Amit, H.; Coutelier, M.; Christensen, U. R.: On equatorially symmetric and antisymmetric geomagnetic secular variation timescales. Physics of the Earth and Planetary Interiors 276, pp. 190 - 201 (2018)
Christensen, U. R.: Geodynamo models with a stable layer and heterogeneous heat flow at the top of the core. Geophysical journal international 215 (2), pp. 1338 - 1351 (2018)
Yadav, R. K.; Christensen, U. R.; Wolk, S. J.; Poppenhaeger, K.: Magnetic cycles in a dynamo simulation of fully convective M-star Proxima Centauri. Astrophysical Journal 833 (2), L28 (2016)
Yadav, R. K.; Gastine, T.; Christensen, U. R.; Duarte, L.; V., D.; Reiners, A.: Effect of shear and magnetic field on the heat transfer efficiency of convection in rotating spherical shells. Geophysical Journal International 204, pp. 1120 - 1133 (2016)
Yadav, R. K.; Gastine, T.; Christensen, U. R.; Wolk, S. J.; Poppenhaeger, K.: Approaching a realistic force balance in geodynamo simulations. Proc. Nat. Acad. Sci. 113 (43), pp. 12065 - 12070 (2016)
Nathues, A.; Hoffmann, M.; Schaefer, M.; Le Corre, L.; Reddy, V.; Platz, T.; Cloutis, E. A.; Christensen, U.; Kneissl, T.; Li, J.-Y.et al.; Mengel, K.; Schmedemann, N.; Schaefer, T.; Russell, C. T.; Applin, D. M.; Buczkowski, D. L.; Izawa, M. R. M.; Keller, H. U.; OBrien, D. P.; Pieters, C. M.; Raymond, C. A.; Ripken, J.; Schenk, P. M.; Schmidt, B. E.; Sierks, H.; Sykes, M. V.; Thangjam, G. S.; Vincent, J.-B.: Sublimation in bright spots on Ceres. Nature 528, pp. 237 - 240 (2015)
Saur, J.; Duling, S.; Roth, L.; Jia, X.; Strobel, D. F.; Feldman, P. D.; Christensen, U. R.; Retherford, K. D.; McGrath, M. A.; Musacchio, F.et al.; Wennmacher, A.; Neubauer, F. M.; Simon, S.; Hartkorn, O.: The search for a subsurface ocean in Ganymede with Hubble Space Telescope observations of its auroral ovals. Journal Geophysical Research 120, pp. 1715 - 1737 (2015)
Yadav, R. K.; Christensen, U. R.; Morin, J.; Gastine, T.; Reiners, A.; Poppenhaeger, K.; Wolk, S. J.: Explaining the coexistence of large-scale and small-scale magnetic fields in fully convective stars. Astrophysical Journal 813, L31 (2015)
Yadav, R.; Gastine, T.; Christensen, U.; Reiners, A.: Formation of starspots in self-consistent global dynamo models: Polar spots on cool stars. Astronomy and Astrophysics 573, A68 (2015)
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).
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).