Cameron, R. H.; Schüssler, M.: Solar activity: periodicities beyond 11 years are consistent with random forcing. Astronomy and Astrophysics 625, A28 (2019)
Borrero, J. M.; Jafarzadeh, S.; Schüssler, M.; Solanki, S. K.: Solar Magnetoconvection and Small-Scale Dynamo Recent Developments in Observation and Simulation. Space Science Reviews 210 (1-4), S. 275 - 316 (2017)
Cameron, R.; Schüssler, M.: The turbulent diffusion of toroidal magnetic flux as inferred from properties of the sunspot butterfly diagram. Astronomy and Astrophysics 591, A46 (2016)
Beeck, B.; Schüssler, M.; Cameron, R. H.; Reiners, A.: Three-dimensional simulations of near-surface convection in main-sequence stars - III. The structure of small-scale magnetic flux concentrations. Astronomy and Astrophysics 581, A42 (2015)
Beeck, B.; Schüssler, M.; Cameron, R. H.; Reiners, A.: Three-dimensional simulations of near-surface convection in main-sequence stars - IV. Effect of small-scale magnetic flux concentrations on centre-to-limb variation and spectral lines. Astronomy and Astrophysics 581, A43 (2015)
Hanasoge, S.; Miesch, M. S.; Roth, M.; Schou, J.; Schüssler, M.; Thompson, M. J.: Solar Dynamics, rotation, convection and overshoot. Space Science Reviews 196, S. 79 - 99 (2015)
Cameron, R. H.; Jiang, J.; Schuessler, M.; Gizon, L.: Physical causes of solar cycle amplitude variability. Journal of Geophysical Research: Space Physics 119, S. 680 - 688 (2014)
Jiang, J.; Cameron, R. H.; Schüssler, M.: Effects of the scatter in sunspot group tilt angles on the large‐scale magnetic field at the solar surface. Astrophysical Journal 791, 5 (2014)
Reiners, A.; Schüssler, M.; Passegger, V. M.: Generalized investigation of the rotation‐activity relation: Favoring rotation period instead of Rossby number. Astrophysical Journal 794, 144 (2014)
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)
Bewerbungsfrist 1 November 2022. Promotionsprojekte in Planetenwissenschaft, Sonnenphysik, Astrophysik, Magnetfelder der Sonne, Helioseismologie, Asteroseismologie ...
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