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Uspekhi Fizicheskikh Nauk, 2016, Volume 186, Number 10, Pages 1090–1116
DOI: https://doi.org/10.3367/UFNr.2016.05.037813
(Mi ufn5670)
 

This article is cited in 26 scientific papers (total in 26 papers)

100th ANNIVERSARY OF THE BIRTH OF V L GINZBURG. REVIEWS OF TOPICAL PROBLEMS

Double plasma resonance and its manifestations in radio astronomy

V. V. Zheleznyakov, E. Ya. Zlotnik, V. V. Zaitsev, V. E. Shaposhnikov

Institute of Applied Physics, Russian Academy of Sciences, Nizhny Novgorod
References:
Abstract: The double plasma resonance (DPR) effect is the phenomenon of a sharply increased instability of plasma waves in a magnetized plasma when the upper hybrid frequency coincides with the cyclotron harmonic frequency. A radiation mechanism associated with this effect provides an explanation for the origin of the ‘zebra pattern’ in radio spectra of the Sun, Jupiter, and the Crab pulsar. The diversity of these astronomical objects and the successful interpretation of their spectra in terms of the DPR effect point to the universal nature of this phenomenon and suggest that the same radiation mechanism can operate under a variety of astronomical conditions.
Funding agency Grant number
Russian Foundation for Basic Research 14-02-00766
14-02-00133
16-02-00373
Russian Academy of Sciences - Federal Agency for Scientific Organizations П-7
Russian Science Foundation 16-12-10528
This study was supported by the RFBR grants 14-02-00766, 14-02-00133, and 16-02-00373, by the Program of Basic Research of the Presidium of RAS P-7, and partially by the RSF grant 16-12-10528.
Received: May 6, 2016
Accepted: May 24, 2016
English version:
Physics–Uspekhi, 2016, Volume 59, Issue 10, Pages 997–1020
DOI: https://doi.org/10.3367/UFNe.2016.05.037813
Bibliographic databases:
PACS: 52.35.-g, 52.35.Hr, 52.35.Qz, 96.60.P-, 96.60.Tf, 97.60.Gb
Language: Russian
Citation: V. V. Zheleznyakov, E. Ya. Zlotnik, V. V. Zaitsev, V. E. Shaposhnikov, “Double plasma resonance and its manifestations in radio astronomy”, UFN, 186:10 (2016), 1090–1116; Phys. Usp., 59:10 (2016), 997–1020
Citation in format AMSBIB
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