On the origin of the rapid fluctuations in the level of pulsar radiation

Details On the origin of the rapid fluctuations in the level of pulsar radiation On the origin of the rapid fluctuations in the level of pulsar radiation

Jun 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980pazh....6..282d&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 6, May 1980, p. 282-285.) Soviet Astronomy Letters, vol. 6, May-June 1980, p. 156-158.

Astronomy and Astrophysics

Astronomy

1

Astronomical Models, Pulsars, Radiant Flux Density, Radio Astronomy, Stellar Radiation, Astronomical Photometry, Fluctuation Theory, Propagation Velocity

Scientific paper

A mechanism is proposed to explain the rapid fluctuations observed in the radio intensity level of pulsars. The mechanism rests on an effect discussed previously by the authors: electrons would become accelerated when they are trapped by an amplitude-modulated electromagnetic wave emitted by the pulsar, since the group velocity of the wave will rise as it travels toward regions of lower density. Rapid fluctuations will then develop because of the absorption of the radiant energy by the accelerated electrons.

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