Theory of orthogonal modes in pulsar radio emission
Journal Article
·
· Sov. Astron. Lett. (Engl. Transl.); (United States)
OSTI ID:5080885
The magnetoactive, relativistic electron--positron plasma in a pulsar magnetosphere will influence the propagation of radio waves and the manner in which they are polarized. The distinctive double-peaked structure and mutually orthogonal polarization of subpulses might be attributable to anomalous double refraction as radio waves pass through the dense magnetospheric plasma.
- Research Organization:
- Institute for Space Research, USSR Academy of Sciences, Moscow
- OSTI ID:
- 5080885
- Journal Information:
- Sov. Astron. Lett. (Engl. Transl.); (United States), Journal Name: Sov. Astron. Lett. (Engl. Transl.); (United States) Vol. 7:6; ISSN SALED
- Country of Publication:
- United States
- Language:
- English
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Related Subjects
640102* -- Astrophysics & Cosmology-- Stars & Quasi-Stellar
Radio & X-Ray Sources
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
COSMIC RADIO SOURCES
EARTH ATMOSPHERE
ELECTROMAGNETIC RADIATION
MAGNETOSPHERE
OPTICAL PROPERTIES
OSCILLATION MODES
PHYSICAL PROPERTIES
PLASMA
POLARIZATION
PULSARS
PULSES
RADIATIONS
RADIOWAVE RADIATION
REFRACTIVITY
RELATIVISTIC PLASMA
WAVE PROPAGATION
Radio & X-Ray Sources
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
COSMIC RADIO SOURCES
EARTH ATMOSPHERE
ELECTROMAGNETIC RADIATION
MAGNETOSPHERE
OPTICAL PROPERTIES
OSCILLATION MODES
PHYSICAL PROPERTIES
PLASMA
POLARIZATION
PULSARS
PULSES
RADIATIONS
RADIOWAVE RADIATION
REFRACTIVITY
RELATIVISTIC PLASMA
WAVE PROPAGATION