Polarization of radio emission from the pulsar PP 0943

Details Polarization of radio emission from the pulsar PP 0943 Polarization of radio emission from the pulsar PP 0943

Oct 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974azh....51..927s&link_type=abstract

Astronomicheskii Zhurnal, vol. 51, Sept.-Oct. 1974, p. 927-930. In Russian.

Astronomy and Astrophysics

Astronomy

Astronomical Spectroscopy, Fine Structure, Polarized Electromagnetic Radiation, Pulsars, Radio Emission, Emission Spectra, Faraday Effect, Frequency Response, Interstellar Magnetic Fields, Radio Astronomy, Scintillation

Scientific paper

The fine spectral structure caused by the Faraday effect in the interstellar medium was revealed in radio observations of the pulsar PP 0943 in the wavelength range from 80 to 90 MHz. The average degree of polarization in this range was 40 plus or minus 10 percent. The average strength, weighted according to number of electrons, of the interstellar line-of-sight magnetic field component was found to be about 1.3 microgauss. The frequency correlation radius of interstellar scintillations at 100-MHz frequency in the direction of PP 0943 was estimated to be 2.4 plus or minus 0.9 kHz.

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