Multifrequency observations of pulsars

Details Multifrequency observations of pulsars Multifrequency observations of pulsars

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pazh...15.1001m&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 15, Nov. 1989, p. 1001-1007. In Russian. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

Frequency Distribution, Pulsars, Radio Emission, Cross Correlation, Electric Potential, Radio Telescopes

Scientific paper

Results are presented from simultaneous single pulse observations at 410 MHz, 928 MHz, and 5860 MHz. The pulsars PSR 1133+16 and 1929+10 show correlations between single pulse intensity fluctuations over the whole frequency range. It is proposed that the dynamics of electron-proton pair production in the jump of electric potential above the surface of a neutron star may determine single pulse intensity fluctuations over a broad radio frequency range.

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