Properties of gaps in pulsar magnetospheres

Details Properties of gaps in pulsar magnetospheres Properties of gaps in pulsar magnetospheres

Jan 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981mnras.194...95h&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 194, Jan. 1981, p. 95-110.

Astronomy and Astrophysics

Astronomy

19

Charge Distribution, Magnetic Charge Density, Magnetic Stars, Pulsar Magnetospheres, Pulsars, Angular Velocity, Charged Particles, Gaps, Space Plasmas, Stellar Magnetic Fields, Temperature Effects

Scientific paper

The distribution of charged particles in the corotating regions of a pulsar magnetosphere is subject to the formation of gaps, in which the charge density (and particle density) becomes zero. Some detailed properties of such gaps (in the axisymmetric magnetosphere) are analyzed, in particular the properties associated with finite plasma temperature and with departures of the magnetosphere from corotation.

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