Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apjs...55..247s&link_type=abstract
Astrophysical Journal Supplement Series (ISSN 0067-0049), vol. 55, June 1984, p. 247-277
Astronomy and Astrophysics
Astronomy
155
Polarization Characteristics, Pulsars, Radio Astronomy, Statistical Analysis, Angular Distribution, Circular Polarization, Instrument Errors, Linear Polarization, Waveforms
Scientific paper
Individual-pulse polarization observations of 11 strong low-dispersion pulsars obtained at 1404 MHz using the 305-m Arecibo telescope during October, 1981 are reported; four pulsars were observed simultaneously at 800 MHz using the 92-m NRAO telescope at Green Bank, West Virginia. The results are presented graphically as distribution displays and polarization waveforms and compared with published data obtained at lower frequencies. Depolarization is observed at high frequencies and attributed to instantaneous superposition of nearly 100-percent orthogonally polarized radiation, which is found at both high and low frequencies (430-1404 MHz). These findings suggest that most pulsar emission occurs in one of the orthogonal polarization modes.
Boriakoff Valentin
Cordes James M.
Rankin Joanna M.
Stinebring Daniel R.
Weisberg Joel M.
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