Publication data of Sur, Sharanya: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion20062008201020122014201620182020202220240100200300400500600
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications20062008201020122014201620182020202220240510152025012345
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion20062008201020122014201620182020202220240246810
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestThe generation of strong magnetic fields during the formation of the first starsThe generation of strong magnetic fields during the formation of the first sta…The formation of supermassive black holes in the first galaxiesGeneration of strong magnetic fields via the small-scale dynamo during the formation of the first starsGeneration of strong magnetic fields via the small-scale dynamo during the f…Magnetic fields during primordial star formationModeling the Survival of Population III Stars to the Present DayProperties of Polarized Synchrotron Emission from Fluctuation Dynamo Action—II. Effects of Turbulence Driving in the ICM and Beam SmoothingProperties of Polarized Synchrotron Emission from Fluctuation Dynamo Actio…The role of the Yoshizawa effect in the Archontis dynamoThe impact of thermodynamics on gravitational collapse: filament formation and magnetic field amplificationThe impact of thermodynamics on gravitational collapse: filament formation …Properties of polarized synchrotron emission from fluctuation-dynamo action – I. Application to galaxy clustersProperties of polarized synchrotron emission from fluctuation-dynamo action …Kinematic alpha effect in isotropic turbulence simulationsGalaxy Outflows Without SupernovaeExploring diffuse radio emission in galaxy clusters and groups with uGMRT and SKAExploring diffuse radio emission in galaxy clusters and groups with uGMRT an…Decaying turbulence and magnetic fields in galaxy clustersKinetic and magnetic alpha effects in nonlinear dynamo theoryGalactic dynamos supported by magnetic helicity fluxesMagnetic field amplification during gravitational collapse - Influence of initial conditions on dynamo evolution and saturationMagnetic field amplification during gravitational collapse - Influence of initial …Small-scale dynamo action during the formation of the first stars and galaxies. I. The ideal MHD limitSmall-scale dynamo action during the formation of the first stars and galaxie…The generation of strong magnetic fields during the formation of the first starsThe generation of strong magnetic fields during the formation of the first sta…A new Jeans resolution criterion for (M)HD simulations of self-gravitating gas: Application to magnetic field amplification by gravity-driven turbulenceA new Jeans resolution criterion for (M)HD simulations of self-gravitating gas: …20062008201020122014201620182020202220240100200300400500600
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)The generation of strong magnetic fields during the formation of the first starsThe generation of strong magnetic fields during the formation of the first sta…The formation of supermassive black holes in the first galaxiesGeneration of strong magnetic fields via the small-scale dynamo during the formation of the first starsGeneration of strong magnetic fields via the small-scale dynamo during the f…Magnetic fields during primordial star formationModeling the Survival of Population III Stars to the Present DayProperties of Polarized Synchrotron Emission from Fluctuation Dynamo Action—II. Effects of Turbulence Driving in the ICM and Beam SmoothingProperties of Polarized Synchrotron Emission from Fluctuation Dynamo Actio…The role of the Yoshizawa effect in the Archontis dynamoThe impact of thermodynamics on gravitational collapse: filament formation and magnetic field amplificationThe impact of thermodynamics on gravitational collapse: filament formation …Properties of polarized synchrotron emission from fluctuation-dynamo action – I. Application to galaxy clustersProperties of polarized synchrotron emission from fluctuation-dynamo action …Kinematic alpha effect in isotropic turbulence simulationsGalaxy Outflows Without SupernovaeExploring diffuse radio emission in galaxy clusters and groups with uGMRT and SKAExploring diffuse radio emission in galaxy clusters and groups with uGMRT an…Decaying turbulence and magnetic fields in galaxy clustersKinetic and magnetic alpha effects in nonlinear dynamo theoryGalactic dynamos supported by magnetic helicity fluxesMagnetic field amplification during gravitational collapse - Influence of initial conditions on dynamo evolution and saturationMagnetic field amplification during gravitational collapse - Influence of initial …Small-scale dynamo action during the formation of the first stars and galaxies. I. The ideal MHD limitSmall-scale dynamo action during the formation of the first stars and galaxie…The generation of strong magnetic fields during the formation of the first starsThe generation of strong magnetic fields during the formation of the first sta…A new Jeans resolution criterion for (M)HD simulations of self-gravitating gas: Application to magnetic field amplification by gravity-driven turbulenceA new Jeans resolution criterion for (M)HD simulations of self-gravitating gas: …20062008201020122014201620182020202220240255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average2006200820102012201420162018202020222024020406080100