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)
The European Space Agency (ESA) has given the green light to build the flight models of the spacecraft and science payload for the PLATO mission to search for extrasolar planets.
In the "Solar and Stellar Interiors" department, Laurent Gizon, Jesper Schou, Aaron Birch, Robert Cameron and others offer PhD projects in solar physics and astrophysics. Helioseismology and asteroseismology are used as important tools to study the oscillating Sun and stars.
The longest-serving solar observatory in space has turned 25 and is still making significant contributions to solar research. Its old age has become an important merit.