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Fast Probe Results and Plans. By J. Boedo For the UCSD and NSTX Teams. Probe Installed and Commissioned. Location is 6/8” below midplane. 11 deg angle. 6.8”. New head and tips to accommodate curvature and heat flux. Thermal Conductivity Thermalgraph Tips (parallel) 800 W/mK
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Fast Probe Results and Plans By J. Boedo For the UCSD and NSTX Teams J. Boedo, UCSD
Probe Installed and Commissioned Location is 6/8” below midplane 11 deg angle 6.8” J. Boedo, UCSD
New head and tips to accommodate curvature and heat flux Thermal Conductivity Thermalgraph Tips (parallel) 800 W/mK Copper 401 W/mK POCO graphite 72 W/mK J. Boedo, UCSD
Existing Probe Head has 10 Tips • Tips in blue will be active on day one, the rest implemented as upgrades (if funded) • Fluctuations to 1 MHz • Two Vf tips used for Epol (and fluctuations) • Two Vf tips used as Er (and fluctuations) >> Reynolds Stress • One tip as Isat >> ne • Two tips as double probe (Te and Ne profiles) Vf1 Epol Isat Vf2 Er Vf3 Vf4 Te fluct Bt Mach1 Double Probe Mach2 J. Boedo, UCSD
Data Taken at High Spatial and Temporal Resolution Insertion completed in 100 ms. ~30 ms in plasma Time resolution for Te and Ne is 1 ms Time resolution for fluctuations is 1 micro sec Spatial resolution is 1.5-2 mm (tip size + probe motion) J. Boedo, UCSD
Within the limited shot space, density and power were varied. So scaling is inconclusive • So far: • decreases in H mode with power 2.5>1.5 cm • Will obtain wider operating space in the future and produce scalings J. Boedo, UCSD
H-mode Radial Electric Field Flat in SOL J. Boedo, UCSD
Fluctuation Quantities to Characterize in NSTX Need to add Te fluct capability J. Boedo, UCSD
Harmonic Diganostic Probe V R1 Ampli- tude detector Amp C1 C3 fdrive= 400 kHz R2 V_fast I C2 400 kHz Bandpass filter Ampli- tude detector Pearson coil Amp Amp 250 W RF amp I2 800 kHz Bandpass filter Ampli- tude detector Amp Amp I_fast Dummy transmission line I_min V_min I /I2 Analog divider Compa- rator Compa- rator Adder Tunable LPF Analog multiplier Ref Ref Analog multiplier Te_slow J. Boedo, UCSD
Harmonics Technique Current to a DC-floating probe driven by sinusoidal voltage can be expressed as a series of sinusoidal harmonics [1]: where - amplitude of mth harmonic - Bessel functions of integer order k For eU0/kTe << 1: Thus Te can be determined from the ratio of the amplitudes of 1st and 2nd harmonics The error of this approximation for eU0/kTe= 1 is only about 5% [1] [1] Boedo et al,Rev. Sci. Instrum.70 (1999), 2997 J. Boedo, UCSD
Need to Include Magnetic component Particle Flux Reynolds Stress (neglecting ion pressure fluctuations) Heat Flux Parallel Current Flux Helicity Flux J. Boedo, UCSD
Normalized N fluctuations very large J. Boedo, UCSD
Radial Turbulent Flux Lower in H-mode Value is ~3-5 1017 cm-2 s-1 J. Boedo, UCSD
Intermittent Plasma Events Pervasive J. Boedo, UCSD
Power Spectrum Comparison Power spectrum vs f (in kHz) from probe data during gas injection (solid circles) and without(x) and comparison to that obtained form the GPI system (open circles). Note that the power spans y 4 orders of magnitude indicating excellent S/N ratio. J. Boedo, UCSD
Intermittency (Radial Convective Transport) Lower in H-Mode L-Mode 109033 H-Mode 109052 Intermittency is very strong in NSTX! J. Boedo, UCSD
Intermittency (Radial Convective Transport) Lower in H-Mode L-Mode 109033 H-Mode 109052 Intermittency is very strong in NSTX! J. Boedo, UCSD
L-Mode 109033 Density is highly intermittent Rate of bursts is ~1E4 Poloidal field is much less intermittent Coherent modes show in Etheta Instantaneous flux is 1-3E15 cm-2s-1 J. Boedo, UCSD
H-Mode 109052 Density is intermittent (ELMs?) Rate of bursts is 2E3 Poloidal field is much less intermittent Coherent modes show in Etheta Instantaneous flux is ~2E15 cm-2s-1 J. Boedo, UCSD
Initial Reynolds Stress and Bicoherency Measurements H-Mode Codes Written and Tested L-Mode J. Boedo, UCSD
Bispectrum H-mode L-Mode f3=f1+f2 f3=f1-f2 J. Boedo, UCSD
Bicoherency H-mode L-Mode J. Boedo, UCSD
Profile Conclusions • Edge/SOL profiles available with high spatial (2-2.5 mm) resolution • Limited to 1086xx, 1089xx, 109032-109062 • Fully calibrated data for 109032-xxx062 • NSTX profiles seem different from larger aspect ratio devices • Te profile in the edge/SOL is flat at 25-30 eV • Ne profile has a very long decay length. Reduced by power! • H-mode Er profile flat in SOL • How do flat Te profiles are maintained? • Do we have (more) anomalous radial transport? (intermittency) • Adding fast Te diagnostic J. Boedo, UCSD
Future Work and Goals • Data obtained in L and H-mode. SOL length scales with power. Ongoing • Many puzzles need addressing • Features usually associated with LCFS vicinity are different in NSTX, such as a potential well, steep H-mode profiles, etc Ongoing • Intermittency is quite strong in NSTX (very strong radial transport?) • Need to quantify electrostatic turbulence and Intermittency (enough to explain strong transport?) Codes just ported for electrostatic turbulence, ongoing for intermittency! • Bicoherency and Reynolds Stress codes just finished. Investigate energy cascading and self-organized flows • Need to quantify electromagnetic components of transport • Upgraded head partially designed and to be built in FY04 J. Boedo, UCSD