Jurčák, J.; Collados, M.; Leenaarts, J.; van Noort, M.; Schlichenmaier, R.: Recent advancements in the EST project. Advances in Space Research 63 (4), pp. 1389 - 1395 (2019)
Siu-Tapia, A. L.; Lagg, A.; van Noort, M.; Rempel, M.; Solanki, S. K.: Superstrong photospheric magnetic fields in sunspot penumbrae. Astron. Astrophys.; EDP Sciences, Les Ulis Cedex A France 631, A99 (2019)
Löptien, B.; Lagg, A.; van Noort, M.; Solanki, S. K.: Measuring the Wilson depression of sunspots using the divergence-free condition of the magnetic field vector. Astronomy and Astrophysics 619, A42 (2018)
Centeno, R.; Blanco Rodriguez, J.; Del Toro Iniesta, J. C.; Solanki, S. K.; Barthol, P.; Gandorfer, A.; Gizon, L.; Hirzberger, J.; Riethmüller, T. L.; van Noort, M.et al.; Orozco Suarez, D.; Berkefeld, T.; Schmidt, W.; Pillet, V. M.; Knoelker, M.: A Tale of Two Emergences: SUNRISE II Observations of Emergence Sites in a Solar Active Region. Astrophysical Journal, Suppl. Ser. 229 (1), 3 (2017)
Gorobets, A. Y.; Berdyugina, S. V.; Riethmüller, T.; Rodríguez, J. B.; Solanki, S. K.; Barthol, P.; Gandorfer, A. M.; Gizon, L.; Hirzberger, J.; van Noort, M.et al.; Del Toro Iniesta, J. C.; Orozco Suárez, D.; Schmidt, W.; Martínez Pillet, V.; Knölker, M.: The Maximum Entropy Limit of Small-scale Magnetic Field Fluctuations in the Quiet Sun. The Astrophysical Journal Supplement Series 233, 5 (2017)
Analyzing the high spatial resolution solar Ca II H and K emission data obtained by the SUNRISE mission and building a model of other stars more active than the Sun
For PhD students whose project is already funded and who are applying for admission to the IMPRS, or for applicants who want to bring their own funding and their own project idea to the IMPRS.
The magnetic field in the solar atmosphere exceeds the geomagnetic field strength by four orders of magnitude. It greatly influences the processes of energy transport within the solar atmosphere, and dominates the morphology of the solar chromosphere and corona. Kinetic energy from convective motions in the Sun can be efficiently stored in magnetic fields and subsequently released - to heat the solar corona to several million degrees or to blast off coronal mass ejections.
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.