activity
20102015
most citedDifferential rotation in solar-like stars from global simulations

130 citations · 460 across the 9 of their papers we have counts for

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9 papers · 1 filter

astro-ph.SR2015★ 21 cited

Dynamics of Turbulent Convection and Convective Overshoot in a Moderate Mass Star

Irina N. Kitiashvili, Alexander G. Kosovichev, Nagi N. Mansour +1

Continued progress in observational stellar astrophysics requires a deep understanding of the underlying convection dynamics. We present results of realistic 3D radiative hydrodyna…

astro-ph.SR2015★ 94 cited

On the role of tachoclines in solar and stellar dynamos

G. Guerrero, P. K. Smolarkiewicz, E. M. de Gouveia Dal Pino +2

Rotational shear layers at the boundary between radiative and convective zones, tachoclines, play a key role in the process of magnetic field generation in solar-like stars. We pre…

astro-ph.SR2013★ 130 cited

Differential rotation in solar-like stars from global simulations

G. Guerrero, P. K. Smolarkiewicz, A. G. Kosovichev +1

To explore the physics of large-scale flows in solar-like stars, we perform 3D anelastic simulations of rotating convection for global models with stratification resembling the sol…

astro-ph.SR2013★ 5 cited

Solar differential rotation: hints to reproduce a near-surface shear layer in global simulations

G. Guerrero, P. K. Smolarkiewicz, A. Kosovichev +1

Convective turbulent motions in the solar interior, as well as the mean flows resulting from them, determine the evolution of the solar magnetic field. With the aim to get a better…

astro-ph.SR2010★ 13 cited

Numerical MHD Simulations of Solar Magnetoconvection and Oscillations in Inclined Magnetic Field Regions

I. N. Kitiashvili, A. G. Kosovichev, N. N. Mansour +1

The sunspot penumbra is a transition zone between the strong vertical magnetic field area (sunspot umbra) and the quiet Sun. The penumbra has a fine filamentary structure that is c…

astro-ph.SR2010★ 59 cited

Excitation of acoustic waves by vortices in the quiet Sun

I. N. Kitiashvili, A. G. Kosovichev, N. N. Mansour +1

Five-minutes oscillations is one of the basic properties of solar convection. Observations show mixture of a large number of acoustic wave fronts propagating from their sources. We…

astro-ph.SR2010★ 82 cited

Mechanism of spontaneous formation of stable magnetic structures on the Sun

I. N. Kitiashvili, A. G. Kosovichev, A. A. Wray +1

One of the puzzling features of solar magnetism is formation of long-living compact magnetic structures; such as sunspots and pores, in the highly turbulent upper layer of the sola…

astro-ph.SR2010★ 36 cited

Signatures of Emerging Subsurface Structures in Acoustic Power Maps

Thomas Hartlep, Alexander G. Kosovichev, Junwei Zhao +1

We show that under certain conditions, subsurface structures in the solar interior can alter the average acoustic power observed at the photosphere above them. By using numerical s…

astro-ph.SR2010★ 20 cited

Explanation of the sea-serpent magnetic structure of sunspot penumbrae

I. N. Kitiashvili, L. R. Bellot Rubio, A. G. Kosovichev +3

Recent spectro-polarimetric observations of a sunspot showed the formation of bipolar magnetic patches in the mid penumbra and their propagation toward the outer penumbral boundary…