The linear polarization signals produced by scattering processes in strong resonance lines are rich in information on the magnetic and thermal structure of the...
-
PublicaciónThe transfer of resonance line polarization with partial frequency redistribution and J-state interference. Theoretical approach and numerical methods
-
PublicaciónThe Transfer of Resonance Line Polarization with Partial Frequency Redistribution in the General Hanle–Zeeman Regime
The spectral line polarization encodes a wealth of information about the thermal and magnetic properties of the solar atmosphere. Modeling the Stokes profiles...
-
PublicaciónThe use of iteration factors for temperature correction in a stellar atmosphere when convective transport is present
In a previous work (Paper I of this series), we presented a procedure for computing the temperature distribution in a stellar atmosphere under the constraint of...
-
PublicaciónThe 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...
-
PublicaciónThe 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...
-
PublicaciónTheoretical formulation of Doppler redistribution in scattering polarization within the framework of the velocity-space density matrix formalism
Within the framework of the density matrix theory for the generation and transfer of polarized radiation, velocity density matrix correlations represent an...
-
PublicaciónThree-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...
-
PublicaciónThree-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...
-
PublicaciónThree-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...