2011
DOI: 10.1134/s0021364011090025
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Quasistationary magnetic field generated in a plasma by a whistler-mode radio pulse

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Cited by 6 publications
(2 citation statements)
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“…Laboratory setups based on mirror plasma traps are actively used to simulate nonlinear wave-particle interactions in space plasmas [1][2][3][4][5][6][7][8][9][10][11]. In particular, we have reported previously in [12] that a new regime of electron-cyclotron instability has been revealed in a compact axisymmetric mirror trap (the magnetic field in the mirrors is B max = 1.8 T, the distance between the mirrors is 25 cm, the mirror ratio B max /B min = 5) during the plasma decay.…”
Section: Introductionmentioning
confidence: 99%
“…Laboratory setups based on mirror plasma traps are actively used to simulate nonlinear wave-particle interactions in space plasmas [1][2][3][4][5][6][7][8][9][10][11]. In particular, we have reported previously in [12] that a new regime of electron-cyclotron instability has been revealed in a compact axisymmetric mirror trap (the magnetic field in the mirrors is B max = 1.8 T, the distance between the mirrors is 25 cm, the mirror ratio B max /B min = 5) during the plasma decay.…”
Section: Introductionmentioning
confidence: 99%
“…For this reason, the effects of thermal nonlinearity were not developed and f m 1 -the observed cross modulation was most likely due to nonlinearity caused by the averaged ponderomotive force in the spatially inhomogeneous high frequency pump field. It was experimentally shown in [15,16] that the averaged ponderomotive force in the magne tized plasma can result, on one hand, in perturbations of the density and magnetic field owing to the striction effect and, on the other hand, in the generation of closed drift currents perturbing the ambient magnetic field without the modulation of the density. The plasma redistribution rate is limited by the speed of sound, whereas the generation of perturbations of the magnetic field is a fast process.…”
mentioning
confidence: 98%