2018
DOI: 10.1016/j.cpc.2018.04.018
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A simulation environment to simulate lower-hybrid-wave-driven plasmas efficiently

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Cited by 2 publications
(2 citation statements)
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“…where P f and G are now flux functions. By substituting (11), ( 1) is reduced to the standard Grad-Shafranov equation with thermal 'fast electron' contributions: P → P + P f and F → F + G. For the LH current drive application considered in this work, the pressure anisotropy was strong (P P ⊥ ), but the fast electron pressure contributions were small enough that they could be dropped altogether to reduce the model to standard MHD.…”
Section: Extended Mhd Equilibrium Reconstruction With Fast Electronsmentioning
confidence: 99%
See 1 more Smart Citation
“…where P f and G are now flux functions. By substituting (11), ( 1) is reduced to the standard Grad-Shafranov equation with thermal 'fast electron' contributions: P → P + P f and F → F + G. For the LH current drive application considered in this work, the pressure anisotropy was strong (P P ⊥ ), but the fast electron pressure contributions were small enough that they could be dropped altogether to reduce the model to standard MHD.…”
Section: Extended Mhd Equilibrium Reconstruction With Fast Electronsmentioning
confidence: 99%
“…The impact of collisionless fast particles on MHD equilibrium can be studied by considering an extended MHD model with a two-component plasma of bulk MHD fluid and kinetic fast particles [10]. The impact of LH driven fast electrons on MHD was first studied by performing a time-dependent, extended MHD simulation [11]. The work showed the possible importance of the fast electron current.…”
Section: Introductionmentioning
confidence: 99%