Astrophysical: Magnetic fields

  • Publication
    The uncertainty of magnetic fields in 3D non-local thermodynamic equilibrium inversions
    We describe our approach to solving the problem of ensuring the solenoidality of the magnetic field vector in 3D inversions, as well as the estimation of the...
  • Publication
    The usefulness of analytic response functions
    Aims:We introduce analytical response functions and their main properties as an important diagnostic tool that help understand Stokes profile formation physics...
  • Publication
    The Zeeman Effect in the G Band
    We investigate the possibility of measuring magnetic field strength in G-band bright points through the analysis of Zeeman polarization in molecular CH lines...
  • Publication
    The Zigzag Path of Buoyant Magnetic Tubes and the Generation of Vorticity along Their Periphery
    We study the generation of vorticity in the magnetic boundary layer of buoyant magnetic tubes and its consequences for the trajectory of magnetic structures...
  • Publication
    THEMIS observations of the Hanle effect in C_2 lines.
    Analysis of the Hanle effect in solar molecular lines allows us to obtain empirical information on unresolved, tangled magnetic fields at subresolution scales...
  • Publication
    THEMIS: the 2006-2012 perspective. and beyond
    Imaging of the solar surface from ground based telescopes has achieved to be diffraction limited almost ten years ago, while diffraction-limited...
  • Publication
    Theoretical Modeling of Propagation of Magnetoacoustic Waves in Magnetic Regions Below Sunspots
    We use two-dimensional numerical simulations and eikonal approximation to study properties of magnetohydrodynamic (MHD) waves traveling below the solar surface...
  • Publication
    Theory and Modeling of the Zeeman and Paschen-Back Effects in Molecular Lines
    This paper describes a very general approach to the calculation of the Zeeman splitting effect produced by an external magnetic field on the rotational levels...
  • Publication
    Thermal properties of magnetic flux tubes. I. Solution of the diffusion problem
    The heat flow and temperature structure within and surrounding a magnetic flux tube stored in mechanical equilibrium in a stellar convection zone are considered...