activity
20102024
most citedPlanet Hunters X. KIC 8462852 - Where's the Flux?

289 citations · 895 across the 26 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

24 papers · 1 filter

astro-ph.SR2024

Characterising the stellar differential rotation based on largest-spot statistics from ground-based photometry

Mikko Tuomi, Jyri J. Lehtinen, Gregory W. Henry +1

Stellar spot distribution has consequences on the observable periodic signals in long-time baseline ground-based photometry. We model the statistics of the dominating spots of two…

astro-ph.SR2023

From convective stellar dynamo simulations to Zeeman-Doppler images

Thomas Hackman, Oleg Kochukhov, Mariangela Viviani +3

Zeeman-Doppler imaging (ZDI) is used to reconstruct the surface magnetic field of late-type stars from high resolution spectropolarimetric observations. The results are usually des…

astro-ph.SR2022★ 4 cited

V889 Her: abrupt changes in the magnetic field or differential rotation?

Teemu Willamo, Thomas Hackman, Jyri J. Lehtinen +2

We have applied Zeeman-Doppler imaging (ZDI) to an extensive spectropolarimetric HARPSpol data set of the magnetically active young solar analogue V889 Her, covering 35 spectra obt…

astro-ph.SR2020★ 16 cited

A Knee-Point in the Rotation-Activity Scaling of Late-type Stars with a Connection to Dynamo Transitions

Jyri J. Lehtinen, Maarit J. Käpylä, Nigul Olspert +1

The magnetic activity of late-type stars is correlated with their rotation rates. Up to a certain limit, stars with smaller Rossby numbers, defined as the rotation period divided b…

astro-ph.SR2020★ 41 cited

Common dynamo scaling in slowly rotating young and evolved stars

Jyri J. Lehtinen, Federico Spada, Maarit J. Käpylä +2

One interpretation of the activity and magnetism of late-type stars is that these both intensify with decreasing Rossby number up to a saturation level, suggesting that stellar dyn…

astro-ph.SR2020★ 87 cited

Hidden magnetic fields of young suns

O. Kochukhov, T. Hackman, J. J. Lehtinen +1

Global magnetic fields of active solar-like stars are nowadays routinely detected with spectropolarimetric measurements and are mapped with Zeeman-Doppler imaging (ZDI). However, d…