First Quantification of Electron Thermal Transport in the MST Reversed-Field Pinch

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First Quantification of Electron Thermal Transport in the MST Reversed-Field Pinch Title Abs. TS over. MStFIt j 2kA Te ne Zeff 4kA Te ne Zeff Pohm, W, TauE,beta Xe,D Mot. FIR pola. Monte Carlo Un. An. j ft q,b j ft q,b Conc.? NIRB Zeff eta F.R. Pcrit eta F.R. Pcrit Rep.

First Quantification of Electron Thermal Transport in the MST Reversed-Field Pinch T.M. Biewer, J.K., B.E. Chapman, N.E. Lanier, S.R. Castillo, D.J. Craig, D.J. Den Hartog, and C.B. Forest University of Wisconsin-Madison. Recent diagnostic developments, including an upgrade of the MST Thomson scattering system, have facilitated the first power balance analysis of electron thermal transport in the MST. Recent experiments have focused on acquiring kinetic profile data for electron temperatures and densities under standard and enhanced confinement operating modes. This paper presents results from these experiments, including the first measurement of confinement based upon profile measurements, and a comparison of χe for conventional RFP discharges and discharges with inductively modified current profiles. The methodology of the transport analysis begins with 2D equilibrium reconstructions of the current profile and flux surface geometry, constrained by all available magnetic data. Power deposition is calculated from the measured current density profile and estimates of the neoclassical (Hirshman-Sigmar) resistivity (trapped particle corrections to resistivity are found to be significant for 2D RFP equilibria.) Inversions of interferometer data are performed in the flux geometry to determine the electron density profile. Measured electron temperatures from 6 spatial locations are mapped to the flux geometry and fit by spline functions. Ion temperatures (when available from passive spectroscopy of impurity radiation) are similarly constrained. A Monte Carlo uncertainty analysis is done for all results of the transport analysis. This work was supported by the U.S. D.O.E.

Motivation Ongoing improvements to the diagnostic arsenal of the Madison Symmetric Torus have initiated new investigations into the plasma physics of MST transport. The use of Pulsed Poloidal Current Drive () in the past has demonstrated improved confinement in the MST, based on central electron temperature measurements and a hypothesized profile shape. Recent upgrades of the Thomson scattering system have facilitated measurements of the T e profile in the MST out to r/a=.88. Addition of an NIR Bremstrahlung array has allowed an estimation of Z eff in the MST. We assume Z eff =2. These measurements, when coupled with density profiles from FIR Interferometry and MSTFIT reconstructed equilibria, have made it possible to calculate many transport quantities, including the electron thermal conductivity χ e and the energy confinement time τ E. Monte Carlo analysis is used to ascribe error bands for transport quantities, rather than attempting to nonlinearly propagate the experimental uncertainty in the measured data.

What is Pulsed Poloidal Current Drive? Loop Voltage (V) soft X-ray ratio (~Te) Toroidal Gap Voltage (V) Reversal Parameter, F F=Bt(a)/<Bt> standard discharge 23-oct-1998 #6 discharge 23-oct-1998 #51 During a "normal" plasma discharge a series of 5 voltage pulses are applied to the MST shell to produce a magnetic field which is in the opposite sense to the established toroidal magnetic field, forcing flux out of the MST. This opposing B is thought to cause a poloidally driven edge current. is observed to improve machine performance. It is believed that magnetic modes in the MST derive their free energy from the gradient in the current profile, which is steepest at the edge. By inductively driving current in the edge, could reduce the gradient and remove free energy from the magnetic modes, resulting in decreased magnetic fluctuations and hence improved particle and energy confinement. t (s) from begining of discharge

MST Thomson Scattering Diagnostic 5J single-pulse/single-point ruby laser TS system: ensembling of shots (over multiple days) is necessary to construct spacial profiles AND time evolution. z r correction lenses movable fiber bundle spectrometer to beam dump MCP & electronics edge ruby laser path MST toriodal centerline 1.5 m r/a=.9 viewing dump central ruby laser path r/a=.6 T A A B B T T f=15 mm conv. lens steering mirrors r/a 1.8.6.4.2 21 12 24 9 27 6 3 3 33 chords used Thomson Scattering Views view r/a φ 1.627-18.46 2.455-16.93 3.283-13.53 4.115 5.8 123.91 6.244 147.6 7.415 151.39 8.587 153.19 9.882 22.28 1.769 31.41 11.681 43.26 12.63 57.76 13.625 73.61 14.666 88.59 15.746 11.1 16.854 11.82 15 view 1 5.2.4.6.8 1 r/a error bars indicate radial range of scattering volume on each view

Far Infrared Interferometer Diagnostic H α and Electron Density Profile Measurements on MST 9 Chord H α Array Waveguides Signal Beam 11 Chord Far Infrared Interferometer Reference Beam Wire Mesh BeamSplitters Twin Far Infrared Lasers 25mW Each λ 432µm Plasma Vacuum Duct CO 2 Pumping Laser 125W Continuous λ =1.6µm Schottky Detectors The 11 Chord Far Infrared(FIR) Laser Interferometer provides electron density measurements with 4 µ s time resolution. The 9 Chord H α Array along with the data obtained from the FIR interferometer allow measurements of the neutral Hydrogen density.

NIR Bremsstrahlung Zeff Diagnostic A spectral window in Bremsstrahlung's broadband spectrum - through which other plasma radiative sources (e.g. spectral lines, recombination radiation) are absent or negligible - has been found in the NIR. An array of detectors sensitive to this narrow bandwidth centered at 14 nm, has been installed on MST. Mid-plane of MST Poloidal distribution of 17 NIRB Viewing Chords six detectors are currently set up on outboard chords signal out Bremsstrahlung detectors view the plasma through a series of optical lenses. The optics include an H-alpha filter and a bandpass filter centered at 14 nm. "Perpendicular" Plane Note shift of flux surfaces from the "Perpendicular" Plane. A center shift of 6cm is assumed Filtered radiation is detected by a photodiode and amplified by a high gain transconductance amplifier. Bremsstrahlung emissivity ( ) can be directly related to Plasma Zeff by the formula: ε(λ ) =1.89x1 28 g ff n 2 Z eff e (hc/λt e ) signal out Thus, the detector response (V) across the length (l) of a chord is: V det = λ 2 T e F cal (λ)ε(λ,l) dλdl Detector Voltage (in V) Characteristic NIRB Detector Output 2 1.5 1.5 1 2 3 4 time (in ms) A calibration function (Fcal) has been derived for each detector, but the apparent contamination of recombination radiation at MST's edge (due to lower temperatures) has delayed the data inversions that will produce conclusive Zeff profiles. Center to Edge Detector Signals.35 Encouragingly, the raw data displays expected.3 behavior. By selecting appropriate times within each shot, and averaging the signal.25 over an interval, one value (in Volts) is found for each detector in each shot. Here is one.2 such plot of each of the six signals. Note the sharp rise at the edge where recombination.15 radiation dominates and the low emission at the center (as expected for shots)..1 Detector Voltage (in V).2.4.6.8 1 Detector position (in r/a)

MSTFIT is a fully toroidal, 2D equilbrium reconstruction code

MSTFIT and Monte Carlo Error Analysis MSTFIT is a fully toroidal (2D) equilibrium reconstruction code that utilizes measured data to constrain the reconstruction. Plasma Parameters: F, θ, and I p are entered along with edge magnetic probe signals to manage the reconstruction of equilibrium quantities. Once an equilibrium is found, it becomes easier to invert chord averaged quantities, such as FIR measured electron density. The inversions are done in flux coordinate geometry, which can differ significantly from machine geometry. Diagnostic data such as T e, T i, n e, dt e /dt, dn e /dt, and Z eff are then combined with reconstructed quantities to ultimately calculate profiles of transport coefficients. By randomly varying the measured quantities within their error bars and collecting the calculated transport quantities, a Monte Carlo type "error band" is derived.

Measured Profiles Ip~2 ka 6 5 First 6 point electron temperature profiles measured on the MST. 4 T e (ev) 3 2 1 15 6 chord, ensembled Thomson scattering Biewer.1.2.3.4.5 Thomson Scattering measurements are assembled over multiple days and are susceptible to changes in machine conditions. inferred T i (ev) 1 5 The assumptions that Ti=1/4 Te for and Ti=1/2 Te for discharges are supported by measurements from majority and minority impurity diagnostics. 1.2 1 19.1.2.3.4.5 n e (m -3 ) 1 1 19 8 1 18 6 1 18 4 1 18 FIR Interferomety measured density profiles are Abel inverted using MSTFIT, a fully toroidal equilibrium reconstruction code. 2 1 18 Abel Inverted 11 chord Far Infrared Interferometry Lanier.1.2.3.4.5

Measured Profiles Ip~4 ka 8 7 6 First 6 point electron temperature profiles measured on the MST. 5 T e (ev) 4 3 2 1 25 6 chord, ensembled Thomson scattering Biewer.1.2.3.4.5 Thomson Scattering measurements are assembled over multiple days and are susceptible to changes in machine conditions. inferred T i (ev) 2 15 1 5 The assumptions that Ti=1/4 Te for and Ti=1/2 Te for discharges are supported by measurements from majority and minority impurity diagnostics. n e (m -3 ) 1.4 1 19.1.2.3.4.5 1.2 1 19 1 1 19 8 1 18 6 1 18 FIR Interferomety measured density profiles are Abel inverted using MSTFIT, a fully toroidal equilibrium reconstruction code. 4 1 18 2 1 18 Abel Inverted 11 chord Far Infrared Interferometry Lanier.1.2.3.4.5

1.5 1 6 Reconstructed Profiles Ip~2 ka current density (A/m 2 ) 1 1 6 5 1 5 The current density on axis clearly increases, whereas in the edge there is little apparent change..1.2.3.4.5.6 trapped particle fraction.5.4.3.2 MSTFIT predicts that a substantial fraction of the particles are magnetically trapped in the MST during both and discharges. q dq/dr.1.3.2.1 -.5-1.1.2.3.4.5 -.1 -.2.5 -. 1.56.1.2.3.4.5.1.2.3.4.5 5 Bp Bt Btot Bp Bt Btot.25.2.15.1.5 1.55 1.54 1.53 1.52 1.51 B (T) R surf (m) The application of clearly shifts the flux reversal surface inward, as shown by observing the zero crossing of the toroidal magnetic field. Also, leads to an increase in the amount of magnetic sheer at the edge of the plasma. -1.5.1.2.3.4.5.1.2.3.4.5 1.5

2.5 1 6 Reconstructed Profiles Ip~4 ka current density (A/m 2 ) 2 1 6 1.5 1 6 1 1 6 5 1 5.6.1.2.3.4.5 The current density on axis clearly increases, whereas in the edge there is little apparent change. trapped particle fraction.5.4.3.2 MSTFIT predicts that a substantial fraction of the particles are magnetically trapped in the MST during both and discharges..1 q dq/dr.3.2.1.1.2.3.4.5 -.1 -.2.5 1.56 -.1.1.2.3.4.5.1.2.3.4.5 -.5-1 Bp Bt Btot Bp Bt Btot.5.4.3.2.1 1.55 1.54 1.53 1.52 1.51 B (T) R surf (m) The application of clearly shifts the flux reversal surface inward, as shown by observing the zero crossing of the toroidal magnetic field. Also, leads to an increase in the amount of magnetic sheer at the edge of the plasma. -1.5.1.2.3.4.5.1.2.3.4.5 1.5

resistivity H-S (ohm-m) eta*j 2 (W/m 3 ) 1-5 1-6 1-7 1-8 1.2 1 6 1 1 6 8 1 5 6 1 5 4 1 5 2 1 5 Calculated Profiles Ip~2 ka.1.2.3.4.5.1.2.3.4.5 Neoclassical effects become very important when modeling in 2D. Using Hirshman-Sigmar resistivity (rather than Spitzer) in "" reconstructions matches the measured and calculated ohmic input power with a conservative estimate of Zeff=2. I.e. No need of "anomalous" resistivty to account for MHD dynamo action. Normalizing to total input power shows that power deposition is enhanced in the edge during as compared to dischages at this current. etaj 2 /etaj 2 tot 3.5 3 2.5 2 1.5 1.5.1.2.3.4.5 3 1 6 4 P ohmic (W) 2.5 1 6 2 1 6 1.5 1 6 1 1 6 5 1 5 P ohmic ηj 2 dv.1.2.3.4.5 Stored Thermal Energy, W (J) 35 3 25 2 15 1 W 3 2 (n et e + n i T i )dv 5.1.2.3.4.5

resistivity H-S (ohm-m) eta*j 2 (W/m 3 ) 1-5 1-6 1-7 1-8 1.6 1 6 1.4 1 6 1.2 1 6 1 1 6 8 1 5 6 1 5 Calculated Profiles Ip~4 ka.1.2.3.4.5 Neoclassical effects become very important when modeling in 2D. Using Hirshman-Sigmar resistivity (rather than Spitzer) in "" reconstructions matches the measured and calculated ohmic input power with a conservative estimate of Zeff=2. I.e. No need of "anomalous" resistivty to account for MHD dynamo action. Normalizing to total input power shows that the power deposition profile is nearly identical during and dischages at this current. 2.5 2 4 1 5 2 1 5.1.2.3.4.5 etaj 2 /etaj 2 tot 1.5 1.5.1.2.3.4.5 5 1 6 1 1 4 4 1 6 8 P ohmic (W) 3 1 6 2 1 6 P ohmic ηj 2 dv 1 1 6.1.2.3.4.5 Stored Thermal Energy, W (J) 6 4 2 W 3 2 (n et e + n i T i )dv.1.2.3.4.5

2 ka Pohmic 2.45 +/-.22 1.7 +/-.8 MW W 2. +/-.1 4.2 +/-.2 kj dw/dt 383.1 +/- 28.6 kw Main Results 4 ka Pohmic 4.34 +/-.16 1.99 +/-.12 MW W 4.4 +/-.2 8.8 +/-.4 kj dw/dt 133.1 +/- 38.1 kw τe.81 +/-.1 6.45 +/- 1.28 ms βpol 6.36 +/-.33 13.28 +/-.66 % τe 1.2 +/-.7 4.83 +/-.65 ms βpol 3.29 +/-.11 7.52 +/-.38 % 1 W τ E = P ohmic W t 1 β p = 1 V (n et e + n i T i )dv 1 2 B p 2µ 1 1 X e (m 2 /s) 1 X e (m 2 /s) 1 1.1.1.2.3.4.5 η 1 HS j 2 dv + 3 Χ e t 2 n et e dv n e T e 4π 2 5 R r 2 D Class.T e n e 1.1.1.2.3.4.5 D Class. = η HS(n e T e + n i T i ) 2.5 m 2 /s for comparison: B tot T e D Bohm = 1 m 2 /s 16eB tot

Conclusions For the first time, 6 point profiles of T e have been measured during in the MST. Low X e in the edge is coincident with enhanced magnetic shear in the edge. During the flux surface where toroidal magnetic field reverses direction is forced inward (i.e. F is deepened), leading to a steepening of the q profile, particularly in the edge. It is unnecessary to invoke any anomalous resistivty during "standard" MST discharges if the fraction of trapped particles is taken into account, along with a neoclassical (as per Hirshman and Sigmar) assessment of resistivity. With a very reasonable estimation of Zeff=2 the reconstructed input power matches the measured input power. The energy confinement time greatly improves during, presumably due to the reduction of magnetic fluctuations. τe~6 ms (if Z eff ~2) from 1 ms β p reaches 13% during low current.