Diffraction effects in pulsating radio sources

Details Diffraction effects in pulsating radio sources Diffraction effects in pulsating radio sources

Feb 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apl....16...35h&link_type=abstract

Astrophysical Letters, vol. 16, no. 1, 1975, p. 35-38. USAF-supported research.

Astronomy and Astrophysics

Astrophysics

Astronomical Models, Emission Spectra, Pulsars, Radio Emission, Wave Diffraction, Normal Density Functions, Pulse Duration, Scintillation Counters, Spectrum Analysis, Stellar Spectra

Scientific paper

A pulsar radio emission model is developed to explore the effects of diffraction on pulsar beaming. At very low frequencies (not exceeding 2n MHz, where n is the number of pulse components), an increase of pulse width and the discovery of new pulsars are predicted. The pulse width increase might be difficult to untangle from interstellar scintillation effects. Observation of these diffraction effects would place restrictions on the size and radius of curvature of the emission regions.

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