activity
20162026
most citedThree-dimensional simulation of the fast solar wind driven by compressible magnetohydrodynamic turbulence

87 citations · 477 across the 33 of their papers we have counts for

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Showing 2025Show all

5 papers · 1 filter

astro-ph.SR2025

Influence of kinetic effects in large-scale magnetic reconnection with multi-hierarchy simulation code KAMMUY

Keita Akutagawa, Shinsuke Imada, Munehito Shoda

Magnetic reconnection is a multiscale phenomenon where fluid- and particle-scale processes interact. The particle-in-cell (PIC) method, capable of resolving kinetic (particle-scale…

astro-ph.SR2025

Empirical Optimization of the Source-Surface Height in the PFSS extrapolation

Munehito Shoda, Kyogo Tokoro, Daikou Shiota +1

The potential field source surface (PFSS) method is a widely used magnetic field extrapolation technique in the space weather community. The only free parameter in the PFSS method…

astro-ph.SR2025

Can plasmoid-mediated reconnection occur in collisionless systems?

Keita Akutagawa, Shinsuke Imada, Munehito Shoda

Magnetic reconnection is a process that converts magnetic energy into plasma energy by changing the magnetic field line topology. The outstanding question is why the reconnection r…

astro-ph.SR2025

Model of X-ray and extreme-UV emission from magnetically heated atmospheres in classical T Tauri stars: Case study of TW Hya

Munehito Shoda, Riouhei Nakatani, Shinsuke Takasao

Photoevaporation caused by X-rays and ultraviolet radiation from the central star has attracted attention as a key process driving the dispersal of protoplanetary discs. Although n…

astro-ph.SR2025★ 3 cited

Density fluctuation in the solar corona and solar wind: A comparative analysis of radio-occultation observations and magnetohydrodynamic simulation

Shota Chiba, Munehito Shoda, Takeshi Imamura

Recent in-situ observations and numerical models indicated various types of magnetohydrodynamic (MHD) waves contributing to the solar wind acceleration. Among them is an MHD wave d…