Stenborg, G.; Marsch, E.; Vourlidas, A.; Howard, R.; Baldwin, K.: A novel technique to measure intensity fluctuations in EUV images and to detect coronal sound waves nearby active regions. Astronomy and Astrophysics 526, A58 (2011)
Yao, S.; He, J.-S.; Marsch, E.; Tu, C.-Y.; Pedersen, A.; Rème, H.; Trotignon, J. G.: Multi-scale anti-correlation between electron density and magnetic field strength in the solar wind. Astrophysical Journal 728, 146 (2011)
Bourouaine, S.; Marsch, E.; Neubauer, F. M.: Correlations between the proton temperature anisotropy and transverse high-frequency waves in the solar wind. Geophysical Research Letters 37, L14104, pp. 1 - 4 (2010)
Guo, J. N.; Büchner, J.; Otto, A.; Santos, J.; Marsch, E.; Gan, W. Q.: Is the 3-D magnetic null point with a convective electric field an efficient particle accelerator? Astronomy and Astrophysics 513, A73 (2010)
He, J.-S.; Marsch, E.; Tu, C.-Y.; Tian, H.; Guo, L.-J.: Reconfiguration of the coronal magnetic field by means of reconnection driven by photospheric magnetic flux convergence. Astronomy and Astrophysics 510, A40 (2010)
Petrosyan, A.; Balogh, A.; Goldstein, M. L.; Léorat, J.; Marsch, E.; Petrovay, K.; Roberts, B.; von Steiger, R.; Vial, J. C.: Turbulence in the Solar Atmosphere and Solar Wind. Space Science Reviews 156, pp. 135 - 238 (2010)
Yao, S.; Marsch, E.; Tu, C.; Schwenn, R.: Identification of prominence ejecta by the proton distribution function and magnetic fine structure in interplanetary coronal mass ejections in the inner heliosphere. Journal Geophysical Research 115, A05103 (2010)
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.