activity
20102013
most citedCyclic magnetic activity due to turbulent convection in spherical wedge geometry

157 citations · 1.1k across the 23 of their papers we have counts for

collaborators

23 papers

astro-ph.GA2013★ 15 cited

High-resolution ammonia mapping of the very young protostellar core Chamaeleon-MMS1

M. S. Väisälä, J. Harju, M. J. Mantere +4

Cha-MMS1 was mapped in the NH_3(1,1) line and the 1.2 cm continuum using the Australia Telescope Compact Array, ATCA. The angular resolution of the ATCA observations is 7'' (~ 1000…

astro-ph.SR2013★ 48 cited

Azimuthal dynamo wave in spherical shell convection

Elizabeth Cole, Petri J. Käpylä, Maarit J. Mantere +1

We report the finding of an azimuthal dynamo wave of a low-order (m=1) mode in direct numerical simulations (DNS) of turbulent convection in spherical shells. Such waves are predic…

astro-ph.SR2013★ 27 cited

Multiperiodicity, modulations and flip-flops in variable star light curves II. Analysis of II Peg photometry during 1979-2010

Marjaana Lindborg, Maarit J. Mantere, Nigul Olspert +5

According to earlier Doppler images of the magnetically active primary giant component of the RS CVn binary II Peg, the surface of the star was dominated by one single active longi…

astro-ph.SR2013★ 54 cited

Magnetic field topology of the RS CVn star II Pegasi

O. Kochukhov, M. J. Mantere, T. Hackman +1

The dynamo processes in cool active stars generate complex magnetic fields responsible for prominent surface stellar activity and variability at different time scales. For a small…

astro-ph.SR2013★ 138 cited

Effects of enhanced stratification on equatorward dynamo wave propagation

Petri J. Käpylä, Maarit. J. Mantere, Elizabeth Cole +2

We present results from simulations of rotating magnetized turbulent convection in spherical wedge geometry representing parts of the latitudinal and longitudinal extents of a star…

astro-ph.SR2013★ 52 cited

Spoke-like differential rotation in a convective dynamo with a coronal envelope

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

We report on the results of four convective dynamo simulations with an outer coronal layer. The magnetic field is self-consistently generated by the convective motions beneath the…