Tipo de publicación: Sin árbitro

  • Publicación
    Inferring stellar population properties from HST+JWST photometry using Normalizing Flows
    Spectral energy distributions (SEDs) encode information about the stellar populations within galaxies. By investigating the properties of these stars, such as...
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    Inflation and the CMB
    Not Available
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    Influence of Coronal EUV Irradiance on the Stokes Profiles of the He I 10830 Å Multiplet
    One of the most useful spectral windows for spectropolarimetric investigations of the solar chromosphere is the one provided by the spectral lines of the He I...
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    Influence of longitudinal structure in the fast modes of prominence threads
    Recent high-resolution observations have pointed out that prominences are made of small threads (also named fibrils) piled up to form the body of the prominence...
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    Influence of the magnetic cycle on the excitation of solar-like acoustic modes
    The Sun's convective envelope generates, by dynamo effect, a surface magnetic field whose strength evolves on an 11-year cycle, with a change in polarity at the...
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    Influence of the Paschen-Back effect on the results of polarimetric inversions of the He I 10830 Å triplet
    The He I triplet at 10830 Å has a great potential for determining the magnetic field vector in the upper chromosphere. The triplet is Zeeman sensitive (Landé...
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    Influence of Unresolved Optically-Thin Irregularities on Quiet Sun Magnetic Field Determinations
    Observations and theory both point out that the magnetic photosphere is not smooth but irregular at optically-thin scales. The relevance of these irregularities...
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    Influence of unresolved optically-thin irregularities on quiet Sun magnetic field determinations.
    Not Available
  • Publicación
    INFRA-RED SPACE OBSERVATORY Observations of the Pleiades Brown Dwarfs Teide 1 and Calar 3
    Not Available