Second Switching Power Amplifier (SPA) Upgrade Physics Considerations Discussion S.A. Sabbagh 1, and the NSTX Research Team 1 Department of Applied Physics,

Slides:



Advertisements
Similar presentations
Potential Upgrades to the NBI System for NSTX-Upgrade SPG, TS NSTX Supported by Culham Sci Ctr U St. Andrews York U Chubu U Fukui U Hiroshima U Hyogo U.
Advertisements

Study of tearing mode stability in the presence of external perturbed fields Experimental validation of MARS-K/Q and RDCON codes Z.R. Wang 1, J.-K. Park.
NSTX-U T&T TSG Contributions to FY15 JRT NSTX-U Supported by Culham Sci Ctr York U Chubu U Fukui U Hiroshima U Hyogo U Kyoto U Kyushu U Kyushu Tokai U.
Summary of Presentations on Plasma Start-up and Progress on Small ST devices from STW2011 R. Raman University of Washington, Seattle, WA The Joint Meeting.
Development and characterization of intermediate- δ discharge with lithium coatings XP-919 Josh Kallman Final XP Review June 5, 2009 NSTX Supported by.
NSTX Status and Plans College W&M Colorado Sch Mines Columbia U Comp-X General Atomics INEL Johns Hopkins U LANL LLNL Lodestar MIT Nova Photonics New York.
NSTX XP830 review – J.W. Berkery J.W. Berkery, S.A. Sabbagh, H. Reimerdes Supported by Columbia U Comp-X General Atomics INEL Johns Hopkins U LANL LLNL.
NSTX SAS – APS DPP ‘05 Supported by Office of Science S.A. Sabbagh 1, A.C. Sontag 1, W. Zhu 1, M.G. Bell 2, R. E. Bell 2, J. Bialek 1, D.A. Gates 2, A.
NSTX NSTX Team Meeting Jan. 3, 2013 NSTX Team Meeting Jan. 3, 2013 Culham Sci Ctr U St. Andrews York U Chubu U Fukui U Hiroshima U Hyogo U Kyoto U Kyushu.
NSTX Team Meeting May 28, 2008 Supported by Office of Science College W&M Colorado Sch Mines Columbia U Comp-X General Atomics INEL Johns Hopkins U LANL.
Quality Assurance Readiness for Operations Review Judy Malsbury, Head of QA Princeton Plasma Physics Laboratory NSTX Upgrade LSB B318 December 9-11, 2014.
Relay Feedback and X-point Height Control Egemen Kolemen S. Gerhardt and D. A. Gates 2010 Results Review Nov/30/2010 NSTX Supported by College W&M Colorado.
PCS Navigation D. Mueller January 26-28, 2010 Culham Sci Ctr U St. Andrews York U Chubu U Fukui U Hiroshima U Hyogo U Kyoto U Kyushu U Kyushu Tokai U NIFS.
XP1518: RWM PID control optimization based on theory and experiment S. A. Sabbagh, J.W. Berkery, J.M Bialek Y.S. Park, (et al…) Department of Applied Physics,
EP-TSG session Meeting agenda et al. M. Podestà NSTX-U Research Forum 2015 EP-TSG session PPPL, Room B252 02/24/2015 NSTX-U Supported by Culham Sci Ctr.
Non-axisymmetric Control Coil Upgrade and related ideas NSTX Supported by V1.0 Culham Sci Ctr U St. Andrews York U Chubu U Fukui U Hiroshima U Hyogo U.
Current status of high k scattering system J. Kim 1, Y. Ren 2, K-C. Lee 3 and R. Kaita 2 1) POSTECH 2) PPPL 3) UC Davis NSTX Monday Physics Meeting LSB-318,
1 Update on Run Schedule R. Raman NSTX Team Meeting PPPL, Princeton, NJ, 08 February, 2006 Work supported by DOE contract numbers DE-FG02-99ER54519 AM08,
Supported by Office of Science Culham Sci Ctr U St. Andrews York U Chubu U Fukui U Hiroshima U Hyogo U Kyoto U Kyushu U Kyushu Tokai U NIFS Niigata U U.
NSTX Supported by Culham Sci Ctr U St. Andrews York U Chubu U Fukui U Hiroshima U Hyogo U Kyoto U Kyushu U Kyushu Tokai U NIFS Niigata U U Tokyo JAEA Hebrew.
Radiative divertor with impurity seeding in NSTX V. A. Soukhanovskii (LLNL) Acknowledgements: NSTX Team NSTX Results Review Princeton, NJ Wednesday, 1.
NSTX Team Meeting July 21,, 2011 NSTX TF Update NSTX Team Meeting July 21, 2011 NSTX Supported by Culham Sci Ctr U St. Andrews York U Chubu U Fukui U Hiroshima.
NSTX Effects of NTSX Upgrades on DiagnosticsFebruary 8, NSTX Supported by College W&M Colorado Sch Mines Columbia U CompX General Atomics INEL Johns.
Prototype Multi-Energy Soft X-ray Diagnostic for EAST Kevin Tritz Johns Hopkins University NSTX-U Monday Physics Meeting PPPL, Princeton, NJ June 25 th,
Direct measurement of plasma response using Nyquist Contour Z.R. Wang 1, J.-K. Park 1, M. J. Lanctot 2, J. E. Menard 1,Y.Q. Liu 3, R. Nazikian 1 1 Princeton.
ASC Five Year Plan Chapter Status Stefan Gerhardt NSTX-U Supported by Culham Sci Ctr York U Chubu U Fukui U Hiroshima U Hyogo U Kyoto U Kyushu U Kyushu.
NSTX Upgrade Project – Final Design Review June , NSTX Supported by College W&M Colorado Sch Mines Columbia U CompX General Atomics INEL.
1 R Raman, B.A. Nelson, D. Mueller 1, T.R. Jarboe, M.G. Bell 1, J. Menard 1, R. Maqueda 2 et al. University of Washington, Seattle 1 Princeton Plasma Physics.
Xp705: Multimode ion transport: TAE avalanches E D Fredrickson, N A Crocker, N N Gorelenkov, W W Heidbrink, S Kubota, F M Levinton, H Yuh, R E Bell NSTX.
NSTX XP818: ELM mitigation w/midplane coils - SAS S. A. Sabbagh, J-K. Park, T. Evans, S. Gerhardt, R. Maingi, J.E. Menard, many others… (joint ELM mitigation.
Development of Improved Vertical Position Control S.P. Gerhardt, E. Kolemen ASC Session, NSTX 2011/12 Research Forum Location Date NSTX Supported by College.
1 Roger Raman for the NSTX Research Team University of Washington, Seattle NSTX Run Usage 27 February – 5 May, 2006 NSTX Mid-Run Assessment PPPL, Princeton,
Energy Confinement Scaling in the Low Aspect Ratio National Spherical Torus Experiment (NSTX) S. M. Kaye, M.G. Bell, R.E. Bell, E.D. Fredrickson, B.P.
Some Halo Current Measurements in 2009 S.P. Gerhardt Thanks to: E. Fredrickson, H. Takahashi, L. Guttadora NSTX Results Review, 2009 NSTX Supported by.
Macroscopic Stability TSG Pre-forum Meeting #1 J.W. Berkery Department of Applied Physics, Columbia University, New York, NY NSTX-U Supported by Culham.
XP1020: Determination of Weak RWM Stability Rotation Profiles J.W. Berkery, S.A. Sabbagh, H. Reimerdes Department of Applied Physics, Columbia University,
NSTX Team Meeting February 7, 2007 Supported by Office of Science College W&M Colorado Sch Mines Columbia U Comp-X General Atomics INEL Johns Hopkins U.
Supported by Office of Science NSTX H. Yuh (Nova Photonics) and the NSTX Group, PPPL Presented by S. Kaye 4 th T&C ITPA Meeting Culham Lab, UK March.
Development and characterization of intermediate- δ discharge with lithium coatings XP-919 Josh Kallman XP Review - ASC Feb 2, 2009 NSTX Supported by College.
NSTX Team Meeting December 21, 2009 College W&M Colorado Sch Mines Columbia U Comp-X General Atomics INEL Johns Hopkins U LANL LLNL Lodestar MIT Nova Photonics.
Enhancement of edge stability with lithium wall coatings in NSTX Rajesh Maingi, Oak Ridge National Lab R.E. Bell, B.P. LeBlanc, R. Kaita, H.W. Kugel, J.
Effect of 3-D fields on edge power/particle fluxes between and during ELMs (XP1026) A. Loarte, J-W. Ahn, J. M. Canik, R. Maingi, and J.-K. Park and the.
NSTX-Upgrade Magnetics And Related Diagnostics SPG NSTX Supported by Culham Sci Ctr U St. Andrews York U Chubu U Fukui U Hiroshima U Hyogo U Kyoto U Kyushu.
NSTX NSTX Team Meeting May 7, 2013 NSTX Team Meeting May 7, 2013 Culham Sci Ctr U St. Andrews York U Chubu U Fukui U Hiroshima U Hyogo U Kyoto U Kyushu.
First results of fast IR camera diagnostic J-W. Ahn and R. Maingi ORNL NSTX Monday Physics Meeting LSB-318, PPPL June 22, 2009 NSTX Supported by College.
NSTX NSTX TF, PF and umbrella Upgrade Internal ReviewFeb 24, NSTX Supported by College W&M Colorado Sch Mines Columbia U CompX General Atomics INEL.
NSTX NSTX LidsJuly 6, NSTX Supported by College W&M Colorado Sch Mines Columbia U CompX General Atomics INEL Johns Hopkins U LANL LLNL Lodestar.
NSTX Team Meeting June 30, 2009 College W&M Colorado Sch Mines Columbia U Comp-X General Atomics INEL Johns Hopkins U LANL LLNL Lodestar MIT Nova Photonics.
Supported by Office of Science NSTX S.M. Kaye, PPPL ITPA PPPL 5-7 Oct Confinement and Transport in NSTX: Lithiumized vs non-Lithiumized Plasmas Culham.
NSTX-U Disruption PAM Working Group – Controlled Shutdown XP Discussion S. A. Sabbagh and R. Raman Department of Applied Physics, Columbia University,
Global Mode Stability and Active Control in NSTX S.A. Sabbagh 1, J.W. Berkery 1, R.E. Bell 2, J.M. Bialek 1, S. Gerhardt 2, R. Betti 3, D.A. Gates 2, B.
Planning for Toroidal Lithium Divertor Target for NSTX and Supporting Experiments on CDX-U/LTX R. Kaita Boundary Physics Science Focus Group Meeting July.
Upgrades to PCS Hardware (Incomplete) KE, DAG, SPG, EK, DM, PS NSTX Supported by Culham Sci Ctr U St. Andrews York U Chubu U Fukui U Hiroshima U Hyogo.
NSTX 2007 MHD XP Review – J. Menard 1 Optimization of RFA detection algorithms during dynamic error field correction Presented by: J.E. Menard, PPPL Final.
Presently Planned Vacuum-Side Diagnostics for the NSTX-Upgrade Center Column NSTX Supported by Culham Sci Ctr U St. Andrews York U Chubu U Fukui U Hiroshima.
XP-945: ELM Pacing via Vertical Position Jogs S.P. Gerhardt, J.M. Canik, D. Gates, R. Goldston, R. Hawryluk, R. Maingi, J. Menard, S. Sabbagh, A. Sontag.
Preliminary Results from XP1020 RFA Measurements J.W. Berkery Department of Applied Physics, Columbia University, New York, NY, USA NSTX Monday Physics.
Implementation of a 3D halo neutral model in the TRANSP code and application to projected NSTX-U plasmas S. S. Medley 1, D. Liu 2, M. V. Gorelenkova 1,
NSTX NSTX Team Meeting –Masa Ono August 15, 2014 NSTX-U Team Meeting August 15, 2014 Culham Sci Ctr U St. Andrews York U Chubu U Fukui U Hiroshima U Hyogo.
Advanced Scenario Development on NSTX D. A. Gates, PPPL For the NSTX Research Team 50th APS-DPP meeting Dallas, TX November 17, 2008 College W&M Colorado.
NSTX-U Collaboration Status and Plans for: M.I.T. Plasma Science and Fusion Center Abhay K. Ram, Paul Bonoli, and John Wright NSTX-U Collaborator Research.
1 Status of the 2008 ASC TSG Run plan Presented by D. A. Gates (J. Menard Deputy) At the NSTX Mid-run asessment PPPL April 16, 2008 Supported by Office.
1 Roger Raman for the NSTX Research Team University of Washington, Seattle Update on the NSTX Run Plan PPPL, Princeton, NJ, 15 May, 2006 Supported by Office.
Monitoring impact of the LLD Adam McLean, ORNL T. Gray, R. Maingi Lithium, TSG group preliminary research forum PPPL, B252 Nov. 23, 2009 NSTX Supported.
Comments on HC Measurements for NSTX- Upgrade SPG CS Upgrade Meeting 11/2/11 NSTX Supported by Culham Sci Ctr U St. Andrews York U Chubu U Fukui U Hiroshima.
Correlation between Electron Transport and Shear Alfven Activity in NSTX College W&M Colorado Sch Mines Columbia U Comp-X General Atomics INEL Johns Hopkins.
Supported by Office of Science NSTX K. Tritz, S. Kaye PPPL 2009 NSTX Research Forum PPPL, Princeton University Dec. 8-10, 2008 Transport and Turbulence.
NSTX Team Meeting April 5, 2006 Supported by Office of Science College W&M Colorado Sch Mines Columbia U Comp-X General Atomics INEL Johns Hopkins U LANL.
XP-950: XP-950: Dependence of metallic impurity accumulation on I p and the outer gap in the presence of lithium deposition S. Paul, S. P. Gerhardt are.
NSTX NSTX Upgrade Project – Final Design ReviewJune 22-24, NSTX Supported by College W&M Colorado Sch Mines Columbia U CompX General Atomics INEL.
Presentation transcript:

Second Switching Power Amplifier (SPA) Upgrade Physics Considerations Discussion S.A. Sabbagh 1, and the NSTX Research Team 1 Department of Applied Physics, Columbia University, New York, NY, USA NSTX ARRA Meeting May 20, 2009 PPPL College W&M Colorado Sch Mines Columbia U Comp-X General Atomics INEL Johns Hopkins U LANL LLNL Lodestar MIT Nova Photonics New York U Old Dominion U ORNL PPPL PSI Princeton U Purdue U Sandia NL Think Tank, Inc. UC Davis UC Irvine UCLA UCSD U Colorado U Maryland U Rochester U Washington U Wisconsin Culham Sci Ctr U St. Andrews York U Chubu U Fukui U Hiroshima U Hyogo U Kyoto U Kyushu U Kyushu Tokai U NIFS Niigata U U Tokyo JAEA Hebrew U Ioffe Inst RRC Kurchatov Inst TRINITI KBSI KAIST POSTECH ASIPP ENEA, Frascati CEA, Cadarache IPP, Jülich IPP, Garching ASCR, Czech Rep U Quebec NSTX Supported by v1.0

NSTX Second SPA Upgrade - discussion (S.A. Sabbagh)May 20 th, Second Switching Power Amplifier Planned for NSTX  Part of NSTX 5-year Plan  ( ) “Implement 2 nd switching power amplifier (SPA) to allow independent control of all 6 midplane RWM coils”  Engineering meeting held in parallel to March ReNeW workshop at PPPL  Existing Status (bullets from Raki’s talk 3/18/09)  The Six RWM coils are grouped in pairs  Each Pair is fed from one sub-unit of SPA which has 3 sub-units  Each coil has two turns. Maximum of 3.33kA Pulsed power feed.  Three dedicated ckts. & power loops for RWM Coils exist  Proposed Change  Each RWM coils are to be individually fed  Each coil to be fed from one sub-unit of SPA

NSTX Second SPA Upgrade - discussion (S.A. Sabbagh)May 20 th, Some physics program considerations for 2 nd SPA  More flexible RWM feedback capability  n = 2 (and n = 3) field for rotation control during n = 1 RWM feedback  Could begin multi-mode RWM control studies, n = 2 with n = 1 RWM feedback  Greater spectrum for dynamic error field correction  More flexible rotation control capability  Simultaneous odd/even n field spectrum for NTV rotation control  Greater rotation control flexibility for real-time rotation control  More flexible field generation for ELM control  independent n = 1, 2, 3 amplitude and phase control for RMP studies (with n=1 RWM feedback)  Independent use for CHI  Run CHI absorber and n=1, 3 control simultaneously

NSTX Second SPA Upgrade - discussion (S.A. Sabbagh)May 20 th, Design work for upgraded non-axisymmetric control capabilities has begun  Capabilities  Non-axisymmetric control coil (NCC) – at least four applications RWM stabilization (n > 1, higher  N ) DEFC with greater field correction capability ELM control (n = 6) n > 1 propagation, increased V  control) Similar to proposed ITER coil design Consider design to allow moderate 3-d shaping for mode control In incremental budget  Addition of 2 nd SPA power supply unit for simultaneous n > 1 fields  Non-magnetic RWM sensors; advanced RWM active feedback control algorithms Primary PP option Secondary PP option Existing coils Proposed Internal Non-axisymmetric Control Coil (NCC) (initial designs - 12 coils toroidally) RWM with n > 1 RWM observed (Sabbagh, et al., Nucl. Fusion 46, 635 (2006). )

NSTX Second SPA Upgrade - discussion (S.A. Sabbagh)May 20 th, VALEN RWM predictions for new control coils behind passive plates (PP) coils behind copper passive plates perform worse than existing external RWM change copper passive plates to SS RWM performs better than existing external RWM nn growth rate  [1/s] passive Ideal wall limit copper PP Coils behind Cu secondary PP Coils behind Cu primary PP external system nn growth rate  [1/s] passive Ideal wall limit partial steel PP Coils behind SS secondary PP Coils behind SS primary PP external system J. Bialek

NSTX Second SPA Upgrade - discussion (S.A. Sabbagh)May 20 th, Proposed NSTX upgrade, coils on plasma side of passive plates Possible upgrades: coils on plasma side of passive plates we examine only one such coil system at a time we approach the ideal wall limit with either coil system new coils plasma side primary passive plates new coils plasma side secondary passive plates

NSTX Second SPA Upgrade - discussion (S.A. Sabbagh)May 20 th, New control coils on plasma side of NSTX copper passive plates (PP) stabilize to C  >99% passive existing coils Ideal wall limit existing coils nn nn growth rate  [1/s] coils on plasma side Cu secondary PP stabilize to  n = 7.04 coils on plasma side Cu primary PP stabilize to  n = 7.05 Ideal wall limit  n = 7.06 J. Bialek

NSTX Second SPA Upgrade - discussion (S.A. Sabbagh)May 20 th, Recent ELM mitigation results show promising results with NCC  n = 6 configuration  Higher q 95 shows best results T. Evans, GA

NSTX Second SPA Upgrade - discussion (S.A. Sabbagh)May 20 th, Consider a more capable power supply upgrade to best support future non-axisymmetric field upgrades?  Investment to support future upgrades  JEM: “2nd SPA would be needed for any future RMP/RWM/EF control coils, so this is a good investment”  JEM: “More coils are next in line as a possible major facility upgrade”  Consider a power supply that will best support internal NCC coil upgrade  Internal RWM coil upgrade will allow expanded physics studies that is best supported by faster power supplies  RWM stabilization up to the with-wall beta limit (  growth < 1 ms)  Greater control capability for RWMs with fast growth (  growth < 1 ms)  Potential for control of NTMs at large R (f ~ n*10 kHz)  Potential for non-resonant increase of plasma rotation (f ~ n*10 kHz)