The resonant magnetic perturbation (RMP) is one of powerful means to mitigate or control ELMs and thus eliminate transient substantial heat loads on plasma facing components. However, one tradeoff for this benefit is that the RMP probably causes a higher power threshold for the LàH transition. Motivated by this, we present a new mean field model including stochastic magnetic field effect which may explain the increased LàH power threshold.
The model consists of coupled equations for mean radial electric field, poloidal rotation, toroidal rotation, density ion temperature and turbulence intensity. Novel features include a Maxwell stress on poloidal rotation
Vθ
induced by the stochastic magnetic field. This tends to work against
Vθ
, since it has the same phase as, but sign opposite to, the Reynolds stress. The effect of Maxwell stress on
Vφ
can induce force through radial current across separatrix and reverse the toroidal rotation on the stochastic layers. Stochastic magnetic fields induce a non-diffusive, parallel flow gradient driven particle flux, which may explain RMP-induced pump-out. In addition, stochastic magnetic fields can degrade the coherence of
Vr
and
Vθ
in the Reynolds stress, thus weakening the LàH trigger mechanism. Finally, stochastic fields necessarily carry a portion of the ion heat flux.
Results so far indicate that
brbθ≠0
breaks ambipolarity, so both amplitude and
profile of
br2
are significant,
Jr
(induced by
brbθ
) drives an intrinsic toroidal torque,
V'E
ensures that
brbθ
opposes
VrVθ
, and that
br2
can modify
Ti
and
n
profiles. The dimensionless parameter that quantifies the increment in power threshold is identified as α≡[
br2q]/(ρ*2βϵ)
and this is used to assess the impact of stochastic field on the L-H transition. Results indicate that the routine RMP strength of
br~10-4
is sufficient to inhibit the transition. Ongoing work is concerned with quantifying power threshold dependencies. Both a 0-D and 1-D numerical solutions of the model are ongoing.