activity
20072024
most citedReconnection-Condensation Model for Solar Prominence Formation

54 citations · 291 across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.SR2024

Conditions for Solar Prominence Formation Triggered by Single Localized Heating

Takero Yoshihisa, Takaaki Yokoyama, Takafumi Kaneko

We performed numerical simulations to study mechanisms of solar prominence formation triggered by a single heating event. In the widely accepted ``chromospheric-evaporation condens…

astro-ph.SR2022★ 8 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.SR2021★ 23 cited

Data-driven MHD simulation of successive solar plasma eruptions

Takafumi Kaneko, Sung-Hong Park, Kanya Kusano

Solar flares and plasma eruptions are sudden releases of magnetic energy stored in the plasma atmosphere. To understand the physical mechanisms governing their occurrences, three-d…

astro-ph.SR2018★ 22 cited

Impact of Dynamic State on the Mass Condensation Rate of Solar Prominences

Takafumi Kaneko, Takaaki Yokoyama

The interiors of quiescent prominences are filled with turbulent flows. The evolution of upflow plumes, descending pillars, and vortex motions has been clearly detected in high-res…

astro-ph.SR2017★ 54 cited

Reconnection-Condensation Model for Solar Prominence Formation

Takafumi Kaneko, Takaaki Yokoyama

We propose a reconnection-condensation model in which topological change in a coronal magnetic field via reconnection triggers radiative condensation, thereby resulting in prominen…

astro-ph.SR2015★ 25 cited

Apparent cross-field superslow propagation of magnetohydrodynamic waves in solar plasmas

T. Kaneko, M. Goossens, R. Soler +4

In this paper we show that the phase mixing of continuum Alfvén waves and/or continuum slow waves in magnetic structures of the solar atmosphere as, e.g., coronal arcades, can crea…