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19942018
most citedDoes a Non-Magnetic Solar Chromosphere Exist?

359 citations · 2.7k across the 38 of their papers we have counts for

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astro-ph2008★ 1 cited

Supergranulation Scale Connection Simulations

R. F. Stein, A. Nordlund, D. Georgobiani +2

Results of realistic simulations of solar surface convection on the scale of supergranules (96 Mm wide by 20 Mm deep) are presented. The simulations cover only 10% of the geometric…

astro-ph2007★ 36 cited

Helioseismic Holography of Simulated Solar Convection and Prospects for the Detection of Small-Scale Subsurface Flows

D. C. Braun, A. C. Birch, D. Benson +2

We perform helioseismic holography on realistic solar convection simulations and compare the observed travel-time perturbations with the expected travel times from the horizontal f…

astro-ph2006★ 67 cited

Validation of Time-Distance Helioseismology by Use of Realistic Simulations of Solar Convection

Junwei Zhao, Dali Georgobiani, Alexander G. Kosovichev +3

Recent progress in realistic simulations of solar convection have given us an unprecedented opportunity to evaluate the robustness of solar interior structures and dynamics obtaine…

astro-ph2006★ 140 cited

Excitation of solar-like oscillations across the HR diagram

R. Samadi, D. Georgobiani, R. Trampedach R. +3

We extend semi-analytical computations of excitation rates for solar oscillation modes to those of other solar-like oscillating stars to compare them with recent observations. Nume…

astro-ph2006★ 51 cited

Local helioseismology and correlation tracking analysis of surface structures in realistic simulations of solar convection

Dali Georgobiani, Junwei Zhao, Alexander Kosovichev +3

We apply time-distance helioseismology, local correlation tracking and Fourier spatial-temporal filtering methods to realistic supergranule scale simulations of solar convection an…

astro-ph2005★ 29 cited

Effect of the radiative background flux in convection

A. Brandenburg, K. L. Chan, A. Nordlund +1

Numerical simulations of turbulent stratified convection are used to study models with approximately the same convective flux, but different radiative fluxes. As the radiative flux…