Publication data of Inutsuka, Shu-ichiro: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion200020052010201520202025050010001500200025003000
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications200020052010201520202025025507510012503691215
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion20002005201020152020202505101520253035
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestDynamical expansion of ionization and dissociation front around a massive star. 2. on the generality of triggered star formationDynamical expansion of ionization and dissociation front around a massive st…Two-Fluid MHD Simulations of Converging HI Flows in the Interstellar Medium. I: Methodology and Basic ResultsTwo-Fluid MHD Simulations of Converging HI Flows in the Interstellar Medium.…Self-sustained ionization and vanishing dead zones in protoplanetary disksThe field condition: a new constraint of spatial resolution in simulations of thermally unstable hydrodynamicsThe field condition: a new constraint of spatial resolution in simulations of th…An upper limit on the mass of a primordial star due to the formation of an hii region: the effect of ionizing radiation forceAn upper limit on the mass of a primordial star due to the formation of an hii …Making the corona and the fast solar wind: A Self-consistent simulation for the low-frequency Alfven waves from photosphere to 0.3 AUMaking the corona and the fast solar wind: A Self-consistent simulation for th…Protoplanetary Disk Winds by Magnetorotational Instability : Formation of an Inner Hole and a Crucial Assist for Planet FormationProtoplanetary Disk Winds by Magnetorotational Instability : Formation of an …Formation Scenario for Wide and Close Binary SystemsConditions for the Formation of First-Star BinariesMagnetohydrodynamic Simulations of Global Accretion Disks with Vertical Magnetic FieldsMagnetohydrodynamic Simulations of Global Accretion Disks with Vertical Ma…Saturation and thermalization of the magnetorotational instability: recurrent channel flows and reconnectionsSaturation and thermalization of the magnetorotational instability: recurrent …Molecular evolution in collapsing prestellar coresDisk Winds Driven by Magnetorotational Instability and Dispersal of Proto-Planetary DisksDisk Winds Driven by Magnetorotational Instability and Dispersal of Proto-Pla…A Detailed Study of the Molecular and Atomic Gas Toward the {gamma}-ray SNR RX J1713.7-3946: Spatial TeV {gamma}-ray and ISM Gas CorrespondenceA Detailed Study of the Molecular and Atomic Gas Toward the {gamma}-ray …Molecular cloud formation in shock-compressed layersTurbulence and Magnetic Field Amplification in Supernova Remnants: Interactions Between A Strong Shock Wave and Multi-Phase Interstellar MediumTurbulence and Magnetic Field Amplification in Supernova Remnants: Interac…An origin of supersonic motions in interstellar cloudsAngular momentum transport by MHD turbulence in accretion disks: Gas pressure dependence of the saturation level of the magnetorotational instabilityAngular momentum transport by MHD turbulence in accretion disks: Gas pre…Toward Understanding the Cosmic-ray Acceleration at Young Supernova Remnants Interacting with Interstellar Clouds: Possible Applications to RX J1713.7-3946Toward Understanding the Cosmic-ray Acceleration at Young Supernova Rem…200020052010201520202025050010001500200025003000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)Dynamical expansion of ionization and dissociation front around a massive star. 2. on the generality of triggered star formationDynamical expansion of ionization and dissociation front around a massive st…Two-Fluid MHD Simulations of Converging HI Flows in the Interstellar Medium. I: Methodology and Basic ResultsTwo-Fluid MHD Simulations of Converging HI Flows in the Interstellar Medium.…Self-sustained ionization and vanishing dead zones in protoplanetary disksThe field condition: a new constraint of spatial resolution in simulations of thermally unstable hydrodynamicsThe field condition: a new constraint of spatial resolution in simulations of th…An upper limit on the mass of a primordial star due to the formation of an hii region: the effect of ionizing radiation forceAn upper limit on the mass of a primordial star due to the formation of an hii …Making the corona and the fast solar wind: A Self-consistent simulation for the low-frequency Alfven waves from photosphere to 0.3 AUMaking the corona and the fast solar wind: A Self-consistent simulation for th…Protoplanetary Disk Winds by Magnetorotational Instability : Formation of an Inner Hole and a Crucial Assist for Planet FormationProtoplanetary Disk Winds by Magnetorotational Instability : Formation of an …Formation Scenario for Wide and Close Binary SystemsConditions for the Formation of First-Star BinariesMagnetohydrodynamic Simulations of Global Accretion Disks with Vertical Magnetic FieldsMagnetohydrodynamic Simulations of Global Accretion Disks with Vertical Ma…Saturation and thermalization of the magnetorotational instability: recurrent channel flows and reconnectionsSaturation and thermalization of the magnetorotational instability: recurrent …Molecular evolution in collapsing prestellar coresDisk Winds Driven by Magnetorotational Instability and Dispersal of Proto-Planetary DisksDisk Winds Driven by Magnetorotational Instability and Dispersal of Proto-Pla…A Detailed Study of the Molecular and Atomic Gas Toward the {gamma}-ray SNR RX J1713.7-3946: Spatial TeV {gamma}-ray and ISM Gas CorrespondenceA Detailed Study of the Molecular and Atomic Gas Toward the {gamma}-ray …Molecular cloud formation in shock-compressed layersTurbulence and Magnetic Field Amplification in Supernova Remnants: Interactions Between A Strong Shock Wave and Multi-Phase Interstellar MediumTurbulence and Magnetic Field Amplification in Supernova Remnants: Interac…An origin of supersonic motions in interstellar cloudsAngular momentum transport by MHD turbulence in accretion disks: Gas pressure dependence of the saturation level of the magnetorotational instabilityAngular momentum transport by MHD turbulence in accretion disks: Gas pre…Toward Understanding the Cosmic-ray Acceleration at Young Supernova Remnants Interacting with Interstellar Clouds: Possible Applications to RX J1713.7-3946Toward Understanding the Cosmic-ray Acceleration at Young Supernova Rem…2000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average200020052010201520202025050100150200250300