Publication data of Socas-Navarro, Hector: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion19952000200520102015202020250100200300400500
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications1995200020052010201520202025010203040500246810
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion199520002005201020152020202502468101214
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestShocks in the quiet solar photosphere: A Rather common occurrenceSpectropolarimetric inversions of the Ca II 8498 A and 8542 A lines in the quiet SunSpectropolarimetric inversions of the Ca II 8498 A and 8542 A lines in the qu…Spectro-polarimetric observations and non-lte modeling of ellerman bombsA High-Resolution Three-Dimensional Model of the Solar Photosphere Derived from Hinode ObservationsA High-Resolution Three-Dimensional Model of the Solar Photosphere Derived …Strategies for spectral profile inversion using artificial neural networksAre electric currents heating the magnetic chromosphere?Physical properties of spicules from simultaneous spectro-polarimetric observations of He I and Ca II linesPhysical properties of spicules from simultaneous spectro-polarimetric observ…The intrinsic dimensionality of spectro-polarimetric dataSpectral Line Selection for HMI: A Comparison of FeI 6173 and NiI 6768Signatures of incomplete Paschen-Back splitting in the polarization profiles of the He I 10830 A multipletSignatures of incomplete Paschen-Back splitting in the polarization profiles of…A new approach to the solar oxygen abundance problemSpinor: visible and infrared spectro-polarimetry at the national solar observatorySpinor: visible and infrared spectro-polarimetry at the national solar observat…On the fine structure of the sunspot penumbrae. 3. the vertical extension of penumbral filamentsOn the fine structure of the sunspot penumbrae. 3. the vertical extension of …Can a negative-mass cosmology explain dark matter and dark energy?The three-dimensional structure of a sunspot magnetic fieldObservational evidence for small-scale mixture of weak and strong fields in the quiet SunObservational evidence for small-scale mixture of weak and strong fields in t…VFISV: Very Fast Inversion of the Stokes Vector for the Helioseismic and Magnetic ImagerVFISV: Very Fast Inversion of the Stokes Vector for the Helioseismic and Magn…Magnetic properties of photospheric regions having very low magnetic fluxEmergence of Small-Scale Magnetic Loops in the Quiet Sun Internetwork19952000200520102015202020250100200300400500
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)Shocks in the quiet solar photosphere: A Rather common occurrenceSpectropolarimetric inversions of the Ca II 8498 A and 8542 A lines in the quiet SunSpectropolarimetric inversions of the Ca II 8498 A and 8542 A lines in the qu…Spectro-polarimetric observations and non-lte modeling of ellerman bombsA High-Resolution Three-Dimensional Model of the Solar Photosphere Derived from Hinode ObservationsA High-Resolution Three-Dimensional Model of the Solar Photosphere Derived …Strategies for spectral profile inversion using artificial neural networksAre electric currents heating the magnetic chromosphere?Physical properties of spicules from simultaneous spectro-polarimetric observations of He I and Ca II linesPhysical properties of spicules from simultaneous spectro-polarimetric observ…The intrinsic dimensionality of spectro-polarimetric dataSpectral Line Selection for HMI: A Comparison of FeI 6173 and NiI 6768Signatures of incomplete Paschen-Back splitting in the polarization profiles of the He I 10830 A multipletSignatures of incomplete Paschen-Back splitting in the polarization profiles of…A new approach to the solar oxygen abundance problemSpinor: visible and infrared spectro-polarimetry at the national solar observatorySpinor: visible and infrared spectro-polarimetry at the national solar observat…On the fine structure of the sunspot penumbrae. 3. the vertical extension of penumbral filamentsOn the fine structure of the sunspot penumbrae. 3. the vertical extension of …Can a negative-mass cosmology explain dark matter and dark energy?The three-dimensional structure of a sunspot magnetic fieldObservational evidence for small-scale mixture of weak and strong fields in the quiet SunObservational evidence for small-scale mixture of weak and strong fields in t…VFISV: Very Fast Inversion of the Stokes Vector for the Helioseismic and Magnetic ImagerVFISV: Very Fast Inversion of the Stokes Vector for the Helioseismic and Magn…Magnetic properties of photospheric regions having very low magnetic fluxEmergence of Small-Scale Magnetic Loops in the Quiet Sun Internetwork19952000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average1995200020052010201520202025020406080