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2006MNRAS.368.1764P - Mon. Not. R. Astron. Soc., 368, 1764-1772 (2006/June-1)
Statistics of the individual-pulse polarization based on propagation effects in the pulsar magnetosphere.
PETROVA S.A.
Abstract (from CDS):
The model suggested allows one to reproduce the basic features of the one-dimensional distributions of the individual-pulse polarization characteristics. Besides that, the propagation origin of the pulsar polarization implies a certain correlation between the mode ellipticity and position angle. On a qualitative level, for different sets of parameters, the expected correlations appear compatible with the observed ones. Further theoretical studies are necessary to establish the quantitative correspondence of the model to the observational results and to develop a technique of diagnostics of the pulsar plasma on this basis.
Abstract Copyright: 2006 The Author. Journal compilation © 2006 RAS
Journal keyword(s): plasmas - polarization - waves - pulsars: general
Simbad objects: 2
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