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)
Images from ESA’s Solar Orbiter offer the best look yet at a source region of the solar wind - and challenge our view of the continuous particle stream from the Sun.
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