The spatial structure of the emitting region of the pulsar PSR 1702-19

Details The spatial structure of the emitting region of the pulsar PSR 1702-19 The spatial structure of the emitting region of the pulsar PSR 1702-19

May 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pazh...15..438k&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 15, May 1989, p. 438-442. In Russian. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

Pulsars, Spatial Distribution, Stellar Radiation, Lines Of Force, Pulsar Magnetospheres, Stellar Magnetic Fields, Stellar Rotation

Scientific paper

A method based on the interpulse analysis is proposed for determining the inclination of the magnetic axis to the spin axis (beta) and to the line of sight (sigma). For the pulsar PSR 1702-19, it is found that beta = 88 deg, sigma for the main pulse = -4 deg, and sigma for the interpulse = -8 deg. Also, it is shown that the halfwidth of open field line cone (theta) = 14 deg, the height of the emitting region (r) = 0.03, and the value for rLC = 4 x 10 to the 7th cm in the magnetosphere at a frequency of 400 MHz.

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