Download presentation
Presentation is loading. Please wait.
Published byMaryann Leonard Modified over 9 years ago
1
D-Alpha Fast-Ion Diagnostic: Recent Results from DIII-D W.W. Heidbrink, UC Irvine D-Alpha Diagnostic: Yadong Luo, K. Burrell, + Ion Cyclotron Heating: R. Pinsker, C. Petty, P. Politzer, M. Murakami, + Fast-ion instabilities: R. Nazikian, M. van Zeeland, T. Rhodes, G. McKee, E. Fredrickson, E. Synakowski, + Diagnostic Concept Classical Fast-ion Distribution RF Acceleration Spatial Profile during Instabilities
2
THE FAST-ION DISTRIBUTION IS UNCERTAIN IN MOST AT DISCHARGES Nucl. Fusion 42 (2002) 972. Ad hoc diffusion model matches neutron rate. Introduces uncertainties in pressure and current profile control and analysis.
3
Bright Backgrounds: Injected, Halo, and Edge Neutrals What viewing geometry Doppler shifts the relatively dim fast-ion light away from these backgrounds?
4
Exploit gyro-motion: use a vertical view Notch filter blocks light from other neutrals (dynamic range) Beam modulation to subtract bremsstrahlung and edge impurity lines
5
Diagnostic Concept Demonstrated: 2003 data from a radial view PPCF 46 (2004) 1855. Fast-ion feature has expected temporal, spectral, and density dependencies. Signal weak at high density (>7x10 19 m -3 )
6
Atomic Physics Processes Neutralization depends on relative velocity between injected neutrals and fast ions. Intrinsic spatial resolution ~5 cm. Doppler shift determined by velocity component along line of sight. Stark broadening of minor importance
7
D Instrumentation for 2005 Campaign New dedicated 2-channel instrument with full spectra. 8 spatial CER channels with partial spectra (tuned to D sometimes)
8
Complications in the Interpretation of the Signal Ideally, the fast-ion density would be proportional to the signal, BUT … The injected neutral density depends on the beam deposition The Doppler shift depends on only one velocity component Impurity lines can contaminate the spectrum ELMs can complicate the background subtraction
9
“Boring” Shot with Classical Fast- ion Behavior
10
Spectra from Spatial Array in Quiet Plasma Signal visible from edge to center
11
Spatial Profile in Quiet Plasma Looks Reasonable Signal integrated from 40-80 keV and over 1.5 s. Geometrical corrections omitted.
12
Velocity-space weighting depends on pitch-angle scattering rate Competition between deceleration (T e ) and pitch- angle scattering (Z eff ) determines fraction of velocity space occupied by perpendicular ions
13
Quiet shot with T e Variation 50 keV perpen dicular neutrals
14
Expected Qualitative Dependence on Electron Temperature
15
No Prominent Contaminating Lines in Spectrum Single 1 ms spectrum Background subtraction works well for low charge states. CER lines for E>80 keV
16
Resumed High Harmonic Heating Experiments in 2005 60 MHz System Injected > 1 MW into L-Mode plasmas and ~0.6 MW into AT target. Studied beam-ion acceleration at 4 th -6 th harmonics 2 nd harmonic hydrogen acceleration (by accident!) 116 MHz System Injected ~ 2 MW into L-Mode plasmas Little beam-ion acceleration at 7 th and 8 th harmonic
17
Beam-ion Acceleration during 4 th harmonic heating
18
D Spectrum: Perpendicular Fast- ion Tail during 60 MHz ICH Tail spectrum symmetric--expected for perpendicular ions Spectrum altered at high energies (high harmonic heating) Signal increases 75% with RF Ions accelerated above injection energy Tail correlates with neutron enhancement
19
MANY FAST-ION INSTABILITY EXPERIMENTS WERE COMPLETED Many low-field and reversed shear experiments. New internal fluctuation diagnostics: BES, interferometers, FIR scattering, reflectometry. Fast-ion diagnostics: D-alpha, neutral-particle, neutrons, edge-loss. CAEs are common at low field. Cascade modes are common in reversed and weak shear.
20
“Nasty” Low-field shot with virulent internal kink activity
21
Bizarre Profile with Virulent Instabilities Preliminary: Need improved background subtraction
22
Fast-ion D-Alpha measurements are a very promising technique Technique works best for devices with ~30 keV/amu beams, modulation capability, modest densities, and size >> 5 cm (like DIII-D & NSTX). In quiet plasmas, deposition and T e dependence look reasonable. Need detailed analysis to confirm. Tail populations accelerated by ICRF are readily observed. Will compare with predicted acceleration. We measured fast-ion spatial profiles during CAE, Cascade, internal kink, ITB formation, and helical-field (ELM suppression) experiments. Hope to use internal instability measurements to compare with predicted fast-ion transport.
23
Alfven cascade modes (cylindrical modes at q min ) observed in DIII-D Barely visible on magnetics Clearly seen on internal diagnostics: FIR scattering, interferometers, BES, PCI. Driven by sub-Alfvenic fast ions at full field. Doppler shifts indicate high toroidal mode numbers. Cascade data assist in determination of q profile Nazikian et al., IAEA (2004). NEW FLUCTUATION DIAGNOSTICS
24
CAE ARE OBSERVED ON DIII-D: WILL THESE BE EXCITED IN ITER? Very similar to NSTX instabilities. Agrees qualitatively with CAE theory. Suggest alphas will drive CAE in ITER.
Similar presentations
© 2025 SlidePlayer.com. Inc.
All rights reserved.