Publication data of Stein, Robert: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion1970198019902000201020200500100015002000
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications1970198019902000201020200153045607501.534.567.5
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion1970198019902000201020200510152025
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestThe response of a turbulent accretion disc to an imposed epicyclic shearing motionThe response of a turbulent accretion disc to an imposed epicyclic shearing …Solar oscillations and convection: I. formalism for radial oscillationsNumerical 3D constraints on convective eddy time-correlations: Consequences for stochastic excitation of solar p modesNumerical 3D constraints on convective eddy time-correlations: Consequenc…The effects of numerical resolution on hydrodynamical surface convection simulations and spectral line formationThe effects of numerical resolution on hydrodynamical surface convection si…Dynamics of magnetic flux elements in the solar photosphereMultifrequency Observations of the Candidate Neutrino-emitting Blazar BZB J0955+3551Multifrequency Observations of the Candidate Neutrino-emitting Blazar BZB J…The first systematically identified repeating partial tidal disruption eventConvective contributions to the frequencies of solar oscillationsExcitation of solar-like oscillations across the HR diagramLine formation in solar granulation. 2. The photospheric fe abundanceDynamic hydrogen ionizationObservational manifestations of solar magneto-convection - Center-to-limb variationObservational manifestations of solar magneto-convection - Center-to-limb va…Solar oscillations and convection. 2. Excitation of radial oscillations3-D hydrodynamical model atmospheres of metal-poor stars: evidence for a low primordial li abundance3-D hydrodynamical model atmospheres of metal-poor stars: evidence for a l…Does a Non-Magnetic Solar Chromosphere Exist?Patterns in the Multiwavelength Behavior of Candidate Neutrino BlazarsWaves in the Magnetized Solar Atmosphere. II. Waves from Localized Sources in Magnetic Flux ConcentrationsWaves in the Magnetized Solar Atmosphere. II. Waves from Localized Sources…Line formation in solar granulation: I. fe line shapes, shifts and asymmetriesDynamo-generated Turbulence and Large-Scale Magnetic Fields in a Keplerian Shear FlowDynamo-generated Turbulence and Large-Scale Magnetic Fields in a Kepleria…1970198019902000201020200500100015002000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)The response of a turbulent accretion disc to an imposed epicyclic shearing motionThe response of a turbulent accretion disc to an imposed epicyclic shearing …Solar oscillations and convection: I. formalism for radial oscillationsNumerical 3D constraints on convective eddy time-correlations: Consequences for stochastic excitation of solar p modesNumerical 3D constraints on convective eddy time-correlations: Consequenc…The effects of numerical resolution on hydrodynamical surface convection simulations and spectral line formationThe effects of numerical resolution on hydrodynamical surface convection si…Dynamics of magnetic flux elements in the solar photosphereMultifrequency Observations of the Candidate Neutrino-emitting Blazar BZB J0955+3551Multifrequency Observations of the Candidate Neutrino-emitting Blazar BZB J…The first systematically identified repeating partial tidal disruption eventConvective contributions to the frequencies of solar oscillationsExcitation of solar-like oscillations across the HR diagramLine formation in solar granulation. 2. The photospheric fe abundanceDynamic hydrogen ionizationObservational manifestations of solar magneto-convection - Center-to-limb variationObservational manifestations of solar magneto-convection - Center-to-limb va…Solar oscillations and convection. 2. Excitation of radial oscillations3-D hydrodynamical model atmospheres of metal-poor stars: evidence for a low primordial li abundance3-D hydrodynamical model atmospheres of metal-poor stars: evidence for a l…Does a Non-Magnetic Solar Chromosphere Exist?Patterns in the Multiwavelength Behavior of Candidate Neutrino BlazarsWaves in the Magnetized Solar Atmosphere. II. Waves from Localized Sources in Magnetic Flux ConcentrationsWaves in the Magnetized Solar Atmosphere. II. Waves from Localized Sources…Line formation in solar granulation: I. fe line shapes, shifts and asymmetriesDynamo-generated Turbulence and Large-Scale Magnetic Fields in a Keplerian Shear FlowDynamo-generated Turbulence and Large-Scale Magnetic Fields in a Kepleria…1970198019902000201020200255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average1970198019902000201020200255075100125150175