activity
20102026
most citedDifferential rotation in solar-like stars from global simulations

130 citations · 492 across the 24 of their papers we have counts for

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Showing 2025Show all

6 papers · 1 filter

astro-ph.SR2025

3D Radiative MHD Modeling of Particle Beam Heating of the Solar Atmosphere

Samuel Granovsky, Alexander G. Kosovichev, Irina N. Kitiashvili +1

While solar flares are primarily associated with enhanced ultraviolet and X-ray emission, a subset of flares exhibit significant continuum brightening in visible light and are clas…

astro-ph.SR2025

Activity-Cycle Variations of Convection Scales in Subsurface Layers of the Sun

Alexander V. Getling, Alexander G. Kosovichev

We use subsurface-flow velocity maps inferred by time--distance helioseismology from Doppler measurements with the Helioseismic and Magnetic Imager (HMI) of the Solar Dynamics Obse…

astro-ph.SR2025

Helicity Fluxes and Hemispheric Helicity Rule of Active Regions Emerging from the Convection Zone Dynamo

V. V. Pipin, Shangbin Yang, A. G. Kosovichev

Using a 3D non-linear mean-field solar dynamo model, we investigate the magnetic helicity flux and magnetic twist, and tilt parameters of bipolar magnetic regions (BMRs) emerging f…

astro-ph.SR2025

Time-Dependence of Subsurface Solar Convection Using the Time-Distance Deep-Focus Method

John T. Stefan, Alexander G. Kosovichev, Gustavo Guerrero +1

We re-examine the deep-focus methodology of time-distance helioseismology previously used to estimate the power spectrum of the solar convection at a depth of about 30 Mm, which wa…

astro-ph.SR2025

Improving Our Knowledge of the Solar Near-Surface Shear Layer: The Special Case of the Leptocline

Jean-Pierre Rozelot, Alexander Kosovichev, Irina Kitiashvili

The discovery of the solar activity cycle was linked from the outset to the observation of the temporal variability of sunspots, which we know to be the result of complex processes…

astro-ph.SR2025

Properties of Turbulent Convection and Large-Scale Flows in a Rotating F-type Star Revealed by 3D Realistic Radiative Hydrodynamic Simulations

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

The nonlinear coupling between stellar convection and rotation is of great interest because it relates to understanding both stellar evolution and activity. We investigated the inf…