Wicht, J.; Gastine, T.; Duarte, L. D. V.: Dynamo Action in the Steeply Decaying Conductivity Region of Jupiter‐Like Dynamo Models. Journal of Geophysical Research: Planets 124 (3), pp. 837 - 863 (2019)
Bärenzung, J.; Holschneider, M.; Wicht, J.; Sanchez, S.; Lesur, V.: Modeling and Predicting the Short‐Term Evolution of the Geomagnetic Field. Journal of Geophysical Research: Solid Earth 123 (6), pp. 4539 - 4560 (2018)
Barik, A.; Triana, S. A.; Hoff, M.; Wicht, J.: Triadic resonances in the wide-gap spherical Couette system. The Journal of Fluid Mechanics 843, pp. 211 - 243 (2018)
Becker, A.; Bethkenhagen, M.; Kellermann, C.; Wicht, J.; Redmer, R.: Material Properties for the Interiors of Massive Giant Planets and Brown Dwarfs. The Astronomical Journal 156 (4), 149 (2018)
Dietrich, W.; Hori, K.; Wicht, J.: Core flows and heat transfer induced by inhomogeneous cooling with sub- and supercritical convection. Phys. Earth Planet. Inter. 251, pp. 36 - 51 (2016)
Duarte, L. D. V.; Wicht, J.; Browning, M. K.; Gastine, T.: Helicity inversion in spherical convection as a means for equatorward dynamo wave propagation. Mon. Not. Roy. Astron. Soc. 456, pp. 1708 - 1722 (2016)
Heimpel, M.; Gastine, T.; Wicht, J.: Simulation of deep-seated zonal jets and shallow vortices in gas giant atmospheres. Nature Geoscience 9, pp. 19 - 23 (2016)
Wicht, J.; Meduri, D. G.: A gaussian model for simulated geomagnetic field reversals. Physics of the Earth and Planetary Interiors 259, pp. 45 - 60 (2016)
Dietrich, W.; Wicht, J.; Hori, K.: Effect of width, amplitude, and position of a core mantle boundary hot spot on core convection and dynamo action. Progress in Earth and Planetary Science 2, 35 (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.
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).