Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987afz....27..489b&link_type=abstract
Astrofizika (ISSN 0571-7132), vol. 27, Dec. 1987, p. 489-498. In Russian.
Astronomy and Astrophysics
Astronomy
1
Angular Distribution, Computerized Simulation, Electromagnetic Scattering, Interstellar Matter, Pulsars, Pulse Duration, Cosmic Plasma, Statistical Analysis
Scientific paper
A computer program is considered that enables the calculation of the average scattered pulse profile and pulsar apparent angular size resulting from scattering in a statistically inhomogeneous interstellar medium. This program makes use of the algorithm based on the stochastic ray-path method and the Monte-Carlo technique. The possibilities are discussed of applying the program to the interpretation of pulsar observational data.
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