activity
20152021
most citedEffects of a subadiabatic layer on convection and dynamos in spherical wedge simulations

30 citations · 246 across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.SR2021

Inferring magnetic helicity spectrum in spherical domains: the method and example applications

A. P. Prabhu, N. K. Singh, M. J. Käpylä +1

Obtaining observational constraints on the role of turbulent effects for the solar dynamo is a difficult, yet crucial, task. Without such knowledge, the full picture of the operati…

physics.flu-dyn2020★ 9 cited

On the existence of shear-current effects in magnetized burgulence

Maarit J. Käpylä, Javier Álvarez Vizoso, Matthias Rheinhardt +2

The possibility of explaining shear flow dynamos by a magnetic shear-current (MSC) effect is examined via numerical simulations. Our primary diagnostics is the determination of the…

astro-ph.SR2020★ 12 cited

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★ 20 cited

Topological changes in the magnetic field of LQ Hya during an activity minimum

Jyri J. Lehtinen, Maarit J. Käpylä, Thomas Hackman +6

Previous studies have related surface temperature maps, obtained with the Doppler imaging (DI) technique, of LQ Hya with long-term photometry. We compare surface magnetic field map…

astro-ph.SR2019★ 23 cited

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★ 25 cited

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…