Published January 1988
| Version v1
Journal article
Modes of radio emission of PSR 1530+27 and magnetic poles
Description
It is proved by different methods that the radio emission of PSR 1530+27 is generated at all longitudes of the pulsar. The most probable process of the generation is the antenna one. Two identical modes, having the maximum intensity, are shifted by 145 deg = 0.4 T. The sum of the two modes yields the mean pulse. It is suggested that these modes are generated at the region of two magnetic poles of the asymmetrical dipole
Additional details
Additional titles
- Original title (Russian)
- Моды излучения PSR 1530+27 и магнитные полюса
Publishing Information
- Journal Title
- Astron. Zh.
- Journal Volume
- 65
- Journal Issue
- 1
- Series
- Astron. Zh.
- Journal Page Range
- 131-139
- ISSN
- 0004-6299
- CODEN
- ASZHA
INIS
- Country of Publication
- Russian Federation
- Country of Input or Organization
- USSR
- INIS RN
- 19094370
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- CORRELATION FUNCTIONS; PULSARS; RADIATION FLUX; RADIOWAVE RADIATION; SPACE DEPENDENCE; TIME DEPENDENCE
- Descriptors DEC
- COSMIC RADIO SOURCES; ELECTROMAGNETIC RADIATION; FUNCTIONS; RADIATIONS