353 citations · 4.5k across the 52 of their papers we have counts for
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Generalized investigation of the rotation-activity relation: Favouring rotation period instead of Rossby number
A. Reiners, M. Schuessler, V. M. Passegger
Magnetic activity in Sun-like and low-mass stars causes X-ray coronal emission, which is stronger for more rapidly rotating stars. This relation is often interpreted in terms of th…
MHD simulations of near-surface convection in cool main-sequence stars
Benjamin Beeck, Manfred Schüssler, Ansgar Reiners
The solar photospheric magnetic field is highly structured owing to its interaction with the convective flows. Its local structure has a strong influence on the profiles of spectra…
Comparison of solar photospheric bright points between SUNRISE observations and MHD simulations
T. L. Riethmüller, S. K. Solanki, S. V. Berdyugina +5
Bright points (BPs) in the solar photosphere are radiative signatures of magnetic elements described by slender flux tubes located in the darker intergranular lanes. They contribut…
Effects of the scatter in sunspot group tilt angles on the large-scale magnetic field at the solar surface
J. Jiang, R. H. Cameron, M. Schuessler
The tilt angles of sunspot groups represent the poloidal field source in Babcock-Leighton-type models of the solar dynamo and are crucial for the build-up and reversals of the pola…