Beeck, B.; Cameron, R. H.; Reiners, A.; Schüssler, M.: Three-dimensional simulations of near-surface convection in main-sequence stars II. Properties of granulation and spectral lines. Astronomy and Astrophysics 558, A49 (2013)
Beeck, B.; Collet, R.; Steffen, M.; Asplund, M.; Cameron, R. H.; Freytag, B.; Hayek, W.; Ludwig, H.-G.; Schüssler, M.: Simulations of the solar near-surface layers with the CO5BOLD, MURaM, and Stagger codes. Astronomy and Astrophysics 539, A121 (2012)
Cameron, R. H.; Schüssler, M.: Are the strengths of solar cycles determined by converging flows towards the activity belts? Astronomy and Astrophysics 548, A57 (2012)
Moll, R.; Cameron, R. H.; Schüssler, M.: Vortices, shocks, and heating in the solar photosphere: effect of a magnetic field. Astronomy and Astrophysics 541, A68 (2012)
Afram, N.; Unruh, Y. C.; Solanki, S. K.; Schüssler, M.; Lagg, A.; Vögler, A.: Intensity contrast from MHD simulations and HINODE observations. Astronomy and Astrophysics 526, A120 (2011)
Cameron, R. H.; Vögler, A...; Schüssler, M.: Decay of a simulated mixed-polarity magnetic field in the solar surface layers. Astronomy and Astrophysics 533, A86 (2011)
Jiang, J.; Cameron, R. H.; Schmitt, D.; Schüssler, M.: The solar magnetic field since 1700 I. Characteristics of sunspot group emergence and reconstruction of the butterfly diagram. Astronomy and Astrophysics 528, A82 (2011)
Jiang, J.; Cameron, R. H.; Schmitt, D.; Schüssler, M.: The solar magnetic field since 1700 II. Physical reconstruction of total, polar and open flux. Astronomy and Astrophysics 528, A83 (2011)
Röhrbein, D.; Cameron, R.; Schüssler, M.: Is there a non-monotonic relation between photospheric brightness and magnetic field strength? Astronomy and Astrophysics 532, A140 (2011)
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.