Submicrosecond time resolution observations of PSR0950+08

Details Submicrosecond time resolution observations of PSR0950+08 Submicrosecond time resolution observations of PSR0950+08

Nov 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978natur.276...45h&link_type=abstract

Nature, vol. 276, Nov. 2, 1978, p. 45-47.

Astronomy and Astrophysics

Astronomy

39

Micropulsations, Pulsars, Pulse Duration, Radio Astronomy, Time Dependence, Astronomical Models, Autocorrelation, Brightness Temperature, High Resolution, Microstructure, Pulse Amplitude Modulation, Random Noise, Relativistic Particles, Signal Detection

Scientific paper

The paper reports observations of isolated unresolved 0.8 microsec micropulses which, if it is assumed that a radiating region producing a pulse of duration t cannot be larger than ct, result from emitting volumes less than 250 m in extent. It is shown that even with this high time resolution, the observations are consistent with Rickett's (1975) amplitude modulated noise model for pulsar emission, where all of the observed intensity fluctuations can be represented as the modulation of a more fundamental Gaussian noise process.

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