activity
20082011
most citedA precise asteroseismic age and radius for the evolved Sun-like star KIC 11026764

163 citations · 323 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2011

LES of turbulent convection in solar-type stars and formation of large-scale magnetic structures

I. Rogachevskii, N. Kleeorin, I. N. Kitiashvili +3

In this study we investigate the effects of turbulent convection on formation of large-scale inhomogeneous magnetic structures by means of Large-Eddy Simulation (LES) for convectio…

astro-ph.SR201013 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.SR2010163 cited

A precise asteroseismic age and radius for the evolved Sun-like star KIC 11026764

T. S. Metcalfe, M. J. P. F. G. Monteiro, M. J. Thompson +55

The primary science goal of the Kepler Mission is to provide a census of exoplanets in the solar neighborhood, including the identification and characterization of habitable Earth-…

astro-ph.SR200943 cited

Traveling Waves of Magnetoconvection and the Origin of the Evershed Effect in Sunspots

Irina N. Kitiashvili, Alexander G. Kosovichev, Alan A. Wray +1

Discovered in 1909 the Evershed effect represents strong mass outflows in sunspot penumbra, where the magnetic field of sunspots is filamentary and almost horizontal. These flows p…

astro-ph.SR2009

Realistic Numerical Modeling of Solar Magnetoconvection and Oscillations

Irina Kitiashvili, Laetitia Jacoutot, Alexander Kosovichev +2

We have developed 3D, compressible, non-linear radiative MHD simulations to study the influence of the magnetic field of various strength and geometry on the turbulent convective c…

astro-ph200878 cited

Prediction of Sunspot Cycles by Data Assimilation Method

I. N. Kitiashvili, A. G. Kosovichev

Despite the known general properties of the solar cycles, a reliable forecast of the 11-year sunspot number variations is still a problem. The difficulties are caused by the appare…