Formal Solutions for Polarized Radiative Transfer. I. The DELO Family
arXiv:1709.01274 · doi:10.3847/1538-4357/aa671d
Abstract
The discussion regarding the numerical integration of the polarized radiative transfer equation is still open and the comparison between the different numerical schemes proposed by different authors in the past is not fully clear. Aiming at facilitating the comprehension of the advantages and drawbacks of the different formal solvers, this work presents a reference paradigm for their characterization based on the concepts of order of accuracy, stability, and computational cost. Special attention is paid to understand the numerical methods belonging to the Diagonal Element Lambda Operator family, in an attempt to highlight their specificities.
11 pages, 4 figures
Cited by in corpus (13)
- Modeling the scattering polarization of the solar Ca i 4227 Å line with angle-dependent partial frequency redistribution
- Numerical solutions to linear transfer problems of polarized radiation II. Krylov methods and matrix-free implementation
- The chromosphere above a -sunspot in the presence of fan-shaped jets
- The transfer of polarized radiation in resonance lines with partial frequency redistribution, J-state interference, and arbitrary magnetic fields. A radiative transfer code and useful approximations
- Formal Solutions for Polarized Radiative Transfer. II. High-order Methods
- Thermal Emission and Scattering by Aligned Grains: Plane-Parallel Model and Application to Multiwavelength Polarization of the HL Tau Disk
- Covariant polarized radiative transfer on cosmological scales for investigating large-scale magnetic field structures
- Numerical solutions to linear transfer problems of polarized radiation I. Algebraic formulation and stationary iterative methods
- Discontinuities in numerical radiative transfer
- A New Fast Monte Carlo Code for Solving Radiative Transfer Equations based on Neumann Solution
- Assessment of the CRD approximation for the observer's frame RIII redistribution matrix
- Diagnostic potential of wavelength-integrated scattering polarisation signals of the solar He II Ly-alpha line
- A numerical approach for modelling the polarisation signals of strong resonance lines with partial frequency redistribution. Numerical applications to two-term atoms and plane-parallel atmospheres