116 citations · 513 across the 11 of their papers we have counts for
11 papers
Loss of toroidal magnetic flux by emergence of bipolar magnetic regions
R. H. Cameron, M. Schuessler
The polarity of the toroidal magnetic field in the solar convection zone periodically reverses in the course of the 11/22-year solar cycle. Among the various processes that contrib…
Solar activity: intrinsic periodicities beyond 11 years
Robert Cameron, Manfred Schuessler
Power spectra of solar activity based on historical records of sunspot numbers and on cosmogenic isotopes show peaks with enhanced power apart from the dominant 11-year solar cycle…
Are solar cycles predictable?
Manfred Schuessler
Various methods (or recipes) have been proposed to predict future solar activity levels - with mixed success. Among these, some precursor methods based upon quantities determined a…
Stokes diagnostics of simulated solar magneto-convection
S. Shelyag, M. Schuessler, S. K. Solanki +1
We present results of synthetic spectro-polarimetric diagnostics of radiative MHD simulations of solar surface convection with magnetic fields. Stokes profiles of Zeeman-sensitive…
The origin of the reversed granulation in the solar photosphere
M. C. C. Cheung, M. Schuessler, F. Moreno-Insertis
We study the structure and reveal the physical nature of the reversed granulation pattern in the solar photosphere by means of 3-dimensional radiative hydrodynamics simulations. We…
Magnetic flux transport on active cool stars and starspot lifetimes
Emre Isik, Manfred Schuessler, Sami K. Solanki
We carry out numerical simulations of the surface evolution of bipolar magnetic regions (BMRs) and magnetic spots on stars, which have radii and surface rotational shears of AB Dor…