A remark on co-rotation in pulsar magnetospheres

Details A remark on co-rotation in pulsar magnetospheres A remark on co-rotation in pulsar magnetospheres

Sep 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977ap%26ss..51..239b&link_type=abstract

Astrophysics and Space Science, vol. 51, no. 1, Sept. 1977, p. 239, 240.

Astronomy and Astrophysics

Astrophysics

1

Pulsar Magnetospheres, Pulsars, Relativistic Plasmas, Rotating Plasmas, Stellar Atmospheres, Stellar Rotation, Angular Velocity, Flow Velocity, Magnetohydrodynamic Flow

Scientific paper

Ardavan's (1976) expression relating distance from the light cylinder to the Lorentz factor of the relativistically corotating plasma of an axisymmetric pulsar magnetosphere is examined critically. An analysis is performed which yields a substantially different expression for the distance from the light cylinder in terms of the plasma's Lorentz factor at some cylindrical coordinate. It is concluded that a fuller investigation of the plasma velocity components near the light cylinder is warranted.

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