VARIABLE REPETITION RATE THOMSON SCATTERING SYSTEM FOR THE GLOBUS-M TOKAMAK

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VARIABLE REPETITION RATE THOMSON SCATTERING SYSTEM FOR THE GLOBUS-M TOKAMAK S.Yu.Tolstyakov, V.K.Gusev, M.M.Kochergin, G.S.Kurskiev, E.E.Mukhin, Yu.V.Petrov, G.T.Razdobarin A.F. Ioffe Physico-Technical Institute St. Petersburg, Russia

Presentation outline What is the diagnostics aims? How it can be succeeded? What are results? What are the next steps? Conclusions

What is the diagnostics aims? Plasma stability Auxiliary heating by NBI Auxiliary heating by ICR Plasma fuelling with pellet injection Plasma fuelling with plasma gun

Requirements to diagnostics Time: To cover whole discharge duration To study fast transient process <1ms Multipulse laser: Pulse train duration up to 100ms Repetition rate more 1kHz Space: To cover all plasma A set of spectral devices Data: High accuracy Online System with low light losses Sensitive detector Flexible software Cost: Reasonable frame?

Acceptable options Nd:glass laser: Pulse train of reasonable number of pulses (to cover whole discharge duration) Time spacing and amplitude could vary in the wide range Spectral devices: High throughput filter polychromators Detectors: Digitizer: High sensitive avalanche photodiodes Low noise amplifiers 40Ms/s, 12bits, multichannel

General layout NBI RF preionization 3-channel D α plasma position control NPA TS Nd multipulse laser Tokamak chamber Basic laser Impurity lines monitor SXR Microwave refractometer Beam trap ICRH antenna TS spectrometers

Variable repetition rate laser Optical scheme 5 7 4 3 1 2 6 1- slab Nd:glass active element, 2, 3 master oscillator cavity reflector, 4- electro-optical shutter, 5,6- cylindrical reflectors of double pass optical arrangement, 7- beam dump,

Performance Compact design with joint in a common slab active element Reduced number of optoelectronic units Low pumping energy Target specifications of the laser model Laser operational mode Extreme Routine Pumping energy, kj/pulse Output, J/pulse Number of train pulses Pulses time spacing range, sec Laser pulse duration, nsec Beam divergence, rad Wavelength, nm 3.1 12 20 0.3 10-3 0.3 30 ~10-3 1055 1.3-1.8 1.5-3 20 0.5 10-3 0.3 30 ~10-3

Laser temporal possibility Pumping energy 1.5kJ Pulse repetition rate 1kHz 10Hz 5J Pulse energy reproducibility in pulse repetition operation mode Pumping energy 1.35kJ 30msec 20msec 500Hz 2kHz 500Hz 2kHz 660Hz 2kHz

TS filter spectrometers 1,2 60 80 1,0 50 Transmission, % 60 40 20 1500eV 800eV 500eV 300eV 0,8 0,6 0,4 0,2 δ T e /T e, arb.un. 40 30 20 10 0 0,0 850 900 950 1000 1050 Wavelength, nm 0 500 1000 T e, ev

Photodetectors PMT PD APD Advantages Disadvantages High amplification Bigscale photocathode Relatively low cost Low quantum efficiency High voltage power supply High sensitivity to B r High quantum efficiency Low sensitivity to B r Simple operation Low cost Extremely low noise amplifiers are needed High quantum efficiency High amplification Low sensitivity to B r High cost Excess noise factor >2 Temperature instability

Signal detection and processing APD detectors noise I FM noise = τ e The 30ns-TS signal -> very high speed ~1Gs/s extremely expensive digitizer Economically sound ADCs 40Ms/s 12bits ADC -> pulse elongation up to 250ns. Respective sacrifice of sensitivity ~3 counterbalanced by: increased laser pulse energy (up to 3J) big collection angle (~1/7) high throughput of polychromators (~80%) high APD sensitivity (80-40% for different wavelength)

Signal detection and processing The correct signal recognizing under the noise presence RMS-fitting to the no-noisy reference signal. 250ns Averaging over 20 pulses RMS-fit

Calibration Spectral calibration employing of compact scanning monochromator MDR-206 (routine procedure) Verification- scattered light simulation Absolute calibrations - Raman scattering in nitrogen for the sensitivity coupling of polychromator array; their absolute sensitivities derived using the data of microwave interferometer

Multi-purpose software Drive over the all laser parameters (to set the pulse train temporal scenario, pulse energy and many others) Perform calibration Reconstruct TS signal Proceed data with resulting temporal/spatial distribution of n e, T e online

-HIGH LEVEL OF BACKGROUND Complications plasma light increased in spherical tokamaks -HIGH LEVEL OF STRAY LIGHT Globus-M: Polished inner walls Intimacy wall and plasma border

Complications mitigation High contrast filters (Barr Associates) Notch filter (SPb product) (one spatial point) High transparent polarizer Laser wavelength stabilization using Fabri-Perot interferometer

Results Measurements: Low and high densities regimes Greenwald density limit is overcame With plasma gunfast and deep jet penetration Auxiliary heating NBI valuable increasing of electron energy content

What are the next steps? Light trap on the central column Increasing of spatial channels number New digitizers 500Ms/s and fast amplifiers New observation port New collection optics- achromatic objective and fibers

What are the next steps? Proposed Nowadays observation geometry Measurements from inner to outer plasma border Scattering angle increasing for outer border results in TS spectrum broadening Achromatic objective + fibers strongly simplify alignment of collection optics Possibility to easily spread spatial points over major radius Using of more reliable window protection

Conclusions TS system based on variable repetition rate Nd-glass laser has been designed and built The use of high throughput filter polychromators, low noise detection and dedicated software meets the planned scientific and technical objectives of the Globus-M program The extensive investigations of auxiliary heating, plasma transients and fuelling by jet injection has been performed