2005
DOI: 10.1088/0029-5515/45/6/009
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Transition from weak to strong energetic ion transport in burning plasmas

Abstract: The change in nonlinear energetic particle mode (EPM) dynamics that accompanies the transition from weak to strong energetic ion transport is discussed in this work. It is demonstrated that the nonlinear threshold in fast ion energy density for the onset of strong convective transport occurring in avalanches is close to the linear EPM excitation threshold. This phenomenology is strictly related to the resonant character of the modes, which tend to be radially localized where the drive is strongest. After the c… Show more

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Cited by 90 publications
(197 citation statements)
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References 49 publications
(140 reference statements)
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“…Due to the intrinsic EPM resonant character and their locahzation at the radial position where the drive is strongest [48,49,50], EPMs rapidly redistribute energetic particles. Simulation results indicate that, above the hnear stability threshold, strong EPM induced fast ion transport occurs via processes that can be identified with the convective amplification of an unstable front, which coherently propagates in the radial direction as the fast ion energy density gradient (free energy source) steepens before it eventually relaxes [51]. Such strong transport events occur on time scales of a few inverse linear growth rates (generally 100 -200 AUven times, TA = RQ/VAO, with v^o the Allven speed on the magnetic axis evaluated at BQ) and have a ballistic character [52] that basically differentiates them from the diffusive and local nature of weak transport.…”
Section: A^ = {(0^/(oj){l-(0p/(o)[l+ (L6{ro/r)^^^ + 05^q^'^ mentioning
confidence: 97%
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“…Due to the intrinsic EPM resonant character and their locahzation at the radial position where the drive is strongest [48,49,50], EPMs rapidly redistribute energetic particles. Simulation results indicate that, above the hnear stability threshold, strong EPM induced fast ion transport occurs via processes that can be identified with the convective amplification of an unstable front, which coherently propagates in the radial direction as the fast ion energy density gradient (free energy source) steepens before it eventually relaxes [51]. Such strong transport events occur on time scales of a few inverse linear growth rates (generally 100 -200 AUven times, TA = RQ/VAO, with v^o the Allven speed on the magnetic axis evaluated at BQ) and have a ballistic character [52] that basically differentiates them from the diffusive and local nature of weak transport.…”
Section: A^ = {(0^/(oj){l-(0p/(o)[l+ (L6{ro/r)^^^ + 05^q^'^ mentioning
confidence: 97%
“…These functions are often assumed to weakly depend on time as well, although this is not strictly necessary. The panels from left to right refer to three subsequent times of the 3D Hybrid MHD-Gyrokinetic simulation discussed in [51], with the nonlinear evolution of the radial envelope of a single « = 4 EPM, shown as a function of the radial variable normahzed to the plasma minor radius a on top of the nonlinear distortion of the fast ion free energy source, SUH = -{^7t/Bl)Roq^{d/dr){PH-PH,eqmi), which is identically zero during the hnear unstable phase, where profiles are those given at eqmlibrium initial conditions. Particle radial transport in this case is secular due to coherent non-linear interactions with the modes.…”
Section: ^Mn{rt) =A"^"{t)0{nq{r)-mt) C:±a"{rt)^{nq{r)-mt)mentioning
confidence: 99%
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