An advection-diffusion model for cross-field runaway electron transport in perturbed magnetic fields
arXiv:1606.04409 · doi:10.1088/0741-3335/58/12/125017
Abstract
Disruption-generated runaway electrons (RE) present an outstanding issue for ITER. The predictive computational studies of RE generation rely on orbit-averaged computations and, as such, they lack the effects from the magnetic field stochasticity. Since stochasiticity is naturally present in post-disruption plasma, and externally induced stochastization offers a prominent mechanism to mitigate RE avalanche, we present an advection-diffusion model that can be used to couple an orbit-following code to an orbit-averaged tool in order to capture the cross-field transport and to overcome the latter's limitation. The transport coefficients are evaluated via a Monte Carlo method. We show that the diffusion coefficient differs significantly from the well-known Rechester-Rosenbluth result. We also demonstrate the importance of including the advection: it has a two-fold role both in modelling transport barriers created by magnetic islands and in amplifying losses in regions where the islands are not present.
References in corpus (4)
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- Energetic electron transport in the presence of magnetic perturbations in magnetically confined plasmas
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Cited by in corpus (8)
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- Runaway electron deconfinement in SPARC and DIII-D by a passive 3D coil
- Effects of magnetic perturbations and radiation on the runaway avalanche
- Assessing energy dependence of the transport of relativistic electrons in perturbed magnetic fields with orbit-following simulations
- A fluid-kinetic framework for self-consistent runaway-electron simulations
- Runaway electron modelling in the self-consistent core European Transport Simulator, ETS
- The impact of fusion-born alpha particles on runaway electron dynamics in ITER disruptions
- Modeling the complete prevention of disruption-generated runaway electron beam formation with a passive 3D coil in SPARC