Zhou, X.; Büchner, J.; Barta, M.; Gan, W.; Liu, S.: Particle acceleration by cascading reconnection in the solar corona. 40th COSPAR Scientific Assembly, Moscow, Russia (2014)
Büchner, J.; Nikutowski, B.; Bedrich, S.; Griethe, H.: SCHWARM - Small satellites for the investigation of collisionless plasma turbulence and magnetic reconnection. Max-Planck-Institut für Aeronomie, Katlenburg-Lindau, Germany (2001)
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.
Images from ESA’s Solar Orbiter offer the best look yet at a source region of the solar wind - and challenge our view of the continuous particle stream from the Sun.