Astrofísicas: Corona solar

  • Publicación
    Magnetic Fields beneath Active Region Coronal Loops
    We examine the hypothesis that multipolar magnetic fields advected by photospheric granules can contribute to heating the active chromosphere and corona. On...
  • Charla
    Magnetically driven jets in the solar Atmosphere
    Recent observations of the solar atmosphere have provided new insights concerning medium-sized jet phenomena taking place in the solar corona. These jets are...
  • Publicación
    P-CORONA: A New Tool for Calculating the Intensity and Polarization of Coronal Lines in 3D Models of the Solar Corona
    The critical need to study the magnetic field in the solar corona is highlighted by recent observational facilities, such as the Daniel K. Inouye Solar...
  • Publicación
    Polarization of the Lyα Lines of H I and He II as a Tool for Exploring the Solar Corona
    The near-Earth space weather is driven by the quick release of magnetic free energy in the solar corona. Probing this extremely hot and rarified region of the...
  • Publicación
    Polarization of the Lyα Lines of H I and He II as a Tool for Exploring the Solar Corona
    The near-Earth space weather is driven by the quick release of magnetic free energy in the solar corona. Probing this extremely hot and rarified region of the...
  • Publicación
    Progress in stellar spectral line formation theory; Proceedings of the Advanced Research Workshop, Trieste, Italy, September 4-7, 1984
    Papers on stellar spectral line formation theory are presented. The general topics considered include: frequency redistribution problems in line formation...
  • Publicación
    Solar coronal loop oscillations: theory of resonantly damped oscillations and comparison with observations
    One of the proposed damping mechanisms of coronal transverse loop oscillations in the kink mode is resonant absorption as a result of the spatial variation of...
  • Charla
    Solar-terrestrial relations – combined remote sensing and in-situ data
    The Sun is an active star that influences the Earth as well as the entire solar system. Most dynamic phenomena on the Sun are observed as coronal mass ejections...
  • Publicación
    The Chromosphere Underneath a Coronal Bright Point
    Coronal bright points (CBPs) are sets of small-scale coronal loops, connecting opposite magnetic polarities, primarily characterized by their enhanced extreme...