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..

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  • Observational signatures of the simulated solar photosphere
    Most of the visible light coming from the Sun originates in the solar photosphere. Numerical simulations are a common tool to study the solar atmosphere starting from the basic laws of physics and few additional assumptions. This thesis presents results of three-dimensional radiative magnetohydrodynamic simulations of the quiet-sun, plage and
    Vitas, N.

    Fecha de publicación:

    1
    2011
    Número de citas
    4
  • Numerical simulations of conversion to Alfvén waves in solar active regions
    We study the coupling of magneto-acoustic waves to Alvén waves using 2.5D numerical simulations. In our experiment, a fast magnetoacoustic wave of a given frequency and wavenumber is generated below the surface. The magnetic field in the domain is assumed homogeneous and inclined. The efficiency of the conversion to Alfvén waves near the layer of
    Khomenko, E. et al.

    Fecha de publicación:

    1
    2011
    Número de citas
    24
  • New Results from the Project MASGOMAS: Near-IR Study of the Stellar Population of Sh2-152
    We present a near-IR and optical spectrophotometric characterization of the stellar population of Sh2-152, as part of our MASGOMAS project. Using new broad band photometry (J, H and K_S) for the cluster and a control field, we have constructed CMD in order to select OB-candidates for H and K spectroscopy. Also, we have obtained the cluster mass
    Ramírez Alegría, Sebastián et al.

    Fecha de publicación:

    1
    2011
    Número de citas
    0
  • New insights on the solar core
    Since the detection of the asymptotic properties of the dipole gravity modes in the Sun, the quest to find individual gravity modes has continued. An extensive and deeper analysis of 14 years of continuous GOLF/SoHO observational data, unveils the presence of a pattern of peaks that could be interpreted as individual dipole gravity modes in the
    García, R. A. et al.

    Fecha de publicación:

    1
    2011
    Número de citas
    17
  • Modelling the radio pulses of an ultracool dwarf
    Context. Recently, unanticipated magnetic activity in ultracool dwarfs (UCDs, spectral classes later than M7) has emerged from a number of radio observations. The highly (up to 100%) circularly polarized nature and high brightness temperature of the emission have been interpreted as requiring an effective amplification mechanism of the high
    Yu, S. et al.

    Fecha de publicación:

    1
    2011
    Número de citas
    27
  • Mode visibilities in radial velocity and intensity Sun-as-a-star helioseismic measurements
    We analyze more than 5000 days of Sun-as-a-star radial velocity GOLF and intensity VIRGO observations to measure the visibilities of the I = 0, 1, 2, and 3 modes and the m-amplitude ratios of the I = 2 and 3 modes in the solar acoustic spectrum. We provide observational values that we compare to theoretical predictions.
    Salabert, D. et al.

    Fecha de publicación:

    1
    2011
    Número de citas
    1