Emission modes of PSR 1530 + 27 and magnetic poles

Details Emission modes of PSR 1530 + 27 and magnetic poles Emission modes of PSR 1530 + 27 and magnetic poles

Feb 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988azh....65..131b&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 65, Jan.-Feb. 1988, p. 131-139. In Russian.

Astronomy and Astrophysics

Astronomy

Magnetic Poles, Pulsars, Radio Emission, Longitude, Magnetospheres, Pulse Duration

Scientific paper

It is shown that radio emission of the pulsar PSR 1530 + 27 is generated at all longitudes of the object. The antenna mechanism is shown to be the most probable generation mechanism. Two identical modes, shifted by 145 deg = 0.4 T, have the maximum intensity. The sum of the two modes yields the mean pulse profile. It is suggested that these modes are generated in the region of two magnetic poles of the asymmetrical dipole.

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