Mechanism for the radio emission of pulsars
Journal Article
·
· JETP Lett. (Engl. Transl.); (United States)
OSTI ID:6784524
An instability of the flow of a relativistic electron-positron plasma in a strong curvilinear magnetic field is predicted theoretically. This instability can explain the origin and basic properties of the observed radio emission of pulsars.
- Research Organization:
- Fizicheskii Institut, Moscow, USSR
- OSTI ID:
- 6784524
- Journal Information:
- JETP Lett. (Engl. Transl.); (United States), Journal Name: JETP Lett. (Engl. Transl.); (United States) Vol. 44; ISSN JTPLA
- 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
ELECTRODYNAMICS
ELECTROMAGNETIC RADIATION
INSTABILITY
MAGNETIC FIELDS
NEUTRON STARS
PLASMA
PLASMA DENSITY
PLASMA INSTABILITY
PULSARS
RADIATIONS
RADIOWAVE RADIATION
RELATIVISTIC PLASMA
STARS
Radio & X-Ray Sources
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
COSMIC RADIO SOURCES
ELECTRODYNAMICS
ELECTROMAGNETIC RADIATION
INSTABILITY
MAGNETIC FIELDS
NEUTRON STARS
PLASMA
PLASMA DENSITY
PLASMA INSTABILITY
PULSARS
RADIATIONS
RADIOWAVE RADIATION
RELATIVISTIC PLASMA
STARS