Astrofísicas: Corona solar

  • Publicación
    Exploring the Magnetic and Thermal Evolution of a Coronal Jet
    Coronal jets are the captivating eruptions that are often found in the solar atmosphere and primarily formed due to magnetic reconnection. Despite their short...
  • Publicación
    Fast-to-Alfvén Mode Conversion and Ambipolar Heating in Structured Media. II. Numerical Simulation
    This paper studies the effectiveness of production of Alfvén waves in the solar atmosphere through the processes of mode conversion, taking into account several...
  • Publicación
    First Metis Detection of the Helium D<SUB>3</SUB> Line Polarization in a Large Eruptive Prominence
    Metis on board Solar Orbiter is the space coronagraph developed by an Italian-German-Czech consortium. It is capable of observing solar corona and various...
  • Charla
    Flares: highly energetic explosions on the Sun
    Flares are among the most energetic magnetic solar phenomena. They are often accompanied by ejections of charged particles, which have a direct influence on the...
  • Noticia
    JEFFREY R. KUHN: “A lo largo de nuestra propia vida, una mañana nos despertaremos con la noticia de que hemos descubierto vida”
    El Sol ya no es la piedra al rojo vivo que describiera Anaxágoras. Imaginamos un infierno en su interior y reconocemos la presencia en su superficie de manchas...
  • Publicación
    La mission SoHO vers un nouveau Soleil?
    Not Available
  • Publicación
    Large Ion-neutral Drift Velocities and Plasma Heating in Partially Ionized Coronal Rain Blobs
    In this paper we present a numerical study of the dynamics of partially ionized coronal rain blobs. We use a two-fluid model to perform a high-resolution 2D...
  • Publicación
    Large-amplitude Prominence Oscillations following Impact by a Coronal Jet
    Observational evidence shows that coronal jets can hit prominences and set them in motion. The impact leads to large-amplitude oscillations (LAOs) in the...
  • 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...