xp935: search for multiple rwm behavior at high b n

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NSTX XP935 initial summary - S.A. Sabbagh XP935: Search for multiple RWM behavior at high N Goals Determine if unstable RWM is born from observed, stable RWM (with at peak resonant field amplification – XP931), or a 2 nd mode Either result is important: If same mode, supports single mode physics model; key conclusion for RFA control of NBI (future milestone) If second mode, supports multi-mode theory, PRL-level conclusion, key conclusion for RWM control in ST, also, key conclusion for RFA control of NBI Determine N dependence of RFA for these modes near marginal stability Determine effect of on both modes as marginal stability approached Determine effect of active n = 1 control for these modes near marginal stability Status Scan in normalized beta completed, now with MSE data Notable: six shots with N > 6, reduce I p = 0.52 MA reached N = 7.2 co-rotating 30Hz seed fields appear to be amplified more strongly than counter, consistent with RFA – several long-pulse (~ 1.3s) shots with RFA seed fields ~ 30 Hz activity was shown to increase in radial extent as N increased The observed growing RWM appears to be independent of the 20 - 30 Hz activity

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XP935: Search for multiple RWM behavior at high b N. Goals Determine if unstable RWM is born from observed, stable RWM (with w at peak resonant field amplification – XP931), or a 2 nd mode : Either result is important: - PowerPoint PPT Presentation

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Page 1: XP935: Search for multiple RWM behavior at high  b N

NSTX XP935 initial summary - S.A. Sabbagh

XP935: Search for multiple RWM behavior at high N

• Goals Determine if unstable RWM is born from observed, stable RWM (with at peak

resonant field amplification – XP931), or a 2nd modeEither result is important:

• If same mode, supports single mode physics model; key conclusion for RFA control of NBI (future milestone)

• If second mode, supports multi-mode theory, PRL-level conclusion, key conclusion for RWM control in ST, also, key conclusion for RFA control of NBI

Determine N dependence of RFA for these modes near marginal stability

Determine effect of on both modes as marginal stability approached Determine effect of active n = 1 control for these modes near marginal stability

• Status Scan in normalized beta completed, now with MSE data

• Notable: six shots with N > 6, reduce Ip = 0.52 MA reached N = 7.2

co-rotating 30Hz seed fields appear to be amplified more strongly than counter, consistent with RFA – several long-pulse (~ 1.3s) shots with RFA seed fields

~ 30 Hz activity was shown to increase in radial extent as N increased The observed growing RWM appears to be independent of the 20 - 30 Hz

activity