Vocks, C.: A kinetic model for ions in the solar corona including wave-particle interactions and Coulomb collisions. Astrophysical Journal 568, pp. 1017 - 1029 (2002)
Vocks, C.; Marsch, E.: Kinetic results for ions in the solar corona with wave-particle interactions and Coulomb collisions. Astrophysical Journal 568, pp. 1030 - 1042 (2002)
Vocks, C.: Ein kinetisches Modell der Ionen in koronalen Löchern mit Welle-Teilchen-Wechselwirkung und Coulomb-Stößen. Göttinger Beiträge zur Physik, Duehrkohp & Radicke, Göttingen (2001)
Marsch, E.; Tu, C.-Y.; Vocks, C.: On cyclotron-wave resonance and ion velocity distributions in coronal holes and the fast solar wind. In: Proceedings of SOHO 11 Symposium ``From Solar Min to Max: Half a Solar Cycle with SOHO'',, pp. 395 - 398 (Ed. Wilson, A.). ESA Publ. Div., Noordwijk (2002)
Vocks, C.: Ein kinetisches Modell der Ionen in koronalen Löchern mit Welle-Teilchen-Wechselwirkung und Coulumb-Stößen. Dissertation, Technische Universität Braunschweig (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
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.