Baumann, I.; Schmitt, D.; Schüssler, M.: A necessary extension of the surface flux transport model. Astronomy and Astrophysics 446, pp. 307 - 314 (2006)
Baumann, I.; Solanki, S. K.: On the size distribution of sunspot groups in the Greenwich sunspot record 1874-1976. Astronomy and Astrophysics 443, pp. 1061 - 1066 (2005)
Baumann, I.; Schmitt, D.; Schüssler, M.; Solanki, S. K.: Evolution of the large-scale magnetic field on the solar surface: a parameter study. Astronomy and Astrophysics 426, pp. 1075 - 1091 (2004)
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.
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).