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astro-ph.SR2021★ 59 cited
Solar differential rotation reproduced with high-resolution simulation
H. Hotta, K. Kusano
The Sun rotates differentially with a fast equator and slow pole. Convection in the solar interior is thought to maintain the differential rotation. However, although many numerica…
astro-ph.SR2021
Relationship between magnetic field properties and statistical flow using numerical simulation and magnetic feature tracking on solar photosphere
K. Takahata, H. Hotta, Y. Iida +1
We perform radiative magnetohydrodynamic calculations for the solar quiet region to investigate the dependence of statistical flow on magnetic properties and the three-dimensional…