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Electron Cyclotron Heating by X-wave in the HSX stellarator

Electron Cyclotron Heating by X-wave in the HSX stellarator. K.M.Likin 1 , A.Abdou 1 , A.F.Almagri 1 , D.T.Anderson 1 , F.S.B.Anderson 1 , J.Canik 1 , C.Deng 2 , C.W.Domier 3 , S.P.Gerhardt 1 , R.W.Harvey 4 , H.J.Lu 1 , J.Radder 1 , J.N.Talmadge 1 , K.Zhai 1

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Electron Cyclotron Heating by X-wave in the HSX stellarator

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  1. Electron Cyclotron Heating by X-wave in the HSX stellarator K.M.Likin1, A.Abdou1,A.F.Almagri1, D.T.Anderson1, F.S.B.Anderson1, J.Canik1, C.Deng2, C.W.Domier3, S.P.Gerhardt1, R.W.Harvey4, H.J.Lu1, J.Radder1, J.N.Talmadge1, K.Zhai1 1HSX Plasma Laboratory, Madison, USA3Electrical Engineering Department, UCLA, USA 2Department of Applied Science, UC, Davis, USA4CompX, Del Mar, USA 13th Joint Workshop on ECE and ECRH, Nizhny Novgorod, Russia, May 17-20, 2004

  2. Outline • Introduction on HSX stellarator • Gyrotron power into the machine • Absorption of launched power in HSX plasma • ECE measurements • Fokker-Planck code • Summary 13th Joint Workshop on ECE and ECRH, Nizhny Novgorod, Russia, May 17-20, 2004

  3. The Helically Symmetric Experiment Symmetry in |B| leads to a small deviation of trapped particles orbits from a flux surface and, as a result, to improved neoclassical confinement in a low collisionality regime 13th Joint Workshop on ECE and ECRH, Nizhny Novgorod, Russia, May 17-20, 2004

  4. f = 0o Location of RF antenna f = 22.5o Plasma axis is wound around R = 1.2 m grad|B| Mod|B| Contours f = 45o grad|B| HSX center Nested Flux Surfaces VacuumVessel Major Radius HSX Cross-sections along ½ Field Period 13th Joint Workshop on ECE and ECRH, Nizhny Novgorod, Russia, May 17-20, 2004

  5. 0.3 m E k B grad|B| R Launching Antenna X-wave (E ┴ B) is launched from the low magnetic field side and is focused at the plasma center with a waist of 2 cm (e-2 level) 13th Joint Workshop on ECE and ECRH, Nizhny Novgorod, Russia, May 17-20, 2004

  6. Gyrotron Power vs. Beam Current Po, kW Beam Current, A Gyrotron power on HSX window • Calorimetric measurements are made with a compact dummy load just before the barrier window • In these measurements m-wave diode on the wg directional coupler is calibrated as well Ubeam = 80 kV 13th Joint Workshop on ECE and ECRH, Nizhny Novgorod, Russia, May 17-20, 2004

  7. #3 #2 #4 #1 Attenuator Amplifier Pin Absorption Quartz Window mw Detector #6 #5 Line Average Density, 1018 m-3 Top view Absorption along the machine Six absolutely calibrated m-wave detectors are installed around the HSX at 6, 36, 70 and  100 (0.2 m, 0.9 m, 1.6 m and 2.6 m away from m-wave power launch port, respectively). #3 and #5, #4 and #6 are located symmetrically to the ECRH antenna 13th Joint Workshop on ECE and ECRH, Nizhny Novgorod, Russia, May 17-20, 2004

  8. #1 #2 #3 Absorption in vicinity of ECRH antenna • The same m-wave probes have been installed on the ports next to the ECRH antenna • ECRH power is mostly absorbed in first passes through the plasma column • Absorption is symmetric with respect to the ECRH antenna Absorption efficiency Line Average Density, 1018 m-3 13th Joint Workshop on ECE and ECRH, Nizhny Novgorod, Russia, May 17-20, 2004

  9. First Pass Second Pass Z, m Z, m R, m R, m Ray tracing calculations 3-D Code is used to estimate absorption in HSX plasma • The code runs on a parallel computer with OpenMP and MPI constructs • The code returns an absorbed power profile and integrated efficiency • An optical depth and ECE spectrum can be calculated as well • Bi-Maxwellian plasma is applied if necessary 13th Joint Workshop on ECE and ECRH, Nizhny Novgorod, Russia, May 17-20, 2004

  10. Absorbed Power Profile <ne>= 2·1018 m-3 Te(0) = 0.4 keV P(r), W/cm3 Single-pass absorption Absorption efficiency Line Average Density, 1018 m-3 Profile and Efficiency • Single-pass absorbed power profile is quite narrow (< 0.1ap) • Second Pass: Rays are reflected from the wall and back into the plasma, the absorption is up to 70% while the profile does not broaden • Absorption versus plasma density is calculated (1) at constant Te and (2) based on the TS, ECE and diamagnetic loop data in bi-Maxwellian plasma • Owing to a high non-thermal electron population the absorption can be high enough at a low plasma density 13th Joint Workshop on ECE and ECRH, Nizhny Novgorod, Russia, May 17-20, 2004

  11. Absorbed Power Profile <ne>= 2·1018 m-3 Te(0) = 0.4 keV P(r), W/cm3 Multi-pass absorption • 240 rays are launched into the plasma from 80 points distributed uniformly across and along the machine at a random angle • Multi-pass absorption adds (4 – 7)% to the total efficiency in a wide range of plasma density (0.5 – 2)·1018 m-3 • This multi-pass absorption is low due to (1) low power density in the plasma core and (2) high ray refraction 13th Joint Workshop on ECE and ECRH, Nizhny Novgorod, Russia, May 17-20, 2004

  12. ECE Radiometer • Conventional 8 channel radiometer implemented: 6 channels receive ECE power emitted by plasma at a low magnetic field side and 2 frequency channels – at a high field side • 60 dB BS filter is used to reject the gyrotron power at (28 ± 0.3) GHz and 40 dB fast pin diode protects the mixer from the spurious modes on a leading edge of gyrotron pulse 13th Joint Workshop on ECE and ECRH, Nizhny Novgorod, Russia, May 17-20, 2004

  13. ECE vs. Thomson Scattering ECE Spectrum Tece, keV Te, Tece, keV Line Average Density, 1018 m-3 Frequency, GHz ECE Temperature vs. Plasma Density • ECE temperature drops with plasma density while the electron temperature from Thomson scattering diagnostic is almost independent of plasma density • In plasma density scan the non-thermal feature at a low magnetic field side increases first and then the high frequency emission gets risen 13th Joint Workshop on ECE and ECRH, Nizhny Novgorod, Russia, May 17-20, 2004

  14. a = 90 degs Tece, keV Imkj, cm-1 25 GHz 31 GHz Frequency, GHz Plasma Radius ECE at high plasma density <ne> = 2.5·1018 m-3 • Emission at the high plasma density is thermal • HSX plasma is not a black body: an optical depth should be taken into account to estimate the electron temperature: Tece = Te·(1 - e-t) • Thomson scattering and interferometer data are used to calculate the optical depth 13th Joint Workshop on ECE and ECRH, Nizhny Novgorod, Russia, May 17-20, 2004

  15. Cyclotron Absorption shape Tece, keV Im|kj|, cm-1 a = 90 degs. a = 80 degs. a = 60 degs. We < 0.5wWe > 0.5w Plasma Radius w = 2We ECE at low plasma density • ECE signal is high at both low and high field sides • High signal from outboard side is due to emission from central resonance region where a population of supra-thermal particles is supposed to be high at a central heating • Oblique emission from central regions can contribute to the signal detected at higher frequencies (> 28 GHz, inboard side) 13th Joint Workshop on ECE and ECRH, Nizhny Novgorod, Russia, May 17-20, 2004

  16. Cyclotron Absorption Shape a1 = 90 degs a2 = 60 degs Imkj, cm-1 31 GHz 25 GHz Plasma Radius Energy, keV Density, 1018 m-3 Plasma Radius Plasma Radius Perpendicular and Oblique sight view • Two propagation angles are chosen. Along each direction we assume “Maxwellian tail” with different Te and ne • The following profiles are assumed for tail electrons: Solid lines represent the local absorption at perpendicular propagation and dash lines – at oblique propagation 13th Joint Workshop on ECE and ECRH, Nizhny Novgorod, Russia, May 17-20, 2004

  17. Optical Depth Tece, keV t Frequency, GHz Frequency, GHz ECE Spectrum at 0.5·1018 m-3 • ECE temperature is defined as Tece = Tl·(1 - e-t1) + T2·(1 - e-t2) • This estimate shows that about 30% of electron density belongs to the tail with T1max = 6 keV and T2max = 12 keV, n1max = 0.15·1018 m-3 and n2max = 0.25·1018 m-3 13th Joint Workshop on ECE and ECRH, Nizhny Novgorod, Russia, May 17-20, 2004

  18. rho = 0.05 Absorbed Power Profile Cuts at some pitch angles Pabs = 10 kW unorm = 50 keV CQL3D code for HSX • QHS configuration in HSX has a helical axis of symmetry and itsmod-B is tokamak-like. So with CQL3D code we can simulate the distribution functionin HSX flux coordinates • First runs of CQL3D have been made for HSX plasma at 3·1018 m-3 of central density and 100 kW of launched power. At plasma center a distortion of distribution function occurs in the energy range of (5 – 15) keV 13th Joint Workshop on ECE and ECRH, Nizhny Novgorod, Russia, May 17-20, 2004

  19. Summary • Measured multi-pass absorption efficiency in HSX plasma is high in a wide range of plasma densities • ECE measurements in HSX exhibit a non-thermal feature at a low plasma density • Bi-Maxwellian plasma model partly explains the high absorption and enhanced emission • CQL3D code predicts 5 – 15 keV electrons in the HSX plasma core at 100 kW of launched power 13th Joint Workshop on ECE and ECRH, Nizhny Novgorod, Russia, May 17-20, 2004

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