An empirical model for the polarization of pulsar radio emission

An empirical model for the polarization of pulsar radio emission

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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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Dades bibliogràfiques
Autors principals:	Melrose, D, Miller, A, Karastergiou, A, Luo, Q
Format:	Journal article
Idioma:	English
Publicat:	2006

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