A relation between subpulse widths and the polarization properties of pulsars

Details A relation between subpulse widths and the polarization properties of pulsars A relation between subpulse widths and the polarization properties of pulsars

Jan 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988mnras.230...87a&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 230, Jan. 1, 1988, p. 87-95.

Astronomy and Astrophysics

Astronomy

7

Curve Fitting, Polarization Characteristics, Pulsars, Pulse Duration, Radio Emission, Histograms, Linear Polarization, Polar Caps

Scientific paper

A discussion of the techniques used for estimating the subpulse widths of pulsars concludes that Gaussian fitting has advantages over autocorrelation techniques for single pulse data recorded with millisecond resolution at radio frequencies around 400 MHz. Measurements are presented for 53 pulsars, made from radio observations obtained at Jodrell Bank. A relation is found between the subpulse widths and the polarization properties of the pulsars, which the author interprets in terms of current polar-cap models of the radio emission.

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