activity
20152019
most citedTemperature Structure in the Inner Regions of Protoplanetary Disks: Inefficient Accretion Heating Controlled by Nonideal Magnetohydrodynamics

81 citations · 119 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.EP2019★ 8 cited

The Generalized Nonlinear Ohm's Law: How a Strong Electric Field Influences Non-ideal MHD Effects in Dusty Protoplanetary Disks

Satoshi Okuzumi, Shoji Mori, Shu-ichiro Inutsuka

The magnetohydrodynamics (MHD) of protoplanetary disks are strongly subject to the non-ideal MHD effects arising from the low ionization fraction of the disk gas. A strong electric…

astro-ph.EP2019★ 81 cited

Temperature Structure in the Inner Regions of Protoplanetary Disks: Inefficient Accretion Heating Controlled by Nonideal Magnetohydrodynamics

Shoji Mori, Xue-Ning Bai, Satoshi Okuzumi

The gas temperature in protoplanetary disks (PPDs) is determined by a combination of irradiation heating and accretion heating, with the latter conventionally attributed to turbule…

astro-ph.EP2017★ 10 cited

Electron Heating and Saturation of Self-regulating Magnetorotational Instability in Protoplanetary Disks

Shoji Mori, Takayuki Muranushi, Satoshi Okuzumi +1

Magnetorotational instability (MRI) has a potential to generate the vigorous turbulence in protoplanetary disks, although its turbulence strength and accretion stress remains debat…

astro-ph.EP2015★ 20 cited

Electron Heating in the Magnetorotational Instability: Implications for Turbulence Strength in Outer Regions of Protoplanetary Disks

Shoji Mori, Satoshi Okuzumi

The magnetorotational instability (MRI) drives vigorous turbulence in a region of protoplanetary disks where the ionization fraction is sufficiently high. It has recently been show…