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)
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
First Light for Sunrise III: the first tests with real sunlight were successful. The balloon-borne solar observatory should be ready for launch at the end of May.
First icy cold, then midnight sun: at the Arctic Circle, the team will prepare the next flight of the balloon-borne solar observatory - and hopes for solar fireworks.
Astronomical teamwork: By combining data from Solar Orbiter and SDO, a group of researchers has unambiguously determined the magnetic field at the solar surface.