1999
DOI: 10.1063/1.873550
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Spontaneous hole–clump pair creation

Abstract: Numerical simulations and quantitative theoretical explanations are presented for the spontaneous formation of a hole–clump pair in phase space. The equilibrium is close to the linear threshold for instability and the destabilizing resonant kinetic drive is nearly balanced by either extrinsic dissipation or a second stabilizing resonant kinetic component. The hole and clump, each support a nonlinear wave where the trapping frequency of the particles is comparable to the kinetic linear growth rate from the dest… Show more

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Cited by 142 publications
(203 citation statements)
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“…However, in the theory proposed by Berk, Breizman, and Petviashvili [36][37][38] for the spontaneous generation of hole-clump pairs, albeit for a one-dimensional ͑1-D͒ bump-on-tail resonant interaction, would predict exactly this type of behavior. In this theory, the nonlinear interaction of a marginally unstable resonant mode with a collisionless, inverted fast-particle distribution results in the splitting of the mode frequency, and upward and downward frequency chirping as the "holes" and "clumps" formed in the distribution function propagate in particle phase space.…”
Section: Compressional and Global Alfvén Modesmentioning
confidence: 99%
“…However, in the theory proposed by Berk, Breizman, and Petviashvili [36][37][38] for the spontaneous generation of hole-clump pairs, albeit for a one-dimensional ͑1-D͒ bump-on-tail resonant interaction, would predict exactly this type of behavior. In this theory, the nonlinear interaction of a marginally unstable resonant mode with a collisionless, inverted fast-particle distribution results in the splitting of the mode frequency, and upward and downward frequency chirping as the "holes" and "clumps" formed in the distribution function propagate in particle phase space.…”
Section: Compressional and Global Alfvén Modesmentioning
confidence: 99%
“…In addition, chaotic solutions can display shifting of the mode frequency ͑chirping͒, both upwardly and downwardly, as pairs of hole and clump are formed in the distribution. [8][9][10] On the one hand, theories have been developed by Berk et al 6,[8][9][10][11] to predict the quantitative behavior of such instabilities in various parameter regimes and explain underlying mechanisms. The validity of some of these theories has been tested by numerical simulations based on a reduced model solving only resonant particles with adiabatic and cold bulk plasmas.…”
Section: Introductionmentioning
confidence: 99%
“…9 The ratio of the linear damping rate ␥ d to the linear growth rate ␥ L in the simulation is consistent with hole-clump pair creation which takes place when ␥ d / ␥ L is greater than 0.4. 10,11 In this paper, we focus on the linear properties of the unstable mode. In Ref.…”
Section: Introductionmentioning
confidence: 99%