Gastine, T.; Duarte, L.; Wicht, J.: Dipolar versus multipolar dynamos: the influence of the background density stratification. Astronomy and Astrophysics 546, A19 (2012)
Morgenthaler, A.; Petit, P.; Saar, S.; Solanki, S. K.; Morin, J.; Marsden, S. C.; Auriere, M.; Dintrans, B.; Fares, R.; Gastine, T.et al.; Lanoux, J.; Lignieres, F.; Paletou, F.; Ramirez Velez, J. C.; Theado, S.; Van Grootel, V.: Long-term magnetic field monitoring of the Sun-like star ξ Bootis A. Astronomy and Astrophysics 540, A138 (2012)
Jones, C. A.; Boronski, P.; Brun, A. S.; Glatzmaier, G. A.; Gastine, T.; Miesch, M. S.; Wicht, J.: Anelastic convection-driven dynamo benchmarks. Icarus 216, pp. 120 - 135 (2011)
Bossmann, A. B.; Wicht, J.; Gastine, T.; Christensen, U. R.: Magnetic field morphology of the ice giants linked to their internal structure. 5th Meeting of the DFG-SPP Planetary Magnetism, Nördlingen, Germany (2015)
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.
Next week, JUICE will pass closely by Moon and Earth. The daring maneuver offers the first opportunity to test the scientific instruments in a Jupiter-like setting.