A mode change in the radio emission from the pulsar PSR 1822-09

Details A mode change in the radio emission from the pulsar PSR 1822-09 A mode change in the radio emission from the pulsar PSR 1822-09

Jan 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981mnras.194p...7m&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 194, Jan. 1981, p. 7P-11P.

Astronomy and Astrophysics

Astronomy

8

Pulsars, Pulse Duration, Radio Emission, Emission Spectra, Propagation Modes, Radio Astronomy

Scientific paper

A mode change has been detected in the 1720-MHz and 2650-MHz radiation from PSR 1822-09. At low average intensities, the first component of the main pulse abruptly drops to very small intensity. To within measurement errors, the interpulse remains unchanged. The evidence is consistent with a model in which the main pulse and interpulse originate at opposite magnetic poles.

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