Publicaciones

Esta sección ofrece el acceso a la base de datos de Publicaciones que recopila los artículos del IAC publicados en revistas científicas. Por favor, pulsa la flecha del menú para ver todas las opciones de búsqueda y de ordenación de resultados; autor, revista, año, etc..

Además ofrece acceso al  repositorio de preprints del IAC: https://research.iac.es/preprints/l

  • On the Source of Propagating Slow Magnetoacoustic Waves in Sunspots
    Recent high-resolution observations of sunspot oscillations using simultaneously operated ground- and space-based telescopes reveal the intrinsic connection between different layers of the solar atmosphere. However, it is not clear whether these oscillations are externally driven or generated in situ. We address this question by using observations
    Krishna Prasad, S. et al.

    Fecha de publicación:

    10
    2015
    Número de citas
    55
  • New generation Stokes inversion codes
    We utilize the concept of sparsity or compressibility to develop an new generation of inversion codes for the Stokes parameters. The inversion code uses numerical optimization techniques based on the idea of proximal algorithms to impose sparsity. In so doing, we allow to exploit the presence of spatial correlation on the maps of physical
    Asensio, A. et al.

    Fecha de publicación:

    10
    2015
    Número de citas
    0
  • Molecular hydrogen abundances of galaxies in the EAGLE simulations
    We investigate the abundance of galactic molecular hydrogen (H2) in the `Evolution and Assembly of GaLaxies and their Environments' (EAGLE) cosmological hydrodynamic simulations. We assign H2 masses to gas particles in the simulations in post-processing using two different prescriptions that depend on the local dust-to-gas ratio and the
    Lagos, C. P. et al.

    Fecha de publicación:

    10
    2015
    Número de citas
    211
  • Model Comparison for the Density Structure across Solar Coronal Waveguides
    The spatial variation of physical quantities, such as the mass density, across solar atmospheric waveguides governs the timescales and spatial scales for wave damping and energy dissipation. The direct measurement of the spatial distribution of density, however, is difficult, and indirect seismology inversion methods have been suggested as an
    Arregui, I. et al.

    Fecha de publicación:

    10
    2015
    Número de citas
    24
  • MEASUREMENT OF THE COSMIC RAYS BORON-TO-CARBON RATIO WITH AMS-02
    Desde el descubrimiento de los rayos cósmicos (RC) por Victor Hess en 1912, su estudio ha supuesto una forma complementaria a los aceleradores de partículas para buscar nuevas respuestas al modelo estándar de la física de partículas. Esta radiación que incide sobre la Tierra desde el espacio exterior puede revelar indicios de la aniquilación de
    Rosa Clavero Jiménez

    Fecha de publicación:

    10
    2015
  • LINEAR POLARIZATION MEASUREMENTS OF COOL ATMOSPHERES
    Very low-mass stars, brown dwarfs, and giant planets with effective temperatures < 2700 K (or spectral types cooler than M7) are usually referred to as ultra-cool dwarfs. Their low atmospheric temperatures and high pressures favor the appearance of condensates, which may draw together to form cloud-like structures in their atmospheres. According to
    Paulo Alberto Miles Páez

    Fecha de publicación:

    10
    2015