Development of Kolmogorov spectrum in the pulsar radio emission
classification
🌌 astro-ph
keywords
spectrumanalysisformationpossibleradiostationaryaccountagreement
read the original abstract
It is shown that the scattering of electromagnetic waves by Langmuir ones taking into the account the electric drift motion of particles, is the most intense nonlinear process and should be responsible for the formation of radiation spectrum of radio pulsars. Performed analysis indicates that in the case of existence of inertial interval formation of stationary spectra is possible. Analysis of linear mechanisms of wave generation and silk allows to conclude that only possible stationary solution has spectral index $\alpha =-1.5$. Obtained spectrum is in good agreement with observational data.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.