283 citations · 4.2k across the 89 of their papers we have counts for
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Measurements of the atmospheric neutrino flux by Super-Kamiokande: energy spectra, geomagnetic effects, and solar modulation
E. Richard, K. Okumura, K. Abe +126
A comprehensive study on the atmospheric neutrino flux in the energy region from sub-GeV up to several TeV using the Super-Kamiokande water Cherenkov detector is presented in this…
Atmospheric Escape by Magnetically Driven Wind from Gaseous Planets II --Effects of Magnetic Diffusion--
Yuki A. Tanaka, Takeru K. Suzuki, Shu-ichiro Inutsuka
We investigate roles of Alfvenic waves in the weakly-ionized atmosphere of hot Jupiters by carrying out non-ideal magnetohydrodynamic (MHD) simulations with Ohmic diffusion in one-…
Formation of terrestrial planets in disks evolving via disk winds and implications for the origin of the solar system's terrestrial planets
Masahiro Ogihara, Hiroshi Kobayashi, Shu-ichiro Inutsuka +1
Recent three-dimensional magnetohydrodynamical simulations have identified a disk wind by which gas materials are lost from the surface of a protoplanetary disk, which can signific…
Dust Dynamics in Protoplanetary Disk Winds Driven by Magneto-Rotational Turbulence: A Mechanism for Floating Dust Grains with Characteristic Sizes
Tomoya Miyake, Takeru K. Suzuki, Shu-ichiro Inutsuka
We investigate the dynamics of dust grains with various sizes in protoplanetary disk winds driven by magnetorotational turbulence, by simulating the time evolution of the dust grai…
Stochastic Noncircular Motion and Outflows Driven by Magnetic Activity in the Galactic Bulge Region
Takeru K. Suzuki, Yasuo Fukui, Kazufumi Torii +2
By performing a global magneto-hydrodynamical simulation for the Milky Way with an axisymmetric gravitational potential, we propose that spatially dependent amplification of magnet…
Effects of axions on Nucleosynthesis in massive stars
Shohei Aoyama, Takeru K. Suzuki
We investigate the effect of the axion cooling on the nucleosynthesis in a massive star with by standard stellar evolution calculation. We find that the axion cooling…