output
19922026
Showing 2014 · astro-ph.SRShow all

11 papers · 2 filters

astro-ph.SR2014★ 11 cited

Doppler images and the underlying dynamo. The case of AF Leporis

S. P. Järvinen, R. Arlt, T. Hackman +6

The (Zeeman-)Doppler imaging studies of solar-type stars very often reveal large high-latitude spots. This also includes F stars that possess relatively shallow convection zones, i…

astro-ph.SR2014★ 2 cited

Dynamical quenching with non-local alpha and downward pumping

A. Brandenburg, A. Hubbard, P. J. Käpylä

In light of new results, the one-dimensional mean-field dynamo model of Brandenburg & Kapyla (2007) with dynamical quenching and a nonlocal Babcock-Leighton alpha effect is re-exam…

astro-ph.SR2014★ 11 cited

Multiperiodicity, modulations and flip-flops in variable star light curves III. Carrier fit analysis of LQ Hya photometry for 1982-2014

Nigul Olspert, Maarit J. Käpylä, Jaan Pelt +4

We study LQ Hya photometry for 1982-2014 with the carrier fit (CF) -method and compare our results to earlier photometric analysis and recent Doppler imaging maps. We first utilize…

astro-ph.SR2014★ 63 cited

On the cause of solar-like equatorward migration in global convective dynamo simulations

Jörn Warnecke, Petri J. Käpylä, Maarit J. Käpylä +1

We present results from four convectively-driven stellar dynamo simulations in spherical wedge geometry. All of these simulations produce cyclic and migrating mean magnetic fields.…

astro-ph.SR2014

A Space Weather Mission Concept: Observatories of the Solar Corona and Active Regions (OSCAR)

Antoine Strugarek, Nils Janitzek, Arrow Lee +14

Coronal Mass Ejections (CMEs) and Corotating Interaction Regions (CIRs) are major sources of magnetic storms on Earth and are therefore considered to be the most dangerous space we…

astro-ph.SR2014★ 102 cited

Magnetically controlled stellar differential rotation near the transition from solar to anti-solar profiles

Bidya Binay Karak, Petri J. Kapyla, Maarit J. Kapyla +3

Late-type stars rotate differentially owing to anisotropic turbulence in their outer convection zones. The rotation is called solar-like (SL) when the equator rotates fastest and a…