papers

Publications (19)

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 $βγδ…

astro-ph.SR2011

Dependence of the large-scale vortex instability on latitude, stratification and domain size

Maarit J. Mantere, Petri J. Käpylä, Thomas Hackman

In an earlier study, we reported on the excitation of large-scale vortices in Cartesian hydrodynamical convection models subject to rapid enough rotation. In that study, the condit…

astro-ph.SR2025

Magnetic evolution of complex solar active regions

Shabnam Nikbakhsh, Eija I. Tanskanen, Thomas Hackman

Aims. This study investigates the magnetic evolution of solar active regions (ARs), with a particular focus on understanding how the magnetic morphology of simple and complex ARs c…

astro-ph.SR2019

Spot evolution on LQ Hya during 2006--2017: temperature maps based on SOFIN and FIES data

Elizabeth M. Cole-Kodikara, Maarit J. Käpylä, Jyri J. Lehtinen +4

Context. LQ Hya is one of the most frequently studied young solar analogue stars. Recently, it has been observed to show intriguing behaviour by analysing long-term photometry: dur…

astro-ph.SR2019

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.SR2014

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…