Published 1981 | Version v1
Book

Microstructure crosscorrelation in pulses simultaneously observed at frequencies separated by up to 1 GHz

  • 1. Cornell Univ., Ithaca, NY (USA)
  • 2. NAIC, Arecibo Observatory, Arecibo, PR, USA

Description

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 microspulse 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. (Auth.)

Additional details

Publishing Information

Publisher
D. Reidel.
Imprint Place
Dordrecht, Netherlands
ISBN
90-277-1280-8
Imprint Title
Pulsars
Imprint Pagination
475 p.
Journal Issue
no. 95
Series
International Astronomical Union Symposium.
Journal Page Range
p. 191-196.

Conference

Title
95. International Astronomical Union symposium on pulsars.
Dates
26 - 29 Aug 1980.
Place
Bonn, Germany, F.R.

INIS

Country of Publication
Netherlands
Country of Input or Organization
Netherlands
INIS RN
12640087
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Conference
Descriptors DEI
CORRELATIONS; EMISSION; MHZ RANGE; MHZ RANGE 100-1000; PULSARS; RADIOWAVE RADIATION; TIME DEPENDENCE
Descriptors DEC
COSMIC RADIO SOURCES; ELECTROMAGNETIC RADIATION; FREQUENCY RANGE; RADIATIONS

Optional Information

Notes
Imprint:Includes subject index.