Publication data of Ryu, Dongsu: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion1990199520002005201020152020202502000400060008000
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications199019952000200520102015202020250408012016020003691215
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion199019952000200520102015202020250102030405060
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestShock acceleration efficiency in radio relicsMagnetic Fields, Relativistic Particles, and Shock Waves in Cluster OutskirtsTurbulence and Vorticity in Galaxy Clusters Generated by Structure FormationCosmological Shock Waves in the Large Scale Structure of the Universe: Non-gravitational EffectsCosmological Shock Waves in the Large Scale Structure of the Universe: Non-…Numerical simulations of standing shocks in accretion flows around black holes: a comparative studyNumerical simulations of standing shocks in accretion flows around black hol…Zero energy rotating accretion flows near a black holeCosmic ray protons accelerated at cosmological shocks and their impact on groups and clusters of galaxiesCosmic ray protons accelerated at cosmological shocks and their impact on …Molecular cloud evolution. 1. molecular cloud and thin cnm sheet formationCluster accretion shocks as possible acceleration sites for ultrahigh-energy protons below the Greisen cutoffCluster accretion shocks as possible acceleration sites for ultrahigh-energy pr…Magnetic fields in the Large-Scale Structure of the UniverseDiffusive Shock Acceleration Simulations of Radio RelicsCosmic ray electrons in groups and clusters of galaxies: primary and secondary populations from a numerical cosmological simulationCosmic ray electrons in groups and clusters of galaxies: primary and seconda…A Cosmological hydrodynamic code based on the total variation diminishing schemeA Cosmological hydrodynamic code based on the total variation diminishing …Cosmic magnetic fields in large scale filaments and sheetsThe First Magnetic FieldsProperties of cosmic shock waves in large scale structure formationThe Protogalactic origin for cosmic magnetic fieldsTurbulence and Magnetic Fields in the Large Scale Structure of the UniverseCosmological shock waves and their role in the large scale structure of the universeCosmological shock waves and their role in the large scale structure of the u…1990199520002005201020152020202502000400060008000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)Shock acceleration efficiency in radio relicsMagnetic Fields, Relativistic Particles, and Shock Waves in Cluster OutskirtsTurbulence and Vorticity in Galaxy Clusters Generated by Structure FormationCosmological Shock Waves in the Large Scale Structure of the Universe: Non-gravitational EffectsCosmological Shock Waves in the Large Scale Structure of the Universe: Non-…Numerical simulations of standing shocks in accretion flows around black holes: a comparative studyNumerical simulations of standing shocks in accretion flows around black hol…Zero energy rotating accretion flows near a black holeCosmic ray protons accelerated at cosmological shocks and their impact on groups and clusters of galaxiesCosmic ray protons accelerated at cosmological shocks and their impact on …Molecular cloud evolution. 1. molecular cloud and thin cnm sheet formationCluster accretion shocks as possible acceleration sites for ultrahigh-energy protons below the Greisen cutoffCluster accretion shocks as possible acceleration sites for ultrahigh-energy pr…Magnetic fields in the Large-Scale Structure of the UniverseDiffusive Shock Acceleration Simulations of Radio RelicsCosmic ray electrons in groups and clusters of galaxies: primary and secondary populations from a numerical cosmological simulationCosmic ray electrons in groups and clusters of galaxies: primary and seconda…A Cosmological hydrodynamic code based on the total variation diminishing schemeA Cosmological hydrodynamic code based on the total variation diminishing …Cosmic magnetic fields in large scale filaments and sheetsThe First Magnetic FieldsProperties of cosmic shock waves in large scale structure formationThe Protogalactic origin for cosmic magnetic fieldsTurbulence and Magnetic Fields in the Large Scale Structure of the UniverseCosmological shock waves and their role in the large scale structure of the universeCosmological shock waves and their role in the large scale structure of the u…199019952000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average199019952000200520102015202020250100200300400500