2006
DOI: 10.1063/1.2188086
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Observation of a pressure limit in a gun-driven spheromak

Abstract: Density in a spheromak is lowered by action of a m∕n=2∕4 island, after which the electrons heat rapidly to give profiles of nTbefore=nTafter, indicating that the spheromak heats up to a pressure limit. The spheromak core remains at Te∼150eV for ∼1∕2ms during a period exhibiting low amplitude incoherent fluctuations consistent with a pressure-driven mode, giving the volume-averaged electron beta ⟨βe⟩∼3% and peak βe of ∼6%. Calculations show that measured pressure profiles are close to the Mercier limit.

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Cited by 6 publications
(5 citation statements)
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“…4b of Ref. 25. The corresponding a profile decreases radi-ally outwards from the magnetic axis and is comparable to optimized SSPX profiles, such as the reconstruction shown in Fig.…”
Section: Linear Analysis Of Straight Spheromak Equilibriasupporting
confidence: 77%
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“…4b of Ref. 25. The corresponding a profile decreases radi-ally outwards from the magnetic axis and is comparable to optimized SSPX profiles, such as the reconstruction shown in Fig.…”
Section: Linear Analysis Of Straight Spheromak Equilibriasupporting
confidence: 77%
“…This finding may be relevant to the apparent ideal-MHD -limit observed in SSPX discharges during periods when the safety-factor profile lies above 1/2. 25 A tendency for symmetry-breaking modes and reduced confinement in nonlinear resistive-MHD simulations of the quiescent phase of SSPX discharges has been noted in previous work, 33 and it is possible that consistent twotemperature extended MHD modeling would yield results that better represent the experiment's confinement properties.…”
Section: Discussionmentioning
confidence: 74%
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“…The configuration shown in figure 29 was found to be unstable to an n φ = 2, m = 4 mode at a peak β = 6% [64]. The high-frequency, magnetic fluctuation level also increased relative to that before the instability onset.…”
Section: Pressure Limit In a Large-aspect Ratio Spheromakmentioning
confidence: 92%
“…It is possible that an interchange mode is triggered which may have been seen in experimental observations on sawteeth [25]. It may also be possible that turbulent transport is increased so that the Mercier mode is held at marginal stability as observed in spheromaks by Woodruff et al [26]. Given that the Mercier criterion is violated only at some rational surfaces and that the drive for the instability is the pressure gradient it seems likely for rational surfaces in the core that the Mercier mode would result in enhanced turbulence which would hold the mode at marginal stability.…”
Section: Mercier Stabilitymentioning
confidence: 90%