Chen, F.; Peter, H.: Using coronal seismology to estimate the magnetic field strength in a realistic coronal model. Hinode 9 Science Meeting, Belfast, Ireland (2015)
Peter, H.: Mehrflüssigkeitsmodelle der unteren Sonnenatmosphäre und Schlußfolgerungen für den Sonnenwind. Dissertation, Georg-August-Universität Göttingen (1997)
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.