Physics of auroral phenomena : proceedings of the 38th annual seminar, Apatity, 2-6 march, 2015 / [ed. board: A. G. Yahnin, N. V. Semenova]. - Апатиты : Издательство Кольского научного центра РАН, 2015. - 189 с. : ил., табл.
M E Viktorov et al. competition of the instability and stimulated scattering in the process of generation of plasma waves, or the excitation of fast magnetosonic oscillations of the plasma in the magnetic trap. Since rather high amplification coefficients of plasma waves are realized under the conditions of the experiment, the first reason for occurrence of the pulsations seems to be more probable. The mechanism of double plasma resonance is applied to explain many phenomena in astrophysics. Therefore, laboratory confirmation of this mechanism and identification of its new features, specifically, the pulse regime of generation, are of great importance for future studies of different astrophysical objects. Acknowledgements. This work was supported by the Ministry of Education and Science o f the Russian Federation (project No. 14.Z50.31.0007), Russian Foundation for Basic Research (projects 13-02-00951 and 14-02-31521), and Program No. 15 of the Department of Physical Sciences of the Russian Academy of Sciences “Plasma processes in space and in laboratory.” The work by М. E. Viktorov was also supported by the Grant Council of the President of the Russian Federation (SP-4857.2013.3). The authors are grateful to E.Ya. Zlotnik for discussions of the article. References 1. V.V. Zaitsev and A. V. Stepanov, Astron. Astrophys., 45, 135 (1975). 2. V.V. Zheleznyakov and E.Ya. Zlotnik, Solar Phys., 43,431 (1975). 3. V.V. Zheleznyakov and E.Ya. Zlotnik, Solar Phys., 44, 447 (1975). 4. A.A. Kuznetsov and V.G. Vlasov, Planet. Space Sci., 75, 167 (2013). 5. E.E. Titova, A.G. Demekhov, D.L. Pasmanik, et al., Geophys. Res. Lett., 34., L02112 (2007). 6 . T.N. Hankins and J. A. Eilek, Astrophys. J., 670, 693 (2007). 7. V.V. Alikaev, V. M. Glagolev, and S. A. Morozov, Plasma Phys., 10, No. 8 , 753 (1968). 8 . J.H. Booske, W.D.Getty, R.M.Gilgenbach, and R. A. Jong, Phys. Fluids, 28, 3116 (1985). 9. A.V. Vodopyanov, S.V.Goiubev, A.G. Demekhov, et al., Plasma Phys. Rep., 31, No. 11, 927 (2005). 10. A.G. Shalashov, A.V.Vodopyanov, S. V. Golubev, et al., JETP Lett., 84, 314 (2006). 11. A.V.Vodopyanov, S.V.Goiubev, A.G. Demekhov, et al., J. Exp. Theor. Phys., 104, 296 (2007). 12. M.E. Viktorov, A. V.Vodopyanov, S.V.Goiubev, et al., Radiophys. Quantum Electron., 56, No. 1, 12 (2013). 13. M.E. Viktorov, S. V. Golubev, E. D. Gospodchikov, et al., Radiophys. Quantum Electron., 56, No. 4,216 (2013). 14. A.V. Vodopyanov, S.V. Golubev, V.G. Zorin, et al., Tech. Phys. Lett., 25, 588 (1999). 15. A.G. Shalashov, S.V.Goiubev, E.D.Gospodchikov, et al., Plasma Phys. Control. Fusion, 54, 085023 (2012). 16. R.R. Sharma and L. Vlahos, Astrophys. J., 280,405 (1984). 17. V.V. Zheleznyakov, Radiation in Astrophysical Plasma, Janus-K, Moscow, p. 380 (1997). 18. V.V. Zaitsev, Solar Phys., 20, 95 (1971). 19. A.V. Stepanov, V.V. Zaitsev, and V.M. Nakariakov, Coronal Seismology, Wiley (2012), p. 48. 20. S.I. Braginskii, in: Reviews o fPlasma Theory, ed M.A. Leontovich, Vol. I, Consultants Bureau, New Yoik (1965). 70
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