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Solar magnetoconvection and small-scale dynamo: Recent developments in observation and simulation
J. M. Borrero, S. Jafarzadeh, M. Schüssler +1
A number of observational and theoretical aspects of solar magnetoconvection are considered in this review. We discuss recent developments in our understanding of the small-scale s…
The cause of the weak solar cycle 24
Jie Jiang, Robert H. Cameron, Manfred Schuessler
The ongoing 11-year cycle of solar activity is considerably less vigorous than the three cycles before. It was preceded by a very deep activity minimum with a low polar magnetic fl…
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
Benjamin Beeck, Manfred Schüssler, Robert H. Cameron +1
Magnetic fields affect the local structure of the photosphere of stars. They can considerably influence the radiative properties near the optical surface, flow velocities, and the…
Three-dimensional simulations of near-surface convection in main-sequence stars. III. The structure of small-scale magnetic flux concentrations
Benjamin Beeck, Manfred Schüssler, Robert H. Cameron +1
The convective envelopes of cool main-sequence stars harbour magnetic fields with a complex global and local structure. These fields affect the near-surface convection and the oute…