activity
19972025
most citedTransverse instability for non-normal parameters

61 citations · 421 across the 31 of their papers we have counts for

collaborators
Showing astro-phShow all

18 papers · 1 filter

astro-ph2004★ 51 cited

Dynamo models and differential rotation in late-type rapidly rotating stars

E. Covas, D. Moss, R. Tavakol

Increasing evidence is becoming available about not only the surface differential rotation of rapidly rotating cool stars but, in a small number of cases, also about temporal varia…

astro-ph2003★ 38 cited

The influence of density stratification and multiple nonlinearities on solar torsional oscillations

Eurico Covas, David Moss, Reza Tavakol

Analyses of recent helioseismic data have produced ample evidence for substantial dynamical variation of the differential rotation within the solar convection zone. Given the inevi…

astro-ph2002★ 11 cited

Effects of boundary conditions on the dynamics of the solar convection zone

Reza Tavakol, Eurico Covas, David Moss +1

Recent analyses of the helioseismic data have produced evidence for a variety of interesting dynamical behaviour associated with torsional oscillations. What is not so far clear is…

astro-ph2002

Solar Cycle Variation of the Solar Internal Rotation: Helioseismic Inversion and Dynamo Modelling

S. Vorontsov, R. Tavakol, E. Covas +1

We report our first results on comparing the variations of the solar internal rotation with solar activity, as predicted by non-linear solar dynamo modelling, with helioseismic mea…

astro-ph2001★ 5 cited

Spatiotemporal fragmentation and the uncertainties in the solar rotation law

Eurico Covas, Reza Tavakol, Sergei Vorontsov +1

Analyses of recent helioseismic data indicate that the dynamical regimes at the base of the convection zone can be different from those observed at the top, having either significa…

astro-ph2001

Aspects of the dynamics underlying solar and stellar dynamo models

Reza Tavakol, Eurico Covas

Observations of the Sun and solar-type stars continue to reveal phenomena whose understanding is very likely to require a nonlinear framework. Here we shall concentrate on two such…