Backward-Wave Oscillator Regime in the Magnetosphere Cyclotron Maser Under an Arbitrary Direction of Wave Propagation Relative to an External Magnetic Field
- Authors: Grach V.S.1, Demekhov A.G.1,2
-
Affiliations:
- Institute of Applied Physics of the Russian Academy of Sciences
- Polar Geophysics Institute
- Issue: Vol 60, No 8 (2018)
- Pages: 595-608
- Section: Article
- URL: https://ogarev-online.ru/0033-8443/article/view/243821
- DOI: https://doi.org/10.1007/s11141-018-9830-6
- ID: 243821
Cite item
Abstract
We generalize the equations, which describe the backward-wave oscillator regime in the magnetized plasma in the presence of a jump (“step”) in the velocity distribution function of energetic charged particles, to the case of an arbitrary direction of the wave relative to an external magnetic field and an arbitrary wave mode. The dependence of instability threshold on the angle χ between the wave vector k and the external magnetic field B0 for whistler-mode waves and a slow extraordinary wave (Z-mode) is determined.
About the authors
V. S. Grach
Institute of Applied Physics of the Russian Academy of Sciences
Author for correspondence.
Email: vsgrach@appl.sci-nnov.ru
Russian Federation, Nizhny Novgorod
A. G. Demekhov
Institute of Applied Physics of the Russian Academy of Sciences; Polar Geophysics Institute
Email: vsgrach@appl.sci-nnov.ru
Russian Federation, Nizhny Novgorod; Apatity
Supplementary files
