2014/09/25 by F. Marin, Frédéric Marin, Marin, F. +2
Earth and Planetary Sciences · Physics and Astronomy · #85-05 #Astrophysics of Galaxies (astro-ph.GA) #Atmospheric Ozone and Climate #FOS: Physical sciences #High Energy Astrophysical Phenomena (astro-ph.HE) #Instrumentation and Methods for Astrophysics (astro-ph.IM) #Ionosphere and magnetosphere dynamics #J.2.3 #J.2.9 #Solar and Space Plasma Dynamics #acm:85-05 #astro-ph.GA #astro-ph.HE #astro-ph.IM #msc:85-05
paper · pdf · doi:10.48550/arxiv.1409.7278
6 pages, 2 figures, to be published in the Proceedings of the annual meeting of the French Astronomical Society
arxiv created 2014/09/25 · openalex publication_date 2014/09/25 · arxiv updated 2014/09/26 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
Since it became publicly available in 2004, the radiative transfer code STOKES has been used to model the spectroscopic, polarimetric, timing and imaging signatures for different astrophysical scenarios. Ten years later, at the release of a new version of the Monte Carlo code, we make a census of the different scientific cases explored with STOKES and review the main results obtained so far.