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Berk, H.L.; Breizman, B.N.; Petviashvili, N.V.
Texas Univ., Austin, TX (United States). Inst. for Fusion Studies. Funding organisation: USDOE Office of Energy Research, Washington, DC (United States)1997
Texas Univ., Austin, TX (United States). Inst. for Fusion Studies. Funding organisation: USDOE Office of Energy Research, Washington, DC (United States)1997
AbstractAbstract
[en] A numerical simulation of a kinetic instability near threshold shows how a hole and clump spontaneously appear in the particle distribution function. The hole and clump support a pair of Bernstein, Greene, Kruskal (BGK) nonlinear waves that last much longer than the inverse linear damping rate while they are upshifting and downshifting in frequency. The frequency shifting allows a balance between the power nonlinearly extracted from the resonant particles and the power dissipated into the background plasma. These waves eventually decay due to phase space gradient smoothing caused by collisionality
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Mar 1997; 15 p; IFSR--780; CONTRACT FG03-96ER54346; Also available from OSTI as DE97005050; NTIS; US Govt. Printing Office Dep
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