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Microstructure Crosscorrelation in Pulses Simultaneously Observed at Frequencies Separated by up to 1 GHz

Published online by Cambridge University Press:  14 August 2015

Valentin Boriakoff  and
Dale C. Ferguson
Valentin Boriakoff
Affiliation:
National Astronomy and Ionosphere Center, Cornell University, Ithaca, NY 14853
Dale C. Ferguson
Affiliation:
NAIC, Arecibo Observatory, Arecibo, Puerto Rico 00612

Abstract

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Microstructure crosscorrelation of pulses observed simultaneously at various separations in frequency in the range of 196 to 1420 MHz was done for PSR 0950+08 and PSR 1133+16 at the Arecibo Observatory. Microstructure and subpulse components were identified in the crosscorrelations, and their behaviour vs. pulse longitude was studied. Drastic differences in the subpulse and micropulse behaviour are noted, related in particular to component separation in the double peak average pulse profile of PSR 1133+16. Here the subpulses follow the average pulse profile component separation but the microstructure does not. Interpretation and constraints in terms of some current theories are also presented.

Type
III. Radio Observations of Pulsars
Information
Symposium - International Astronomical Union , Volume 95: Pulsars , 1981 , pp. 191 - 196
Copyright
Copyright © Reidel 1981 

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