Polarization of the radio emission of the pulsar PP 0943

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

Apr 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975sva....18..546s&link_type=abstract

(Astronomicheskii Zhurnal, vol. 51, Sept.-Oct. 1974, p. 927-930.) Soviet Astronomy, vol. 18, Mar.-Apr. 1975, p. 546, 547. Trans

Astronomy and Astrophysics

Astronomy

Fine Structure, Polarized Electromagnetic Radiation, Pulsars, Radio Emission, Astronomical Spectroscopy, 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.

Affiliated with

Also associated with

No associations

Rating

Polarization of the radio emission of the pulsar PP 0943 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Polarization of the radio emission of the pulsar PP 0943, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Polarization of the radio emission of the pulsar PP 0943 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-949319