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 dwarf planet is a bizarre, cryovolcanic world. However, the organic deposits discovered on its surface so far are unlikely to originate from its interior.
The Uranian magnetic field is more expansive than previously thought, according to newly analyzed data from Voyager 2, making it easier to search for moons with oceans.