Publication data of Trampedach, Regner: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion19952000200520102015202020250100200300400500600700
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications19952000200520102015202020250816243240012345
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion199520002005201020152020202502468101214
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestCurrent State of Astrophysical Opacities: A White PaperA Grid of 3D Stellar Atmosphere Models of Solar Metallicity: I. General Properties, Granulation and Atmospheric ExpansionA Grid of 3D Stellar Atmosphere Models of Solar Metallicity: I. General Properti…Three-dimensional surface convection simulations of metal-poor stars -- The effect of scattering on the photospheric temperature stratificationThree-dimensional surface convection simulations of metal-poor stars -- The e…Light bosons and photospheric solutions to the solar abundance problemHow realistic are solar model atmospheres?On the Amplitude of Convective Velocities in the Deep Solar InteriorAbundance Analysis of the Halo Giant HD122563 with Three-Dimensional Model Stellar AtmospheresAbundance Analysis of the Halo Giant HD122563 with Three-Dimensional Mo…A synoptic comparison of the MHD and the OPAL equations of stateRadiative transfer with scattering for domain-decomposed 3D MHD simulations of cool stellar atmospheresRadiative transfer with scattering for domain-decomposed 3D MHD simulatio…The Stagger-grid: A Grid of 3D Stellar Atmosphere Models - I. Methods and General PropertiesThe Stagger-grid: A Grid of 3D Stellar Atmosphere Models - I. Methods and G…The Mass Mixing Length in Convective Stellar EnvelopesThe elemental composition of the Sun I. The intermediate mass elements Na to CaThe elemental composition of the Sun I. The intermediate mass elements Na …Convective contributions to the frequencies of solar oscillationsThe chemical compositions of the extreme halo stars HE0107-5240 and HE1327-2326 inferred from 3D hydrodynamical model atmospheresThe chemical compositions of the extreme halo stars HE0107-5240 and HE1…Excitation of solar-like oscillations across the HR diagramLine formation in solar granulation. 2. The photospheric fe abundance3-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…3D Hydrodynamical Simulations of Surface Convection in Red Giant Stars. Impact on spectral line formation and abundance analysis3D Hydrodynamical Simulations of Surface Convection in Red Giant Stars. Im…Line formation in solar granulation: I. fe line shapes, shifts and asymmetries19952000200520102015202020250100200300400500600700
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)Current State of Astrophysical Opacities: A White PaperA Grid of 3D Stellar Atmosphere Models of Solar Metallicity: I. General Properties, Granulation and Atmospheric ExpansionA Grid of 3D Stellar Atmosphere Models of Solar Metallicity: I. General Properti…Three-dimensional surface convection simulations of metal-poor stars -- The effect of scattering on the photospheric temperature stratificationThree-dimensional surface convection simulations of metal-poor stars -- The e…Light bosons and photospheric solutions to the solar abundance problemHow realistic are solar model atmospheres?On the Amplitude of Convective Velocities in the Deep Solar InteriorAbundance Analysis of the Halo Giant HD122563 with Three-Dimensional Model Stellar AtmospheresAbundance Analysis of the Halo Giant HD122563 with Three-Dimensional Mo…A synoptic comparison of the MHD and the OPAL equations of stateRadiative transfer with scattering for domain-decomposed 3D MHD simulations of cool stellar atmospheresRadiative transfer with scattering for domain-decomposed 3D MHD simulatio…The Stagger-grid: A Grid of 3D Stellar Atmosphere Models - I. Methods and General PropertiesThe Stagger-grid: A Grid of 3D Stellar Atmosphere Models - I. Methods and G…The Mass Mixing Length in Convective Stellar EnvelopesThe elemental composition of the Sun I. The intermediate mass elements Na to CaThe elemental composition of the Sun I. The intermediate mass elements Na …Convective contributions to the frequencies of solar oscillationsThe chemical compositions of the extreme halo stars HE0107-5240 and HE1327-2326 inferred from 3D hydrodynamical model atmospheresThe chemical compositions of the extreme halo stars HE0107-5240 and HE1…Excitation of solar-like oscillations across the HR diagramLine formation in solar granulation. 2. The photospheric fe abundance3-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…3D Hydrodynamical Simulations of Surface Convection in Red Giant Stars. Impact on spectral line formation and abundance analysis3D Hydrodynamical Simulations of Surface Convection in Red Giant Stars. Im…Line formation in solar granulation: I. fe line shapes, shifts and asymmetries19952000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average19952000200520102015202020250255075100125