Chen, Y.; Peter, H.; Przybylski, D.; Tian, H.; Zhang, J.: Doppler shifts of spectral lines formed in the solar transition region and corona. Astronomy and Astrophysics 661, p. A94 (2022)
Chen, Y.; Przybylski, D.; Peter, H.; Tian, H.; Auchère, F.; Berghmans, D.: Transient small-scale brightenings in the quiet solar corona: A model for campfires observed with Solar Orbiter. Astronomy and Astrophysics 656, L7 (2021)
Rempel, M.; Przybylski, D.: Efficient Numerical Treatment of Ambipolar and Hall Drift as Hyperbolic System. The Astrophysical Journal 923, p. 79 (2021)
Felipe, T.; Socas-Navarro, H.; Przybylski, D.: Inversions of synthetic umbral flashes: Effects of scanning time on the inferred atmospheres. Astronomy and Astrophysics 614, p. A73 (2018)
Application deadline 1 October 2024. PhD projects in planetary science, solar and stellar physics, solar magnetism, heliophysics, helioseismology, asteroseismology, ...
In analyzing solar observations from the 19th century, scientists are turning to amateur researchers for help. The project will allow to better understand the history of our star.
Astronomical teamwork: By combining data from Solar Orbiter and SDO, a group of researchers has unambiguously determined the magnetic field at the solar surface.
Application deadline 1 October 2023. PhD projects in planetary science, solar and stellar physics, solar magnetism, heliophysics, helioseismology, asteroseismology, ...
Philipp Löschl has co-authored an excellent publication on Solar Orbiter data which has been awarded best Solar Physics paper of 2022 (Gherardo Valori et al. 2022)
IMPRS alumn Yuto Bekki is given a honourable mention by the IAU Division E Sun and Heliosphere for his PhD thesis “Theory of solar oscillations in the inertial frequency range”
IMPRS alumn Yuto Bekki is awarded the European Physical Society’s (EPS) European Solar Physics Division (ESPD) Patricia Edwin PhD Thesis Prize 2023 for the outstanding collection of original results about modes of solar oscillation in the inertial frequency range and for the development of numerical models to classify and study the various families of inertial modes that permeate the solar convection zone