On the radio wave propagation in the pulsar magnetosphere
High Energy Astrophysical Phenomena
2015-03-18 v2
Abstract
The key properties of the wave propagation theory in the magntosphere of radio pulsars based on the Kravtsov-Orlov equation are presented. It is shown that for radio pulsars with known circular polarization and the swing of the linear polarization position angle one can determine which mode, ordinary or extraordinary one, forms mainly the mean profile of the radio emission. The comparison of the observational data with the theory predictions demonstrates their good agreement.
Keywords
Cite
@article{arxiv.1101.5733,
title = {On the radio wave propagation in the pulsar magnetosphere},
author = {V. S. Beskin and A. A. Philippov},
journal= {arXiv preprint arXiv:1101.5733},
year = {2015}
}
Comments
5 pages, 2 figures, 2 tables, short version of the paper for MNRAS (in preparation)