Lee, Y. J.; Titov, D. V.; Tellmann, S.; Piccialli, A.; Ignatiev, N.; Pätzold, M.; Häusler, B.; Piccioni, G.; Drossart, P.: Vertical structure of the Venus cloud top from the VeRa and VIRTIS observations onboard Venus Express. Icarus 217 (2), pp. 599 - 609 (2012)
Piccialli, A.; Tellmann, S.; Titov, D. V.; Limaye, S. S.; Khatuntsev, I. V.; Paetzold, M.; Haeusler, B.: Dynamical properties of the Venus mesosphere from the radio-occultation experiment VeRa onboard Venus Express. Icarus 217 (2), pp. 669 - 681 (2012)
Various application review phases in 2025. PhD projects in cosmochemistry, planetary science, solar and stellar physics, helioseismology, asteroseismology, ...
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.