The distribution of emission regions in the magnetospheres of pulsars

Details The distribution of emission regions in the magnetospheres of pulsars The distribution of emission regions in the magnetospheres of pulsars

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991pazh...17..595m&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 17, July 1991, p. 595-604. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

1

Line Of Sight, Pulsar Magnetospheres, Radio Emission, Neutron Stars, Radiation Distribution, Stellar Magnetic Fields

Scientific paper

An earlier method for estimating the distances between the line of sight and the emission cone center is used to show that the present estimates of angular distances of a line of sight from the center of the emission cone are in agreement with the traditional concept of decreasing cone sizes at high frequencies. It is inferred from a comparison of the distributions of generation levels with different models that, in a number of pulsars, the magnetic field is nondipolar.

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