Publication type: Refereed

  • Publication
    Three-dimensional magnetic field structure of a flux-emerging region in the solar atmosphere
    We analyze high-resolution spectropolarimetric observations of a flux-emerging region (FER) in order to understand its magnetic and kinematic structure. Our...
  • Publication
    Three-dimensional magnetic field topology in a region of solar coronal heating
    Flares and X-ray jets on the Sun arise in active regions where magnetic flux emerges from the solar interior amd interacts with the ambient magnetic field. The...
  • Publication
    Three-dimensional modeling of chromospheric spectral lines in a simulated active region
    Context. Because of the complex physics that governs the formation of chromospheric lines, interpretation of solar chromospheric observations is difficult. The...
  • Publication
    Three-dimensional P-wave velocity structure of Mt. Etna, Italy
    The three-dimensional P-wave velocity structure of Mt. Etna is determined to depths of 15 km by tomographic inversion of first arrival times from local...
  • Publication
    Three-dimensional Plasmoid Evolution in the Solar Atmosphere
    We present clear evidence of the formation of three-dimensional (3D) plasmoids in the current sheet between two magnetic flux systems in a 3D numerical...
  • Publication
    Three-dimensional Propagation of Magnetohydrodynamic Waves in Solar Coronal Arcades
    We numerically investigate the excitation and temporal evolution of oscillations in a two-dimensional coronal arcade by including the three-dimensional...
  • Publication
    Three-dimensional Radiative Transfer Modeling of the Polarization of the Sun's Continuous Spectrum
    Polarized light provides the most reliable source of information at our disposal for diagnosing the physical properties of astrophysical plasmas, including the...
  • Publication
    Three-dimensional Radiative Transfer Simulations of the Scattering Polarization of the Hydrogen Lyα Line in a Magnetohydrodynamic Model of the Chromosphere–Corona Transition Region
    Probing the magnetism of the upper solar chromosphere requires measuring and modeling the scattering polarization produced by anisotropic radiation pumping in...
  • Publication
    Three-dimensional simulations of solar magneto-convection including effects of partial ionization
    In recent decades, REALISTIC three-dimensional radiative-magnetohydrodynamic simulations have become the dominant theoretical tool for understanding the complex...