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S. Mori

3 papers hereh-index 201.6k citations132 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author2
  • middle author1

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP3
same name
  • S. Mori — 22 papers, h 11
  • S. Mori — 20 papers, h 10
  • S. Mori — 12 papers, h 34
  • S. Mori — 8 papers, h 13
  • S. Mori — 4 papers, h 31
  • S. Mori — 3 papers, h 6

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

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

81 citations · 99 across the 3 of their papers we have counts for

collaborators
Showing astro-ph.EPShow all

3 papers · 1 filter

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…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.