On the radio wave propagation in the pulsar magnetosphere

Details On the radio wave propagation in the pulsar magnetosphere On the radio wave propagation in the pulsar magnetosphere

2011-01-29

arxiv.org/abs/1101.5733v2

Astronomy and Astrophysics

Astrophysics

High Energy Astrophysical Phenomena

5 pages, 2 figures, 2 tables, short version of the paper for MNRAS (in preparation)

Scientific paper

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.

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