Curvature radiation and subpulse polarization characteristics in the observed emission of PSR 2303 + 30

Details Curvature radiation and subpulse polarization characteristics in the observed emission of PSR 2303 + 30 Curvature radiation and subpulse polarization characteristics in the observed emission of PSR 2303 + 30

Mar 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...256..495g&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 256, no. 2, p. 495-497.

Astronomy and Astrophysics

Astrophysics

9

Emission Spectra, Polarization Characteristics, Pulsars, Astronomical Polarimetry, Circular Polarization, Stellar Magnetic Fields, Stellar Winds

Scientific paper

We analyze Arecibo single pulse polarization measurements at 430 MHz for PSR 2303 + 30. Single pulses typically consist of one or two subpulses. Each subpulse is associated with circular polarization which reverses sense near the subpulse peak and with its own swing of the position angle which does not coincide with the average position angle curve. We attempt to explain these observational characteristics of single pulses in the framework of coherent curvature radiation.

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