Published May 1977
| Version v1
Journal article
Model for the microstructure emission of pulsars
Description
Recent observations of radio radiation have been used to construct a qualitative model of the emitting region near pulsars. The data can be reconciled with the view that dense regions, themselves containing many coherent radiating filaments, extend for long distances along the dipolar field lines. (author)
Additional details
Identifiers
Publishing Information
- Journal Title
- Monthly Notices of the Royal Astronomical Society
- Journal Volume
- 179
- Journal Issue
- 3
- Series
- Mon. Not. R. Astron. Soc.
- Journal Page Range
- 311-315
- ISSN
- 0035-8711
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- United Kingdom
- INIS RN
- 8326599
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- COHERENT RADIATION; PULSARS; RADIOWAVE RADIATION; STAR MODELS; WAVE PROPAGATION
- Descriptors DEC
- COSMIC RADIO SOURCES; ELECTROMAGNETIC RADIATION; MATHEMATICAL MODELS; RADIATIONS
Optional Information
- Notes
- Updated automatically by Metadata and Full-Text Enrichment Agent