Cameron, R.; Schüssler, M.: A robust correlation between growth rate and amplitude of solar cycles: consequences for prediction methods. Astrophysical Journal 685, pp. 1291 - 1296 (2008)
Cheung, M. C. M.; Schüssler, M.; Tarbell, T. D.; Title, A. M.: Solar Surface Emerging Flux Regions: A Comparative Study of Radiative MHD Modeling and Hinode SOT Observations. Astrophysical Journal 687, pp. 1373 - 1387 (2008)
Danilovic, S.; Gandorfer, A.; Lagg, A.; Schüssler, M.; Solanki, S. K.; Vögler, A.; Katsukawa, Y.; Tsuneta, S.: The intensity contrast of solar granulation: comparing Hinode SP results with MHD simulations. Astronomy and Astrophysics 484, p. L17 (2008)
Schüssler, M.; Vögler, A.: Strong horizontal photospheric magnetic field in a surface dynamo simulation. Astronomy and Astrophysics 481, pp. L5 - L8 (2008)
Cheung, M.; Schüssler, M.; Moreno-Insertis, F.: The origin of the reversed granulation in the solar photosphere. Astronomy and Astrophysics 461, pp. 1163 - 1171 (2007)
Cheung, M. C. M.; Schüssler, M.; Moreno-Insertis, F.: Magnetic flux emergence in granular convection: radiative MHD simulations and observational signatures. Astronomy and Astrophysics 467, pp. 703 - 719 (2007)
Holzwarth, V.; Schüssler, M.; Schmitt, D.: Flow instabilities of magnetic flux tubes - II. Longitudinal flow. Astronomy and Astrophysics 469, pp. 11 - 17 (2007)
Işık, E.; Schüssler, M.; Solanki, S. K.: Magnetic flux transport on active cool stars and starspot lifetimes. Astronomy and Astrophysics 464, pp. 1049 - 1057 (2007)
Baumann, I.; Schmitt, D.; Schüssler, M.: A necessary extension of the surface flux transport model. Astronomy and Astrophysics 446, pp. 307 - 314 (2006)
Cheung, M. C. M.; Moreno-Insertis, F.; Schüssler, M.: Moving magnetic tubes: fragmentation, vortex streets and the limit of the approximation of thin flux tubes. Astronomy and Astrophysics 451, pp. 303 - 317 (2006)
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.