of planetary magnetospheres and space plasma interactions throughout the solar system. It has contributed instruments to several past missions that flew-by or orbited Jupiter (Galileo, Cassini, Ulysses). The PPE participates in the JUICE mission by contributing hardware and scientific expertise to the Particle Environment Package (PEP).
Application deadline 1 October 2024. PhD projects in planetary science, solar and stellar physics, solar magnetism, heliophysics, helioseismology, asteroseismology, ...
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.
In analyzing solar observations from the 19th century, scientists are turning to amateur researchers for help. The project will allow to better understand the history of our star.
Astronomical teamwork: By combining data from Solar Orbiter and SDO, a group of researchers has unambiguously determined the magnetic field at the solar surface.