Işık, E.; Schmitt, D.; Schüssler, M.: A coupled model of magnetic flux generation and transport in stars. Astron. Nachrichten 328, pp. 1111 - 1113 (2007)
Işık, E.; Schüssler, M.; Solanki, S. K.: Magnetic flux transport on active cool stars and starspot lifetimes. Astronomy and Astrophysics 464, pp. 1049 - 1057 (2007)
Işık, E.; Schüssler, M.; Solanki, S. K.: Magnetic flux transport and the lifetimes of spots on active cool stars. In: Modern Solar Facilities - Advanced Solar Science, pp. 367 - 369 (Eds. Kneer, F.; Puschmann, K. G.; Wittmann, A. D.). Universitätsverlag Göttingen (2007)
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
The Planetary Plasma Environments group (PPE) has a strong heritage in the exploration of planetary magnetospheres and space plasma interactions throughout the solar system. It has contributed instruments to several past missions that flew-by or orbited Jupiter (Galileo, Cassini, Ulysses). The PPE participates in the JUICE mission by contributing hardware and scientific expertise to the Particle Environment Package (PEP).
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.