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Status of EBW Emission Analysis on NSTX. S.J. Diem July 20th, 2006. XP 625: B-X-O Mode Conversion Physics at 8-40 GHz. Study 8-40 GHz thermal EBW emission via oblique B-X-O coupling Use remotely-steered, quad-ridge antennas and dual-channel radiometry at Bay G
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Status of EBW Emission Analysis on NSTX S.J. Diem July 20th, 2006
XP 625: B-X-O Mode Conversion Physics at 8-40 GHz • Study 8-40 GHz thermal EBW emission via oblique B-X-O coupling • Use remotely-steered, quad-ridge antennas and dual-channel radiometry at Bay G • Study behavior of EBWs emitted from the fundamental, 2nd and 3rd harmonic emission from L-mode and H-mode plasmas • Experiment had three objectives: • Map coupling efficiency as a function of antenna pointing direction and compare to theory • Analyze emission polarization and compare to theory • Measure Te(R,t) using thermal EBW emission
Upgraded EBW antennas allow spatial mapping of emission window • Fundamental (8-18 GHz) • 2nd and 3rd harmonic (18-40 GHz) AORSA-1D NSTX = 40% Bt(0) = 3.5 kG f = 28 GHz M. Carter ORNL • Motors allow for ±10 degrees of motion in poloidal and toroidal directions • Fundamental beam waist radius ~ 11° at plasma edge • Harmonics beam waist radius ~ 7 ° at plasma edge Beam waist >90%
Strong fundamental emission observed during L-mode scan Fundamental emission • 800 kA plasma • Te(0)~1.6 keV • Window losses not included Reflectometer signal
L-mode harmonic emission lower than fundamental Reflectometer signal
Spatial scan provides good coverage of emission windows *Window losses not included in mode conversion efficiency calculation
L-mode polarization measurements • Polarization of maximum emission ~1.7 • Polarization varied from 1.25-1.7
Te(R) profile from emission data Thomson data 1.1 600 Ray damping location from GENRAY 500 1.05 Radius [m] 400 Te [eV] 1.0 300 Te (R) from EBW 200 0.95 95 100 105 110 Radius [cm] 12 13 14 15 16 Frequency [GHz]
H-mode emission much lower than L-mode Fundamental emission • 1 MA plasma • Te(0)~1 keV • Window losses not included Reflectometer signal
H-mode spatial scan provides coverage of emission window *Window losses not included in mode conversion efficiency calculation
H-mode polarization measurements • Maximum polarization of 1.7 for peak emission shot • Other polarization measurements varied from 1.2-1.5
Emission level not strongly correlated with Te at UHR 40 40 L-mode 1200 30 20 Te at UHR [eV] 800 Trad [eV] Te at UHR [eV] 20 0 400 10 0.6 0.8 0.4 0.2 1.0 0 Time [s] 0 0.2 0.0 0.6 0.4 300 Time [s] 14 25 400 250 20 10 200 300 Te at UHR [eV] 15 Trad [eV] Te at UHR [eV] 150 Trad [eV] 200 6 10 100 100 5 50 2 0 0 0 0 0.8 0.4 0.2 0.6 1.0 0.0 0.0 0.8 0.4 0.2 0.6 1.0 Time [s] Time [s]
Harmonic emission much lower than 2005 campaign 120 80 Te at UHR [eV] 40 0 0.0 0.2 0.4 1.0 0.6 0.8 Time [s] 200 117982, H-mode (2005) 40 150 30 Trad [eV] 100 Te at UHR [eV] 20 50 10 0 0 0.0 0.8 0.4 0.2 0.6 1.0 Time [s]
Density scale length larger in some H-modes 20 • Ln obtained with Thomson data factor of 2 less than reflectometer data • LnH-mode ≥ LnL-mode • Mode conversion region outside H-mode pedestal • Higher fluctuations in LnH-mode 15 Ln 10 5 0 0.0 0.2 0.4 0.6 0.8 1.0 Time [s] 5 10 4 8 Ln Ln 3 6 2 4 0.6 0.8 0.2 0.4 0.6 0.8 0.4 0.2 Time [s] Time [s]
Future Work • Complete calibrations (including vacuum window) • More accurate mode conversion efficiency map • Previous ray-tracing relied on direct launching of EBW • B-X-O mode coupling and emission packages in GENRAY may provide more accurate results • Use J. Preinhaelter’s code to model H-mode emission • Analysis of gas puffing experiments • Analysis of TF ramping experiments • Correlation analysis of Ln and emission data • Complete upgrades for 2007 run campaign • Design XP for 2007 run to investigate low H-mode emission