The details of point source helicity injection as a noninductive startup technique must be characterized:

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The details of point source helicity injection as a noninductive startup technique must be characterized: Is energy confinement dominated by cross-field transport? Is energy confinement dominated by parallel losses (stochastic field lines)? What is the effect of resistively-driven helicity dissipation? Develop a Thomson scattering diagnostic for the PEGASUS Toroidal Experiment to aid this characterization: Measure scattered light from incident Nd-YAG laser (λ laser =1064 nm) Light detected by a polychromator system Measure n e ~10 19 m -3 and Te ~ 10 ev 1 kev 10 radial locations, radial resolution ~1.75 cm (fine) and 5 cm (coarse)

Thomson scattering can help diagnose unique physics on Pegasus: n e and T e profiles during Taylor relaxation of non-solenoidally generated tokamak-like plasmas Characterization of resistively-driven helicity dissipation High β T, I p /I TF plasmas Phenomenological scales guide effective diagnostic design Scattering cross-section guides minimum etendue, detector choice, etc Non-inductive scale lengths minimum spatial resolution Individual components of MPTS system are strongly coupled

Equilibrium Field Coils" Vacuum Vessel" High-stress Ohmic " heating solenoid" Experimental Parameters Parameter A R(m) I p (MA) I N (MA/m-T) RB t (T-m) κ τ shot (s) β t (%) P HHFW (MW) Achieved 1.15 1.3 0.2 0.45.21 6 12 0.06 1.4 3.7 0.025 25 0.2 Goals 1.12 1.3 0.2 0.45 0.30 6 20 0.1 1.4 3.7 0.05 > 40 1.0 RF Heating Antenna" Toroidal Field Coils" Major research thrusts include:! Non-inductive startup and sustainment! Tokamak physics in small aspect ratio:! - High-I N, high-β operating regimes! - ELM-like edge MHD activity`! Ohmic Trim Coils" Plasma Limiters"

Open field line current M = G Injected current perturbs vacuum magnetic field Dynamics underlying Taylor relaxation will be characterized Use shot-to-shot scans with Thomson scattering to obtain detailed n e and T e profiles Tokamak-like plasma M > G Plasma expands inwards to fill the volume while connected to guns

Total helicity in a tokamak geometry:" K = V ( A + A vac ) ( B B vac ) d 3 x dk dt = 2 V ηj B d3 x Resistive Helicity Dissipation 2 ψ t Ψ 2 A ΦB ds πe 2 m 1/ 2 3 E = ηj η ( ) (Spitzer) 4πε 0 ( ) 2 ( kt e ) ln 12πnλ 3 / 2 D Use Thomson scattering to quantify T e and n e AC Helicity Injection: DC Helicity Injection: K AC = 2 ψ t Ψ = 2V loop Ψ K DC = 2 A ΦB ds = 2V inj B A inj

Using helicity startup Pegasus can access I N > 5 at I p ~ 0.2 MA As facilities are upgraded, expect to challenge the Troyon limit Explore confinement and temperature distributions in these regimes unique to Pegasus

VPH transmission dispersion grating Spectrometer exit lens APD detectors & electronics to digitizers Thomson scattering = scattering of EM radiation from free electrons assumes hν << mc 2 here, assume incoherent scattering (k inc λ D >> 1) Spectrometer entrance lens Fiber optic bundle (one spatial channel) Small scattering cross-section necessitates high-energy incident light (i.e. laser) dp = r 2 dω e sin 2 2 φcε 0 E i s Collection lens Beam steering mirror Scattered light Beam dump Collection lens & fiber bundles provide spatially resolved measurements Frequency bandwidth of the scattered light is proportional to T e Dispersion grating used to measure Δν = c/δλ Plasma Small signal levels dictate highsensitivity, fast detection electronics (ex. APD and fast digitizers) Nd:YAG laser

Preliminary calculations yield scattered intensities of ~8*10 5 total photons Assumes incoherent, nonrelativistic scattering Assumes 2J, 10 ns Nd-YAG laser pulse Assumes solid angle of ~0.01 ster per channel For system with 8 spectral channels, ~10 5 photons incident on APD detector (lossless optics) Since Pegasus shot times are ~30 ms, will only be able to measure one laser pulse Symbol: Inputs: E laser Laser output energy (J) 2! laser Laser wavelength,! m (m) 1.06E-06 n e Electron density (m -3 ) 1.00E+19 l Length of beam for one channel (m) 0.014 " Solid angle subtended by optics 0.01 Pulse duration (s) 0.00000001 Output: I det Number of photons incident 79310.77615 Joules incident at primary wavelength 1.482E-14 Watts at primary wavelength 1.48E-06

Pegasus plasmas typically 100 ev < T e < 1 kev Increased spectral resolution needed for low temperatures: T e = 100eV ~ 5 nm/ch T e = 1000eV ~ 40 nm/ch If possible, 8 spectral bins used to define lower-half Gaussian in each case!"#$%&%'()*+%&(,-./( 86%*&%9"#2(:"#$%&%'(;*+%&(<*&(=>(%?(@(8 % (@(=A%?( *"!!#$')% '!%-.% )"&!#$')% &!%-.% '!!%-.% )"!!#$')% &!!%-.% ("&!#$')% '!!!%-.% /0123-04%567-8-094:% ("!!#$')% '"&!#$')% '"!!#$')% &"!!#$'(%!"!!#$!!% +&!"!%,!!"!%,&!"!% '!!!"!% '!&!"!% ''!!"!% ''&!"!% '(!!"!% '(&!"!%!"#$%&%'(0#1%2%3456(,37/( Based on: J. Sheffield, Plasma Phys., Vol 14, 783-791 (1972) Predictions assume 90 average scattering angle with ~10-2 solid angle Relativistic effects evident in shift of central wavelength at T e = 1 kev

Subassemblies include: 3 5 1) Laser & laser room 2) Beamline housing 3) Beam Dump 4) Viewing Dump 4 2 5) Collection Optics 6) Fiber Optics & spectrometers 7) Data Acquisition 8) Control Code & SCRAM systems interface 7 6 1 8 9) Safety Overall

Specification Value Determining factors Output Energy 2000 mj Scattered intensity fraction Divergence 0.5 mrad Pointing stability 50 µrad Beam line Desired spatial resolution, component damage thresholds Pulse length 10 ns Availability at desired power Repetition Rate 10 Hz Shot duration; availability Jitter 500 ps Time resolution Beam diameter 8 15 mm Availability Polarization ratio 90% Scattering dependence Energy stability ± 2 % Availability; repeatability; Intensity resolution Identify tolerable limits due to physics needs and layout constraints Reliable, turn-key operation of laser desired Nd:YAG used extensively for MPTS in plasmas Operate in steady-state firing mode to obtain maximum stability Implement design with consideration for possible future upgrades: Additional spatial points Multiple laser passes Multiple time points per shot

F/2 optics Off-the-shelf 2 dia. VPH gratings available from Edmund Optics Simple off-the-shelf PCX lenses (Newport) used for modeling Revise to reduce chromatic aberrations for final design from Edmund Optics, informal communications

At low temperatures, need high spectral resolution (~5nm/ch) Implies use of higher dispersion grating for given image plane size, ex. 1200 l/mm At high temperatures, need lower spectral resolution Implies use of low dispersion grating for given image plane size, ex. 600 l/mm Efficiency >80% desired across spectral range!"#$%&#"'()*(+,%)-./)!"#$!%#$!&#$!'#$!(#$!)#$!*#$ #$!"#$%&#"'()*(+,%)1#5)6*1%,%(+23)7'&)#%1%&*,)89:)+&*;(+#) *)##$-.//$0123$ +#%$-.//$042563$ %##$-.//$0123$ +##$ +&#$,##$,&#$ *###$ *#&#$ **##$ 0*1%,%(+23)-(4/) Edmund Optics, 1200 l/mm Kaiser Optical, 806 l/mm VPH-806-950 RCWA Theoretical Performance Unpolarized Light Incident at 22.5 Degrees J. Arns Printed 10/19/10 Edmund Optics, 600 l/mm 100-1 Order 0 Order +1 Order +2 Order 90 80 70 Diffraction Efficiency (%) 60 50 40 30 20 10 0 800 850 900 950 1000 1050 1100 Wavelength (nm)

Laboratory optical characterization presently underway System designed for 1.4 cm radial resolution in plasma core, 2.6 cm radial resolution near edge Etendue calculated to be ~0.23 mm2 ster for least-favorable setup Possibly re-commission TS-1 spheromak optics

Position laser head close to vacuum vessel 2 turns in beamline Total beam path length 5 m Vibration-isolated mounting Environmentally controlled, dedicated laser room Beam Dump Vacuum vessel Turning mirrors & beam entry to vessel Monitor alignment with digital cameras at turning mirrors Remote-controlled actuators may be used for inter-shot beamline tuning Nd:YAG laser Horizontal beam through plasma; vertical viewing Beam dump Use absorbing glass plates for power reduction Terminate with razor blade array to minimize reflections Beam dump Beam entry into vessel

For signal transmission in NIR, use fused silica optical fiber Optimized for transmission from 700-1200 nm NA up to 0.22 readily available (25.4 acceptance) Core diameters 50 µm Attenuation ~ 8 db/km over spectral band Very low losses for lengths 30 m High packing fraction and matched fiberdetector geometries maximize collected light fraction Beam Dump Vacuum vessel Nd:YAG laser Turning mirrors & beam entry to vessel Spectrometers remotely located to allow easy accessibility to spectrometers & electronics Available during shot; minimal interruption to operations Electronics remotely located to reduce stray noise effects Pegasus experimental area heavily affected by power supply switching noise Optically transmit MPTS signal out of area

Many MPTS systems use Perkin- Elmer C30659-1060-3A Large area (3 mm diameter) Relatively high responsivity Coating optimized for 1064 nm 65 half-angle of acceptance Alternate concept is an APD linear array For dispersion-grating based instrument, wider spectral bands map to wider physical dimension Detector array placed directly in spectrometer output plane and individual elements grouped together to form desired spectral bin size (ex. (5) elements @ 0.65x0.2 mm each) Practicality depends on customizability of multi-element APD arrays with small element separations

Design of a new Thomson scattering diagnostic for the Pegasus Toroidal Experiment is underway This diagnostic will be used to characterized physics regimes unique to Pegasus: Taylor relaxation of non-solenoidally generated tokamak-like plasmas, the role of resistively-driven helicity dissipation in these plasmas, and also high β T, I p /I TF plasmas Initial predictions yield feasible scattered intensity and distribution estimates Diagnostic design guided by consideration of physical scale sizes Laser specifications, system throughput, and optical characteristics Novel Volume Phase Holographic (VPH)-based MPTS system proposed If details yield unrealistic constraints, consider pre-existing GA-based filter polychromator method Digitization scheme presently being investigated Ideally digitize at rate faster than background variation, but not necessarily at ~GHz (for 10 ns pulse) Characteristic timescale and intensity for background variations during HI discharges must be estimated

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