Jafarzadeh, S.; Schiavo, L. A. C. A.; Fedun, V.; Solanki, S. K.; Stangalini, M.; Calchetti, D.; Verth, G.; Jess, D. B.; Grant, S. D. T.; Ballai, I.et al.; Gafeira, R.; Keys, P. H.; Fleck, B.; Morton, R. J.; Browning, P. K.; Silva, S. S. A.; Appourchaux, T.; Gandorfer, A.; Gizon, L.; Hirzberger, J.; Kahil, F.; Orozco Suárez, D.; Schou, J.; Strecker, H.; del Toro Iniesta, J. C.; Valori, G.; Volkmer, R.; Woch, J.: Sausage, kink, and fluting magnetohydrodynamic wave modes identified in solar magnetic pores by Solar Orbiter/PHI. Astronomy and Astrophysics 688, p. A2 (2024)
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.