Other
Scientific paper
Dec 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990mnras.247..529a&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 247, Dec. 15, 1990, p. 529-548.
Other
61
Magnetohydrodynamic Stability, Pulsar Magnetospheres, Pulsars, Radio Stars, Stellar Radiation, Extraterrestrial Radiation, Neutron Stars, Plasma Waves, Relativistic Particles, Solitary Waves
Scientific paper
A coherent pulsar emission mechanism is developed which involves, in addition to the assumed development of a relativistic two-stream instability in the neutron star's magnetosphere, both linear and nonlinear instability-development stages. While the linear treatment indicates the pertinence of a dispersion relation specific to pulsars, and the importance of the consequent, unstable plasma wave solution, the nonlinear treatment indicates the evolution of the two-stream interaction and demonstrates the stability of Langmuir soliton-like solutions, designated 'Langmuir microstructures', in the magnetospheric pulsar plasma; these microstructures generate two different types of radiation mechanism, of which one appears insufficient for the radiated power observed, while the other is a direct radiation by the microstructures themselves, and can account for both observed radio luminosities and temporal microstructures.
Asseo Estelle
Pelletier Guy
Sol Hé&Lgrave
No associations
LandOfFree
A non-linear radio pulsar emission mechanism does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with A non-linear radio pulsar emission mechanism, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A non-linear radio pulsar emission mechanism will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1633163