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Cameron, R. H.; Schüssler, M.: Changes of the solar meridional velocity profile during cycle 23 explained by flows towards the activity belts. Astrophysical Journal 720, pp. 1030 - 1032 (2010)
Cheung, M. C. M.; Rempel, M.; Title, A. M.; Schüssler, M.: Simulation of the formation of a solar active region. Astrophysical Journal 720, pp. 233 - 244, (2010)
Danilovic, S.; Beeck, B.; Pietarila, A.; Schüssler, M.; Solanki, S. K.; Martinez Pillet, V.; Bonet, J. A.; del Toro Iniesta, J. C.; Domingo, V.; Barthol, P.et al.; Berkefeld, T.; Gandorfer, A.; Knölker, M.; Schmidt, W.; Title, A. M.: Transverse Component of the Magnetic Field in the Solar Photosphere Observed by SUNRISE. Astrophysical Journal 723 (2), pp. L149 - L153 (2010)
Danilovic, S.; Schüssler, M.; Solanki, S. K.: Magnetic field intensification: comparison of 3D MHD simulations with Hinode/SP results. Astronomy and Astrophysics 509, A76 (2010)
Danilovic, S.; Schüssler, M.; Solanki, S. K.: Probing quiet Sun magnetism using MURaM simulations and Hinode/SP results: support for a local dynamo. Astronomy and Astrophysics 513, A1 (2010)
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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.