activity
20172020
most citedLong-term variations of turbulent transport coefficients in a solar-like convective dynamo simulation

9 citations · 9 across the 1 of their papers we have counts for

collaborators

5 papers

astro-ph.SR2020

Shapes of stellar activity cycles

T. Willamo, T. Hackman, J. J. Lehtinen +4

Magnetic activity cycles are an important phenomenon in both the Sun and other stars. The shape of the solar cycle is commonly characterised by a fast rise and a slower decline, bu…

astro-ph.SR2019

Differences in the solar cycle variability of simple and complex active regions during 1996-2018

Shabnam Nikbakhsh, Eija Tanskanen, Maarit Käpylä +1

Aims. Our aim is to examine the solar cycle variability of magnetically simple and complex active region. Methods. We studied simple ( and ) and complex ( and ) acti…

astro-ph.SR2019

Stellar dynamos in the transition regime: multiple dynamo modes and anti-solar differential rotation

M. Viviani, M. J. Käpylä, J. Warnecke +2

Global and semi-global convective dynamo simulations of solar-like stars are known to show a transition from an anti-solar (fast poles, slow equator) to solar-like (fast equator, s…

astro-ph.SR2018

Starspot activity of HD 199178. Doppler images from 1994--2017

Thomas Hackman, Iya Ilyin, Jyri J. Lehtinen +4

Context. Studying the spots of late-type stars is crucial for distinguishing between the various proposed dynamo mechanisms believed to be the main cause of starspot activity. For…

astro-ph.SR20179 cited

Long-term variations of turbulent transport coefficients in a solar-like convective dynamo simulation

Frederick A. Gent, Maarit J. Käpylä, Jörn Warnecke

The Sun, aside from its eleven year sunspot cycle is additionally subject to long term variation in its activity. In this work we analyse a solar-like convective dynamo simulation,…