An empirical model for the polarization of pulsar radio emission

We present an empirical model for single pulses of radio emission from pulsars based on Gaussian probability distributions for relevant variables. The radiation at a specific pulse phase is represented as the superposition of radiation in two (approximately) orthogonally polarized modes (OPMs) from...

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Detalhes bibliográficos
Main Authors: Melrose, D, Miller, A, Karastergiou, A, Luo, Q
Formato: Journal article
Idioma:English
Publicado em: 2006

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