Fluctuations of pulsar emission with sub-microsecond time-scales

Details Fluctuations of pulsar emission with sub-microsecond time-scales Fluctuations of pulsar emission with sub-microsecond time-scales

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.110..293g&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 110, no. 2, March 1985, p. 293-296.

Astronomy and Astrophysics

Astrophysics

3

Emission Spectra, Pulsars, Stellar Models, Stellar Oscillations, Temporal Distribution, Coherent Radiation, Radiant Flux Density

Scientific paper

A model of pulsar emission fluctuations down to sub-microsecond
time-scales is presented. The model is consistent with the empirical
amplitude modulated noise model. It is proposed that the time-scale of
the shortest observed micropulses is determined by the coherence of
single-particle curvature radiation.

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