Published July 1975
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Pulsar extinction
Description
Radio emission from pulsars, attributed to an instability associated with the creation of electron-positron pairs from gamma rays was investigated. The condition for pair creation therefore lead to an extinction condition. The relevant physical processes were analyzed in the context of a mathematical model, according to which radiation originated at the polar caps and magnetic field lines changed from a closed configuration to an open configuration at the force balance or corotation radius. (Author)
Availability note (English)
MF available from INIS under the Report Number.
Files
Additional details
Additional titles
- Augmented title (English)
- Instability associated with electron pair production
Publishing Information
- Imprint Pagination
- 28 p.
- Report number
- N--75-29969
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 8282463
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ELECTRON PAIRS; GAMMA RADIATION; INSTABILITY; MATHEMATICAL MODELS; PAIR PRODUCTION; PULSARS; RADIOWAVE RADIATION
- Descriptors DEC
- COSMIC RADIO SOURCES; ELECTROMAGNETIC RADIATION; INTERACTIONS; IONIZING RADIATIONS; PARTICLE INTERACTIONS; PARTICLE PRODUCTION; RADIATIONS
Optional Information
- Notes
- Available from NTIS. $3.75.
- Secondary number(s)
- NASA-CR--143272; SU-IPR--633.