Observations of pulsar spectra at 1420 MHz

Details Observations of pulsar spectra at 1420 MHz Observations of pulsar spectra at 1420 MHz

Dec 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974a%26a....37..285w&link_type=abstract

Astronomy and Astrophysics, vol. 37, no. 2, Dec. 1974, p. 285-290.

Astronomy and Astrophysics

Astronomy

10

Interstellar Radiation, Microwave Spectra, Pulsars, Spectral Correlation, Stellar Spectra, Fine Structure, Radio Astronomy, Scintillation, Spectrometers, Statistical Analysis

Scientific paper

Using a correlation spectrometer, narrow-band spectra integrated over short time intervals have been measured at 1420 MHz for four pulsars. The observed large scatter of decorrelation widths is explained in terms of a simple theory based on a ray approximation. We conclude that the statistical properties of this scatter are not due to experimental errors, but depend on the number of interfering beams reaching the observer as well as on the pulsar dispersion measure.

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