Guglielmino, S. L.; Martinez Pillet, V.; Bonet, J. A.; del Toro Iniesta, J. C.; Bellot Rubio, L. R.; Solanki, S. K.; Schmidt, W.; Gandorfer, A.; Barthol, P.; Knoelker, M.: The Frontier Between Small-Scale Bipoles and Ephemeral Regions in the Solar Photosphere: Emergence and Decay of an Intermediate-Scale Bipole Observed with SUNRISE/IMaX. Astrophysical Journal 745 (2), 160 (2012)
Martinez Gonzalez, M. J.; Bellot Rubio, L. R.; Solanki, S. K.; Martinez Pillet, V.; Del Toro Iniesta, J. C.; Barthol, P.; Schmidt, W.: Resolving the Internal Magnetic Structure of the Solar Network. Astrophysical Journal 758 (2), L40 (2012)
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.
Karen Harvey solar physics prize 2020 for Prof. Dr. Tian who studies dynamic phenomena in the Sun’s atmosphere; his research group is a partner group of the Max Planck Institute for Solar System Research.
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.
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.