Structure of the magnetic field in pulsars

Details Structure of the magnetic field in pulsars Structure of the magnetic field in pulsars

Apr 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983afz....19..315m&link_type=abstract

(Astrofizika, vol. 19, Apr.-June 1983, p. 315-321) Astrophysics (ISSN 0571-7132), vol. 19, no. 2, Oct. 1983, p. 182-186. Transla

Astronomy and Astrophysics

Astrophysics

1

Magnetic Field Configurations, Pulsars, Stellar Magnetic Fields, Angles (Geometry), Magnetic Dipoles, Stellar Models

Scientific paper

For four pulsars, on the basis of the polar cap model, comparison of the behavior of the position angle along the mean profile at frequencies 400-1665 MHz shows that the change in the angle of inclination of the axis of the magnetic dipole to the rotation axis of the neutron star in the region of generation of these frequencies is less than 2 deg. It is shown that for pulsars with two-component mean profiles the distortion of the magnetic field due to the rotation of the neutron star is unimportant. It is concluded that in the region of generation of the radio emission of pulsars described by the polar-cap model the magnetic field is nearly dipolar.

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