A New Explanation of the High Effective Temperatures in Pulsar Radioemissions
- 1 December 1982
- journal article
- Published by IOP Publishing in Physica Scripta
- Vol. 26 (6) , 455-458
- https://doi.org/10.1088/0031-8949/26/6/007
Abstract
A new nonlinear process, which can explain the high effective temperatures of pulsar radio emissions, is proposed. It is due to the excitation of low frequency Alfvén waves by waves resonantly interacting with the electrons and positrons in the pulsar ultrarelativistic plasma.Keywords
This publication has 26 references indexed in Scilit:
- Damping and excitation of Langmuir waves in an inhomogeneous relativistic plasma; general theory and pulsar applicationsPlasma Physics, 1982
- On theory of Cherenkov instability of ultrarelativistic beams with one-dimensional distribution of momenta of particlesPlasma Physics, 1981
- Oscillations of an isotropic relativistic plasmaPlasma Physics, 1980
- Some problems of pulsar physics or I'm madly in love with electricitySpace Science Reviews, 1979
- Plasma collective effects and pulsar emission modelsThe Astrophysical Journal, 1979
- Wave production in an ultrarelativistic electron-positron plasmaThe Astrophysical Journal, 1978
- Theory of pulsars - Polar caps, sparks, and coherent microwave radiationThe Astrophysical Journal, 1975
- Role of Adrenal Cortex and Medulla in HypertensionNature New Biology, 1973
- A Model of PulsarsThe Astrophysical Journal, 1971
- On pulsar emission mechanismsPhysics Letters A, 1970