activity
20072025
most citedMechanism of spontaneous formation of stable magnetic structures on the Sun

82 citations · 525 across the 26 of their papers we have counts for

collaborators

27 papers

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

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…

astro-ph.SR2025

Revisiting turbulent properties of solar convection with 3D radiative hydrodynamic modeling

Irina N. Kitiashvili, Alan A. Wray

We discuss the turbulent structure and dynamics of the upper solar convection zone using a 3D radiative hydrodynamic simulation model at 45 degrees latitude. The model reveals the…

astro-ph.SR2022★ 21 cited

Leptocline as a Shallow Substructure of Near-Surface Shear Layer in 3D Radiative Hydrodynamic Simulations

Irina N. Kitiashvili, Alexander G. Kosovichev, Alan A. Wray +2

Understanding effects driven by rotation in the solar convection zone is essential for many problems related to solar activity, such as the formation of differential rotation, meri…

astro-ph.SR2022★ 1 cited

Modeling Stellar Jitter for the Detection of Earth-Mass Exoplanets via Precision Radial Velocity Measurements

Samuel Granovsky, Irina N. Kitiashvili, Alan Wray

The detection of Earth-size exoplanets is a technological and data analysis challenge. Future progress in Earth-mass exoplanet detection is expected from the development of extreme…

astro-ph.SR2021

3D Modeling of the Structure and Dynamics of a Main-Sequence F-type Star

Irina N. Kitiashvili, Alan A. Wray

Current state-of-the-art computational modeling makes it possible to build realistic models of stellar convection zones and atmospheres that take into account chemical composition,…