Published 1977
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Pulsar magnetic alignment. The drifting subpulses
Description
According to Ruderman and Sutherland (Ap.J.;196:51 (1975)) the subpulse drift observed in certain pulsars is a consequence of the circulation around the magnetic axis of electron-positron discharges occurring within an acceleration region near the polar cap. The predicted period of circulation P3 is of the correct order of magnitude, but the sense of circulation and therefore the direction of subpulse drift is not consistent with indirect evidence, from observed integrated pulse widths, on the variation with pulsar age of the angle between the spin and magnetic axes. It is shown that this problem is resolved by a model of the acceleration electric field based on space charge limited ion flow. (author)
Availability note (English)
MF available from INIS under the Report Number.
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Additional details
Publishing Information
- Imprint Pagination
- 12p.
- Report number
- OU-NPL--9/77
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- United Kingdom
- INIS RN
- 8319944
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ACCELERATION; ANGULAR DISTRIBUTION; ELECTRIC FIELDS; IONS; MAGNETIC FIELDS; MATHEMATICAL MODELS; PULSARS; PULSES; RADIOWAVE RADIATION; ROTATION; SPACE CHARGE; VARIATIONS
- Descriptors DEC
- CHARGED PARTICLES; COSMIC RADIO SOURCES; DISTRIBUTION; ELECTROMAGNETIC RADIATION; RADIATIONS