Esta web estará fuera de servicio por mantenimiento el martes 28 de abril de 13:00 a 17:00 aprox.

Astrofísicas: Campos magnéticos

  • Publicación
    Radio-size estimates of SN 1993J
    Supernova 1993J (SN 1993J) in M81, now classified as Type IIb, is a strongly emitting radio supernova whose size can be resolved and whose growth can be...
  • Publicación
    Rapid timing studies of black hole binaries in Optical and X-rays: correlated and non-linear variability
    In a fast multi-wavelength timing study of black hole X-ray binaries (BHBs), we have discovered correlated optical and X-ray variability in the low/hard state...
  • Publicación
    Rayleigh-Taylor instabilities with sheared magnetic fields in partially ionised plasmas
    Aims: In the present study we investigate the nature of the magnetic Rayleigh-Taylor instability appearing at a tangential discontinuity in a partially ionised...
  • Publicación
    Rayleigh-Taylor instability in partially ionized prominence plasma
    We study Rayleigh-Taylor instability (RTI) at the coronal-prominence boundary by means of 2.5D numerical simulations in a single-fluid MHD approach including a...
  • Publicación
    Rayleigh-Taylor instability in prominences from numerical simulations including partial ionization effects
    We study the Rayleigh-Taylor instability (RTI) at a prominence-corona transition region in a non-linear regime. Our aim is to understand how the presence of...
  • Publicación
    Recent Applications of Bayesian Methods to the Solar Corona
    Solar coronal seismology is based on the remote diagnostics of physical conditions in the corona of the Sun by comparison between model predictions and...
  • Publicación
    Recovering coherent flow structures in active regions using machine learning
    Analysing high-resolution solar atmospheric observations requires robust techniques to recover plasma flow features across different scales, especially in...
  • Publicación
    Relation between photospheric magnetic field and chromospheric emission
    Aims: We investigate the relationship between the photospheric magnetic field and the emission of the mid chromosphere of the Sun. Methods: We simultaneously...
  • Publicación
    Relationships between magnetic foot points and G-band bright structures
    Aims:Magnetic elements are thought to be described by flux tube models, and are well reproduced by MHD simulations. However, these simulations are only...