activity
20162023
most citedThree-dimensional simulation of the fast solar wind driven by compressible magnetohydrodynamic turbulence

87 citations · 134 across the 6 of their papers we have counts for

collaborators

10 papers

astro-ph.SR2023

Can the solar p-modes contribute to the high-frequency transverse oscillations of spicules?

Hidetaka Kuniyoshi, Munehito Shoda, Richard J. Morton +1

Lateral motions of spicules serve as vital indicators of transverse waves in the solar atmosphere, and their study is crucial for understanding the wave heating process of the coro…

astro-ph.SR2022

Role of Longitudinal Waves in Alfven-wave-driven Solar/Stellar Wind

Kimihiko Shimizu, Munehito Shoda, Takeru K. Suzuki

We study the role the the p-mode-like vertical oscillation on the photosphere in driving solar winds in the framework of Alfven-wave-driven winds. By performing one-dimensional mag…

astro-ph.SR20227 cited

The Effect of the Chromospheric Temperature on Coronal Heating

Haruka Washinoue, Munehito Shoda, Takeru K. Suzuki

Recent observational and numerical studies show a variety of thermal structures in the solar chromosphere. Given that the thermal interplay across the transition region is a key to…

astro-ph.SR2022

Testing the Alfvén-wave model of the solar wind with interplanetary scintillation

Munehito Shoda, Kazumasa Iwai, Daikou Shiota

Understanding the mechanism(s) of the solar wind acceleration is important in astrophysics and geophysics. A promising model of the solar wind acceleration is known as the wave/tur…

astro-ph.SR2021

Turbulent generation of magnetic switchbacks in the Alfvénic solar wind

Munehito Shoda, Benjamin D. G. Chandran, Steven R. Cranmer

One of the most important early results from the Parker Solar Probe (PSP) is the ubiquitous presence of magnetic switchbacks, whose origin is under debate. Using a three-dimensiona…

astro-ph.SR202040 cited

Alfvén-wave driven magnetic rotator winds from low-mass stars I: rotation dependences of magnetic braking and mass-loss rate

Munehito Shoda, Takeru K. Suzuki, Sean P. Matt +7

Observations of stellar rotation show that low-mass stars lose angular momentum during the main sequence. We simulate the winds of Sun-like stars with a range of rotation rates, co…