D-Index & Metrics Best Publications
Shu-ichiro Inutsuka

Shu-ichiro Inutsuka

D-Index & Metrics D-index (Discipline H-index) only includes papers and citation values for an examined discipline in contrast to General H-index which accounts for publications across all disciplines.

Discipline name D-index D-index (Discipline H-index) only includes papers and citation values for an examined discipline in contrast to General H-index which accounts for publications across all disciplines. Citations Publications World Ranking National Ranking
Physics D-index 86 Citations 21,330 376 World Ranking 1866 National Ranking 55

Overview

What is he best known for?

The fields of study he is best known for:

  • Astronomy
  • Astrophysics
  • Thermodynamics

Shu-ichiro Inutsuka mainly investigates Astrophysics, Magnetohydrodynamics, Molecular cloud, Protostar and Interstellar medium. His Astrophysics study frequently draws parallels with other fields, such as Astronomy. His Magnetorotational instability study, which is part of a larger body of work in Magnetohydrodynamics, is frequently linked to Magnetic pressure, bridging the gap between disciplines.

His research in Molecular cloud intersects with topics in Molecular physics, Fragmentation and Isothermal process. He combines subjects such as Gravitational collapse, Spectral energy distribution, Field line and Angular momentum with his study of Protostar. Shu-ichiro Inutsuka focuses mostly in the field of Interstellar medium, narrowing it down to matters related to Shock wave and, in some cases, Supernova and Interstellar cloud.

His most cited work include:

  • A Radiation Hydrodynamic Model for Protostellar Collapse. II. The Second Collapse and the Birth of a Protostar (431 citations)
  • Discovery of Small-Scale Spiral Structures in the Disk of SAO 206462 (HD 135344B): Implications for the Physical State of the Disk from Spiral Density Wave Theory (364 citations)
  • An Origin of Supersonic Motions in Interstellar Clouds (319 citations)

What are the main themes of his work throughout his whole career to date?

Shu-ichiro Inutsuka mainly investigates Astrophysics, Molecular cloud, Star formation, Astronomy and Magnetohydrodynamics. Shu-ichiro Inutsuka regularly links together related areas like Turbulence in his Astrophysics studies. His Molecular cloud research integrates issues from Gravitational collapse, Shock wave, Supernova and Angular momentum.

Shu-ichiro Inutsuka has researched Star formation in several fields, including Fragmentation and Redshift. His work on Magnetorotational instability as part of general Magnetohydrodynamics study is frequently linked to Magnetic pressure, bridging the gap between disciplines. His studies in Protostar integrate themes in fields like Accretion and Outflow.

He most often published in these fields:

  • Astrophysics (72.45%)
  • Molecular cloud (26.33%)
  • Star formation (21.63%)

What were the highlights of his more recent work (between 2018-2021)?

  • Astrophysics (72.45%)
  • Molecular cloud (26.33%)
  • Star formation (21.63%)

In recent papers he was focusing on the following fields of study:

His scientific interests lie mostly in Astrophysics, Molecular cloud, Star formation, Stars and Interstellar medium. His Astrophysics research incorporates themes from Turbulence and Outflow. His work deals with themes such as Shock wave, Magnetohydrodynamics and Mass fraction, which intersect with Turbulence.

Shu-ichiro Inutsuka has included themes like Eddy current brake and Ohm's law in his Magnetohydrodynamics study. His research in Molecular cloud intersects with topics in Supernova remnant, Cosmic ray, Gravitational collapse, Line-of-sight and Millimeter. His Star formation study incorporates themes from Spectral line, Continuum and Redshift.

Between 2018 and 2021, his most popular works were:

  • The role of magnetic field in molecular cloud formation and evolution (68 citations)
  • The JCMT BISTRO Survey: The Magnetic Field In The Starless Core $ ho$ Ophiuchus C (25 citations)
  • The JCMT BISTRO Survey: The Magnetic Field of the Barnard 1 Star-Forming Region. (25 citations)

In his most recent research, the most cited papers focused on:

  • Astronomy
  • Astrophysics
  • Thermodynamics

His primary areas of study are Astrophysics, Molecular cloud, Star formation, James Clerk Maxwell Telescope and Stars. His study connects Turbulence and Astrophysics. Shu-ichiro Inutsuka interconnects Continuum, Infrared, Outflow, Submillimeter Array and Protoplanetary disk in the investigation of issues within Molecular cloud.

Shu-ichiro Inutsuka combines subjects such as Planetary science, Fragmentation and Interstellar medium with his study of Star formation. His Interstellar medium study deals with Thermal intersecting with Magnetohydrodynamics, Gravitation and Virial theorem. His work on Small Magellanic Cloud as part of his general Stars study is frequently connected to Type, thereby bridging the divide between different branches of science.

This overview was generated by a machine learning system which analysed the scientist’s body of work. If you have any feedback, you can contact us here.

Best Publications

A Radiation Hydrodynamic Model for Protostellar Collapse. II. The Second Collapse and the Birth of a Protostar

Hirohiko Masunaga;Shu-ichiro Inutsuka.
The Astrophysical Journal (2000)

544 Citations

Angular Momentum Transport by MHD Turbulence in Accretion Disks: Gas Pressure Dependence of the Saturation Level of the Magnetorotational Instability

Takayoshi Sano;Shu-ichiro Inutsuka;Neal J. Turner;James M. Stone.
arXiv: Astrophysics (2003)

413 Citations

Discovery of Small-Scale Spiral Structures in the Disk of SAO 206462 (HD 135344B): Implications for the Physical State of the Disk from Spiral Density Wave Theory

T. Muto;T. Muto;C. A. Grady;J. Hashimoto;M. Fukagawa.
The Astrophysical Journal (2012)

404 Citations

An Origin of Supersonic Motions in Interstellar Clouds

Hiroshi Koyama;Shu-ichiro Inutsuka.
The Astrophysical Journal (2001)

401 Citations

Disk Winds Driven by Magnetorotational Instability and Dispersal of Proto-Planetary Disks

T. K. Suzuki;S. Inutsuka.
arXiv: Astrophysics (2008)

387 Citations

Making the corona and the fast solar wind: a self-consistent simulation for the low-frequency Alfven waves from photosphere to 0.3AU

Takeru K. Suzuki;Shu-ichiro Inutsuka.
arXiv: Astrophysics (2005)

370 Citations

Self-similar Solutions and the Stability of Collapsing Isothermal Filaments

Shu-Ichiro Inutsuka;Shoken M. Miyama.
The Astrophysical Journal (1992)

329 Citations

A Radiation Hydrodynamic Model for Protostellar Collapse. I. The First Collapse

Hirohiko Masunaga;Shoken M. Miyama;Shu-ichiro Inutsuka.
The Astrophysical Journal (1998)

329 Citations

A Production Mechanism for Clusters of Dense Cores

Shu-ichiro Inutsuka;Shoken M. Miyama.
The Astrophysical Journal (1997)

317 Citations

ANGULAR MOMENTUM TRANSPORT BY MAGNETOHYDRODYNAMIC TURBULENCE IN ACCRETION DISKS: GAS PRESSURE DEPENDENCE OF THE SATURATION LEVEL OF THE MAGNETOROTATIONAL INSTABILITY

Takayoshi Sano;Takayoshi Sano;Shu-ichiro Inutsuka;Neal J. Turner;Neal J. Turner;James M. Stone;James M. Stone.
The Astrophysical Journal (2004)

306 Citations

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