An empirical model for the polarization of pulsar radio emission

Monthly Notices of the Royal Astronomical Society

Volumn 365, Issue 2, 2006, Pages 638-646

  Melrose, Don ^a   Miller, Andrew ^a   Karastergiou, Aris ^a,b   Luo, Qinghuan ^a  

^a UNIVERSITY OF SYDNEY   (Australia)

^b IRAM   (France)

Author keywords

Polarization; Pulsars: general; Pulsars: individual: PSR B0329+54

Indexed keywords

PROBABILITY DISTRIBUTIONS; PULSARS; SPHERES;

EMPIRICAL MODEL; GAUSSIAN PROBABILITY DISTRIBUTIONS; ORTHOGONALLY POLARIZED MODES; PULSAR RADIO EMISSIONS; PULSAR: INDIVIDUAL: PSR B0329+54; PULSARS: GENERAL; PULSARS:INDIVIDUAL; PULSE PHASE; RADIO EMISSION; SINGLE PULSE;

POLARIZATION;

EID: 33645058658     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2005.09759.x     Document Type: Article

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