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K. Shibata

134 papers hereh-index 7017.5k citations597 works total

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

author position
  • first author6
  • middle author32
  • last author92

Across the 130 of 134 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR91
  • astro-ph32
  • astro-ph.EP3
  • astro-ph.HE3
  • physics.space-ph2
  • econ.GN1
same name
  • K. Shibata — 47 papers, h 27
  • K. Shibata — 13 papers, h 5
  • K. Shibata — 13 papers, h 9
  • K. Shibata — 12 papers, h 23
  • K. Shibata — 11 papers, h 28
  • K. Shibata — 11 papers, h 8

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

activity
19962023
most citedSuperflares on Solar Type Stars Observed with Kepler I. Statistical Properties of Superflares

492 citations · 8k across the 133 of their papers we have counts for

collaborators
Showing 2004Show all

3 papers · 1 filter

astro-ph2004★ 29 cited

The Acceleration Mechanism of Resistive MHD Jets Launched from Accretion Disks

T. Kuwabara, K. Shibata, T. Kudoh +1

We analyzed the results of non-linear resistive magnetohydrodynamical (MHD) simulations of jet formation to study the acceleration mechanism of axisymmetric, resistive MHD jets. Th…

astro-ph2004★ 61 cited

General Relativistic Magnetohydrodynamic Simulations of Collapsars: Rotating Black Hole Cases

Yosuke Mizuno, Shoichi Yamada, Shinji Koide +1

We have performed 2.5-dimensional general relativistic magnetohydrodynamic (MHD) simulations of collapsars including a rotating black hole. This paper is an extension of our previo…

astro-ph2004

The Log-normal Distributions of Physical Quantities of Flare associated Coronal Mass Ejections (CMEs), and Flare/CME Model of Gamma-ray Bursts

Seiichiro I. Aoki, Seiji Yashiro, Kazunari Shibata

We investigated the statistical distributions of physical quantities of solar flares and associated coronal mass ejections (CMEs). We found that the distributions of the X-ray peak…

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