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)
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)
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)
Turbulence plays a very important role in many applications, ranging from geophysics and astrophysics to engineering. In our solar system, turbulence is often driving by thermal effect, rotation, and magnetic field. In this project you will use high-fidelity simulation tools, including direct numerical simulations, data assimilation, and machine learning, to study the physics of turbulence, focusing on convection and dynamos.
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).
In the "Solar and Stellar Interiors" department, Laurent Gizon, Jesper Schou, Aaron Birch, Robert Cameron and others offer PhD projects in solar physics and astrophysics. Helioseismology and asteroseismology are used as important tools to study the oscillating Sun and stars.
Inversion codes are used to aid the detailed interpretation of solar spectro-polarimetric data. This computer code attempts to find the atmospheric structure that produced an observed spectrum by minimizing the difference between the observed spectrum and a Stokes spectrum.
The MPS is one of the leading institutes worldwide in building instruments for solar research, both for ground based observatories as well as for balloon and space-borne missions. Scientists and engineers of MPS conceive new observing methods and develop novel instruments of highest technological complexity. These instruments are built in house, tested, calibrated, and used at the best solar observatories in the world, or delivered to NASA and ESA to be launched to space.
The Solar Lower Atmosphere and Magnetism (SLAM) group covers many exciting subjects in solar physics, focussing on the development and testing of highly novel solar instrumentation, reduction and analysis of highest quality solar observations, or improving and developing advanced techniques for the analysis of solar observations.