Pulsar nulling and drifting subpulse phase memory
Journal Article
·
· Astrophys. J.; (United States)
The standard polar cap model of pulsar radio emission provides acceptable explanations for a wide variety of observed pulsar characteristics. Nevertheless, we show that it has difficulty accounting for certain details pertaining to drifting subpulses, nulling, and mode changing. In particular, the persistence of drifting subpulse phase memory observed during pulsar nulling, as well as the phenomenon of nulling itself, seem to defy simple explanation.
- Research Organization:
- Department of Astronomy, California Institute of Technology
- OSTI ID:
- 5988425
- Journal Information:
- Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 263:2; ISSN ASJOA
- 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
ELECTROMAGNETIC RADIATION
FLUID MECHANICS
HYDRODYNAMICS
INTERACTIONS
MAGNETIC FIELDS
MAGNETOHYDRODYNAMICS
MATHEMATICAL MODELS
MECHANICS
NEUTRON STARS
PAIR PRODUCTION
PLASMA
PULSARS
RADIATIONS
RADIOWAVE RADIATION
STAR MODELS
STARS
Radio & X-Ray Sources
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
COSMIC RADIO SOURCES
ELECTROMAGNETIC RADIATION
FLUID MECHANICS
HYDRODYNAMICS
INTERACTIONS
MAGNETIC FIELDS
MAGNETOHYDRODYNAMICS
MATHEMATICAL MODELS
MECHANICS
NEUTRON STARS
PAIR PRODUCTION
PLASMA
PULSARS
RADIATIONS
RADIOWAVE RADIATION
STAR MODELS
STARS