Astrophysical: Helioseismology

  • Publication
    Helio- and asteroseismology at the dawn of the millennium
    Not Available
  • Publication
    Helioseismic evidence of two solar granulation timescales
    The signature of two different scales of solar granulation in the power spectrum of disk integrated irradiance time series is presented. The fitted timescales...
  • Publication
    Helioseismic holography of simulated sunspots: dependence of the travel time on magnetic field strength and Wilson depression
    Improving methods for determining the subsurface structure of sunspots from their seismic signature requires a better understanding of the interaction of waves...
  • Publication
    Helioseismic Holography of Simulated Sunspots: Magnetic and Thermal Contributions to Travel Times
    Wave propagation through sunspots involves conversion between waves of acoustic and magnetic character. In addition, the thermal structure of sunspots is very...
  • Publication
    Helioseismology program for the PICARD satellite
    The PICARD mission is a CNES micro-satellite to be launched in 2009. Its goal is to better understand the Sun and the potential impact of its activity on earth...
  • Talk
    Heliosismología: la visión pitagórica de la astrofísica.
    Durante los últimos 45 años, el grupo de Sismología Solar (y Estelar y Búsqueda de Exoplanetas) del Instituto de Astrofísica de Canarias, ha estado observando...
  • News
    Hot stars are plagued by giant magnetic spots
    An international team of astronomers, in which the researcher from the Instituto de Astrofísica de Canarias and the Universidad de La Laguna David Jones...
  • Publication
    Improved detection of far-side solar active regions using deep learning
    Context. The analysis of waves on the visible side of the Sun allows the detection of active regions on the far side through local helioseismology techniques...
  • Publication
    Influence of Low-Degree High-Order p-Mode Splittings on the Solar Rotation Profile
    The solar rotation profile is well constrained down to about 0.25 R &sun; thanks to the study of acoustic modes. Since the radius of the inner turning point of...