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astro-ph.SR2014★ 29 cited
Statistical Analysis of the Horizontal Divergent Flow in Emerging Solar Active Regions
Shin Toriumi, Keiji Hayashi, Takaaki Yokoyama
Solar active regions (ARs) are thought to be formed by magnetic fields from the convection zone. Our flux emergence simulations revealed that a strong horizontal divergent flow (HD…
astro-ph.SR2014★ 54 cited
Formation of a Flare-Productive Active Region: Observation and Numerical Simulation of NOAA AR 11158
S. Toriumi, Y. Iida, K. Kusano +2
We present a comparison of the Solar Dynamics Observatory (SDO) analysis of NOAA Active Region (AR) 11158 and numerical simulations of flux-tube emergence, aiming to investigate th…