activity
20172022
most citedSolar differential rotation reproduced with high-resolution simulation

59 citations · 175 across the 7 of their papers we have counts for

collaborators

12 papers

astro-ph.SR20228 cited

Impact of subsurface convective flows on the formation of sunspot magnetic field and energy build-up

Takafumi Kaneko, Hideyuki Hotta, Shin Toriumi +1

Strong solar flares occur in -spots characterized by the opposite-polarity magnetic fluxes in a single penumbra. Sunspot formation via flux emergence from the convection zone to…

astro-ph.SR202159 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…

astro-ph.SR202013 cited

Formation of super-strong horizontal magnetic field in delta-type sunspot in radiation magnetohydrodynamic simulations

H. Hotta, S. Toriumi

We perform a series of radiative magnetohydrodynamic simulations to understand the amplification mechanism of the exceptionally strong horizontal magnetic field in delta-type sunsp…

astro-ph.SR2020

On rising magnetic flux tube and formation of sunspots in a deep domain

H. Hotta, H. Iijima

We investigate the rising flux tube and the formation of sunspots in an unprecedentedly deep computational domain that covers the whole convection zone with a radiative magnetohydr…

astro-ph.SR201941 cited

Spontaneous Generation of delta-sunspots in Convective Magnetohydrodynamic Simulation of Magnetic Flux Emergence

Shin Toriumi, Hideyuki Hotta

Observations reveal that strong solar flares and coronal mass ejections tend to occur in complex active regions characterized by delta-sunspots, spot rotation, sheared polarity inv…