Nagy, A. F.; Winterhalter, D.; Sauer, K.; Cravens, T. E.; Brecht, S.; Mazelle, C.; Crider, D.; Kallio, E.; Zakharov, A.; Dubinin, E.et al.; Verigin, M.; Kotova, G.; Axford, W. I.; Bertucci, C.; Trotignon, J. G.: The plasma environment of Mars. Space Science Reviews 111 (1-2), pp. 33 - 114 (2004)
Florinski, V.; Zank, G. P.; Axford, W. I.: The solar system in a dense interstellar cloud: Implications for cosmic-ray fluxes at Earth and 10Be records. Geophysical Research Letters 30 (23), 2206 (2003)
Trotignon, J. G.; Parrot, M.; Cerisier, J. C.; Menvielle, M.; Axford, W. I.; Pätzold, M.; Warnant, R.; Wernik, A. W.: The plasma environment of Mars: from the shocked solar wind down to the ionosphere. Planetary and Space Science 48, pp. 1181 - 1191 (2000)
Lieu, R.; Ip, W.-H.; Axford, W. I.; Bonamente, M.: Nonthermal origin of the EUV and soft X-rays from the Coma Cluster: Cosmic rays in equipartition with the thermal medium. Astrophys. J. Let. 510, pp. L25 - L28 (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)
Axford, W. I.; Marsch, E.; Oraevsky, V. N.; Kuznetsov, V. D.; Breus, T. K.; Schwenn, R.; Ip, W.-H.; Ksanfomality, L. V.; Thomas, N.; Kogan, A.et al.; Utkin, V. F.; Uspensky, G. R.: Space mission for exploration of the Sun, Mercury and inner heliosphere (``InterHelios''). Advances in Space Research 21, pp. 275 - 289 (1998)
Breus, T. K.; Pimenov, K. Y.; Luhmann, J. G.; Krymskii, A. M.; Hagfors, T.; Axford, W. I.; Kliore, A. J.: Application of Viking radio occultation data to the future studies of the Martian ionosphere. Advances in Space Research 22, pp. 463 - 470 (1998)
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.