Fluctuations in the 102-MHz pulse arrival time for four pulsars

Details Fluctuations in the 102-MHz pulse arrival time for four pulsars Fluctuations in the 102-MHz pulse arrival time for four pulsars

Oct 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982sva....26..545s&link_type=abstract

(Astronomicheskii Zhurnal, vol. 59, Sept.-Oct. 1982, p. 903-907) Soviet Astronomy (ISSN 0038-5301), vol. 26, Sept.-Oct. 1982, p.

Astronomy and Astrophysics

Astronomy

Pulsars, Pulse Rate, Data Processing, Fluctuation Theory, Numerical Integration, Signal To Noise Ratios

Scientific paper

The pulse phase fluctuations of four pulsars have been monitored in a
two-year observing program at 102.5-MHz frequency. For pulsars having P
greater than 1 sec, the frequency dependence of the phase residuals is
tested to see whether the fluctuations might be attributable to
emission-region displacements.

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