Astrofísicas: Métodos

  • Publicación
    Thermodynamic fluctuations in solar photospheric three-dimensional convection simulations and observations
    Not Available
  • Publicación
    Thermodynamic fluctuations in solar photospheric three-dimensional convection simulations and observations
    Context. Numerical three-dimensional (3D) radiative (magneto-)hydrodynamical [(M)HD] simulations of solar convection are nowadays used to understand the...
  • Publicación
    Thin coronal jets and plasmoid-mediated reconnection: Insights from Solar Orbiter observations and Bifrost simulations
    Context. Coronal jets are ubiquitous, collimated million-degree ejections that contribute to the energy and mass supply of the upper solar atmosphere and the...
  • Publicación
    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...
  • Publicación
    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...
  • Publicación
    Three-dimensional Spectral Classification of Low-Metallicity Stars Using Artificial Neural Networks
    We explore the application of artificial neural networks (ANNs) for the estimation of atmospheric parameters (Teff, logg, and [Fe/H]) for Galactic F- and G-type...
  • Publicación
    Three-dimensional structure of a sunspot light bridge
    Context. Active regions are the most prominent manifestations of solar magnetic fields; their generation and dissipation are fundamental problems in solar...
  • Publicación
    Through thick and thin: Structure of the Galactic thick disc from extragalactic surveys
    Context. We aim to understand the accretion history of the Milky Way by exploring the vertical and radial properties of the Galactic thick disc. Aims: We study...
  • Publicación
    Through Thick and Thin—H I Absorption in Cosmological Simulations
    We investigate the column density distribution function of neutral hydrogen at redshift z = 3 using a cosmological simulation of galaxy formation from the...