Global Alfvén eigenmodes in the H-1 heliac
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Hole, Matthew
Blackwell, B D
Bowden, G
Cole, M
Könies, A
Michael, Clive
Zhao, F
Haskey, S R
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IOP Publishing
Abstract
Recent upgrades in H-1 power supplies have enabled the operation of the H-1 experiment at higher
heating powers than previously attainable. A heating power scan in mixed hydrogen/helium plasmas
reveals a change in mode activity with increasing heating power. At low power (<50 kW) modes
with beta-induced Alfvén eigenmode frequency scaling are observed. At higher power modes
consistent with an analysis of nonconventional global Alfvén eigenmodes (GAEs) are observed, the
subject of this work. We have computed the mode continuum, and identified GAE structures using
the ideal MHD solver CKA and the gyrokinetic code EUTERPE. An analytic model for ICRHheated
minority ions is used to estimate the fast ion temperature from the hydrogen species. Linear
growth rate scans using a local flux surface stability calculation, LGRO, are performed. These studies
demonstrate drive from the radial spatial gradient of circulating particles whose speed is significantly
less than the Alfvén speed, and are resonant with the mode through harmonics of the Fourier
decomposition of the strongly shaped heliac magnetic field. They reveal drive is possible with a small
(nf n0 < 0.2) hot energetic tail of the hydrogen species, for which Tf > 300 eV. Local linear
growth rate scans are also complemented with global calculations from CKA and EUTERPE. These
qualitatively confirm the findings from the LGRO study, and show that the inclusion of finite Larmor
radius effects can reduce the growth rate by a factor of up to ten, and increases the marginal stability
fast ion temperature by a factor of two. Finally, a study of damping of the global mode with the
thermal plasma is conducted, computing continuum damping , and the damping arising from finite
Larmor radius and parallel electric fields (via resistivity). We find that continuum damping is of order
0.1% for the configuration studied. A similar calculation in the cylindrical plasma model produces a
frequency 35% higher and a damping 30% of the three-dimensional result: this confirms the
importance of strong magnetic shaping to the frequency and damping. The inclusion of resistivity
lifts the damping to g w = -0.189. Such large damping is consistent with experimental
observations that in absence of drive the mode decays rapidly (∼0.1ms).
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Plasma Physics and Controlled Fusion
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