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Title: Formal Solutions for Polarized Radiative Transfer. II. High-order Methods

Abstract

When integrating the radiative transfer equation for polarized light, the necessity of high-order numerical methods is well known. In fact, well-performing high-order formal solvers enable higher accuracy and the use of coarser spatial grids. Aiming to provide a clear comparison between formal solvers, this work presents different high-order numerical schemes and applies the systematic analysis proposed by Janett et al., emphasizing their advantages and drawbacks in terms of order of accuracy, stability, and computational cost.

Authors:
; ;  [1]
  1. Istituto Ricerche Solari Locarno (IRSOL), 6605 Locarno-Monti (Switzerland)
Publication Date:
OSTI Identifier:
22663242
Resource Type:
Journal Article
Journal Name:
Astrophysical Journal
Additional Journal Information:
Journal Volume: 845; Journal Issue: 2; Other Information: Country of input: International Atomic Energy Agency (IAEA); Journal ID: ISSN 0004-637X
Country of Publication:
United States
Language:
English
Subject:
79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; ACCURACY; COMPARATIVE EVALUATIONS; EQUATIONS; POLARIZATION; RADIANT HEAT TRANSFER; STABILITY; VISIBLE RADIATION

Citation Formats

Janett, Gioele, Steiner, Oskar, and Belluzzi, Luca. Formal Solutions for Polarized Radiative Transfer. II. High-order Methods. United States: N. p., 2017. Web. doi:10.3847/1538-4357/AA7AA3.
Janett, Gioele, Steiner, Oskar, & Belluzzi, Luca. Formal Solutions for Polarized Radiative Transfer. II. High-order Methods. United States. https://doi.org/10.3847/1538-4357/AA7AA3
Janett, Gioele, Steiner, Oskar, and Belluzzi, Luca. 2017. "Formal Solutions for Polarized Radiative Transfer. II. High-order Methods". United States. https://doi.org/10.3847/1538-4357/AA7AA3.
@article{osti_22663242,
title = {Formal Solutions for Polarized Radiative Transfer. II. High-order Methods},
author = {Janett, Gioele and Steiner, Oskar and Belluzzi, Luca},
abstractNote = {When integrating the radiative transfer equation for polarized light, the necessity of high-order numerical methods is well known. In fact, well-performing high-order formal solvers enable higher accuracy and the use of coarser spatial grids. Aiming to provide a clear comparison between formal solvers, this work presents different high-order numerical schemes and applies the systematic analysis proposed by Janett et al., emphasizing their advantages and drawbacks in terms of order of accuracy, stability, and computational cost.},
doi = {10.3847/1538-4357/AA7AA3},
url = {https://www.osti.gov/biblio/22663242}, journal = {Astrophysical Journal},
issn = {0004-637X},
number = 2,
volume = 845,
place = {United States},
year = {Sun Aug 20 00:00:00 EDT 2017},
month = {Sun Aug 20 00:00:00 EDT 2017}
}