A statistical analysis of the fine-scale time structure of PSR 1133+16

Details A statistical analysis of the fine-scale time structure of PSR 1133+16 A statistical analysis of the fine-scale time structure of PSR 1133+16

Apr 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983azh....60..293s&link_type=abstract

(Astronomicheskii Zhurnal, vol. 60, Mar.-Apr. 1983, p. 293-300) Soviet Astronomy (ISSN 0038-5301), vol. 27, Mar.-Apr. 1983, p. 1

Astronomy and Astrophysics

Astronomy

8

Pulsars, Radio Emission, Autocorrelation, Fine Structure, Histograms, Statistical Analysis, Temporal Distribution

Scientific paper

Statistical analysis of the fine structure in the radio emission of PSR 1133 + 16 shows that the micropulse durations are not randomly distributed but display at least two characteristic time scales, one shorter than 250 microsec and the other between 250 microsec and about 1 msec. In more than half the pulses analyzed, the microstructure is quasiperiodic, with short (less than 625-microsec) periods being distinguished from long (625-2500-microsec) periods. The microstructure time-scale and quasiperiod distributions are compared for subpulses belonging to the two separate components of the mean pulse profile.

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