linear coupling of alfv én cascade modes in nstx

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Neal A. Crocker , UCLA ED Fredrickson, 2 NN Gorelenkov, 2 WW Heidbrink, 3 GJ Kramer, 2 RE Bell, 2 D Darrow, 2 J Hosea, 2 S Kubota, 1 BP LeBlanc, 2 KC Lee, 4 FM Levinton, 5 JE Menard, 2 M Podesta, 3 G Taylor, 2 H Yuh 5 and the NSTX Team 1 UCLA, 2 PPPL, 3 UCI, 4 UCD, 5 Nova Photonics 50th Annual Meeting of the Division of Plasma Physics Dallas, TX November 17-21, 2008 Linear coupling of Alfvén Cascade Linear coupling of Alfvén Cascade modes in NSTX modes in NSTX 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 SNL 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 NSTX Supported by

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NSTX. Supported by . Linear coupling of Alfv én Cascade modes in NSTX. 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 SNL Think Tank, Inc. - PowerPoint PPT Presentation

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Page 1: Linear coupling of Alfv én Cascade modes  in NSTX

Neal A. Crocker , UCLAED Fredrickson,2 NN Gorelenkov,2 WW Heidbrink,3

GJ Kramer,2 RE Bell,2 D Darrow,2 J Hosea,2 S Kubota,1 BP LeBlanc,2 KC Lee,4 FM Levinton,5

JE Menard,2 M Podesta,3 G Taylor,2 H Yuh5 and the NSTX Team

1UCLA, 2PPPL, 3UCI, 4UCD, 5Nova Photonics50th Annual Meeting of the Division of Plasma

PhysicsDallas, TX

November 17-21, 2008

Linear coupling of Alfvén Cascade modes Linear coupling of Alfvén Cascade modes in NSTXin NSTX

College W&MColorado Sch MinesColumbia UComp-XGeneral AtomicsINELJohns Hopkins ULANLLLNLLodestarMITNova PhotonicsNew York UOld Dominion UORNLPPPLPSIPrinceton USNLThink Tank, Inc.UC DavisUC IrvineUCLAUCSDU ColoradoU MarylandU RochesterU WashingtonU Wisconsin

Culham Sci CtrU St. Andrews

York UChubu UFukui U

Hiroshima UHyogo UKyoto U

Kyushu UKyushu Tokai U

NIFSNiigata UU Tokyo

JAEAHebrew UIoffe Inst

RRC Kurchatov InstTRINITI

KBSIKAIST

POSTECHASIPP

ENEA, FrascatiCEA, Cadarache

IPP, JülichIPP, Garching

ASCR, Czech RepU Quebec

NSTXNSTX Supported by

Page 2: Linear coupling of Alfv én Cascade modes  in NSTX

NSTXNSTX 50th Annual Meeting of the Division of Plasma Physics – Linear coupling of ACs in NSTX (Crocker) Oct. 17-21, 2008

*a.k.a. reverse-shear Alfvén eigenmodes

Recent NSTX results extend understanding of Alfvén Cascade (AC) mode* physics to high and high

• Alfvén Cascade (AC) modes* unstable in reverse-shear (RS) plasmas– RS is advanced scenario for ITER & Component Test Facility –

• Understanding of AC physics desirable– ACs transport fast-ions (beam ions, ICRF accelerated ions and fusion

alphas) – impact plasma performance– AC modes serve diagnostic function [“MHD spectroscopy” – measure

qmin(t)]

• High and high are relatively unexplored regimes for AC modes

Page 3: Linear coupling of Alfv én Cascade modes  in NSTX

NSTXNSTX 50th Annual Meeting of the Division of Plasma Physics – Linear coupling of ACs in NSTX (Crocker) Oct. 17-21, 2008

Summary of Results

• NOVA-K linear stability code used to calculate shear Alfvén plasma eigenmode structure in NSTX reversed shear plasmas– extends study of Alfvén Cascade (AC) modes to high (ratio of kinetic

and magnetic pressures) and high (inverse aspect ratio, = a/R)

• Eigenmodes not “pure” AC modes  – mode structure shows linear coupling of ACs with toroidicity-induced Alfvén eigenmodes (TAE)

• High and high enhance linear coupling• Coupling gives broad spectrum of poloidal components and

radially extended structure– broad spectrum can lead to enhanced transport – multiple fast-ion

resonances– extended structure enhances edge B, so Mirnov coils see AC

modes – coils relatively insensitive to ACs in conventional tokamaks

Page 4: Linear coupling of Alfv én Cascade modes  in NSTX

NSTXNSTX 50th Annual Meeting of the Division of Plasma Physics – Linear coupling of ACs in NSTX (Crocker) Oct. 17-21, 2008

NOVA-K* code explores high , high AC physics

• Linear, ideal MHD, hybrid/kinetic code.• Computes Alfvén eigenmode (AE) structure, frequency,

growth rate– fast-ions treated perturbatively– “Chu” filtering scheme† eliminates acoustic singularities– geodesic curvature, effects included

• Success demonstrated at predicting mode structure and frequency at low and low – AC, TAE modes in DIII-D (Van Zeeland'06 APS), JET

(Kramer'05 APS), TAE/GAEs in NSTX (Gorelenkov'03 APS)

*C. Z. Cheng et al, Phys. Reports (A Review Sec. of Phys. Letters.), 211, 1 (1992)†M. S. Chu et al., Phys. Fluids B 4, 3713 (1992)

Page 5: Linear coupling of Alfv én Cascade modes  in NSTX

NSTXNSTX 50th Annual Meeting of the Division of Plasma Physics – Linear coupling of ACs in NSTX (Crocker) Oct. 17-21, 2008

NOVA-K finds shear Alfvén plasma eigenmodes

• Toroidal coupling of poloidal component opens “TAE gap” TAEs live in gap

• AC mode lives above continuum at qmin (region of weak shear)• Weak shear at axis makes core AE AC-like

ACcore AE

qmin location

0 1sqrt(pol)

freq

uenc

y

TAE gap

upper TAE continuum(local shear Alfvén frequency)

lower TAE continuum(local shear Alfvén frequency)

. . .

TAEs

Page 6: Linear coupling of Alfv én Cascade modes  in NSTX

NSTXNSTX 50th Annual Meeting of the Division of Plasma Physics – Linear coupling of ACs in NSTX (Crocker) Oct. 17-21, 2008

NOVA-K used to study AC modes over range of in He L-mode NSTX plasmas

• Reverse shear, lower single null• BTOR = 0.45 T, Ip = 0.8 MA • 2 MW Neutral beam heating

–90 keV, Deuterium

tor at qmin up to 11% (including fast ions)–ne0 ~ 1 – 3.5x1019 m-3, Te0 ~ 0.5 – 1 keV

• ne and Te strongly peaked t = 0.23 sec 123810

123810

t = 0.23 sec 123810

q

4

2

050 100 150

R (cm)

magnetic axis

Page 7: Linear coupling of Alfv én Cascade modes  in NSTX

NSTXNSTX 50th Annual Meeting of the Division of Plasma Physics – Linear coupling of ACs in NSTX (Crocker) Oct. 17-21, 2008

NOVA-K shows NSTX eigenmodes not purely TAEs or ACs*: Eigenmodes formed by linear coupling of AC with TAEs

• Eigenmodes have coupled parts with AC-like or TAE-like structure– AC: dominant component (m,n) at minimum

q, with weak sidebands (m±1,n)– TAE: two dominant components, (m-1,n) at

q = (m-1)/n and (m,n) at q = m/n– Core AE: similar to AC (caused by weak

shear at magnetic axis)• NOVA-K finds multiple eigenmodes with

AC-like structure– closely spaced frequencies– structures differ due to parity of coupled

parts• e.g. core AE couples with positive or negative

parity to rest of eigenmode (see right)

Radial structure of eigenmodecore AE AC mode TAEs

r r

*see also M. A. Van Zeeland et al, Phys. Plasmas 14, 056102 (2007)

Page 8: Linear coupling of Alfv én Cascade modes  in NSTX

NSTXNSTX 50th Annual Meeting of the Division of Plasma Physics – Linear coupling of ACs in NSTX (Crocker) Oct. 17-21, 2008

High enhances linear coupling of ACs to TAEs in NSTX

• Higher gives stronger toroidicity-induced coupling NSTX has stronger coupling than conventional tokamaks

• Linear coupling requires AC to have natural frequency similar to TAEs

• Higher widens TAE gap natural AC and TAE frequencies likelier to be similar 

Page 9: Linear coupling of Alfv én Cascade modes  in NSTX

NSTXNSTX 50th Annual Meeting of the Division of Plasma Physics – Linear coupling of ACs in NSTX (Crocker) Oct. 17-21, 2008

High of NSTX enhances coupling of AC mode to TAEs

scan shows increase elevates continuum near qmin– raises AC frequency into TAE gap

–AC “lives” above continuum (AC frequency depends on continuum frequency)

• Elevation into TAE gap AC couples with TAEs–Linear coupling requires AC to have natural frequencies similar to TAEs

qmin location

TAE gap

Page 10: Linear coupling of Alfv én Cascade modes  in NSTX

NSTXNSTX 50th Annual Meeting of the Division of Plasma Physics – Linear coupling of ACs in NSTX (Crocker) Oct. 17-21, 2008

Effect of linear coupling on eigenmode structure impacts fast-ion transport and experimental detection of AC modes

• Coupled eigenmodes have broader poloidal spectrum– Each poloidal harmonic has fast-ion phase space resonance– resonances can overlap at large amplitude, leading to fast-ion

transport– many harmonics can lead to enhanced transport

• Coupled eigenmodes have increased radial extent– enhances edge B edge Mirnov coils see AC modes*

• Mirnov coils relatively insensitive to ACs in conventional tokamak– eigenmode can perturb fast-ion orbits across large radial region,

enhancing fast-ion transport

*see also M. A. Van Zeeland et al, Phys. Plasmas 14, 056102 (2007)

Page 11: Linear coupling of Alfv én Cascade modes  in NSTX

NSTXNSTX 50th Annual Meeting of the Division of Plasma Physics – Linear coupling of ACs in NSTX (Crocker) Oct. 17-21, 2008

Conclusions

• NOVA-K linear stability code used to calculate shear Alfvén plasma eigenmode structure in NSTX reversed shear plasmas– extends study of Alfvén Cascade (AC) modes to high (ratio of kinetic

and magnetic pressures) and high (inverse aspect ratio, = a/R)

• Eigenmodes not “pure” AC modes  – mode structure shows linear coupling of ACs with toroidicity-induced Alfvén eigenmodes (TAE)

• High and high enhance linear coupling• Coupling gives broad spectrum of poloidal components and

radially extended structure– broad spectrum can lead to enhanced transport – multiple fast-ion

resonances– extended structure enhances edge B, so Mirnov coils see AC

modes – coils relatively insensitive to ACs in conventional tokamaks

Page 12: Linear coupling of Alfv én Cascade modes  in NSTX

NSTXNSTX 50th Annual Meeting of the Division of Plasma Physics – Linear coupling of ACs in NSTX (Crocker) Oct. 17-21, 2008

Future work

• Use ORBIT calculation to assess effectiveness of coupled eigenmodes for causing resonance overlap transport

• Experimentally test effect of coupling on transport: coupling experimentally modifiable by changing AC and TAE natural frequencies:– Vary magnetic shear: edge TAE frequency sensitive to edge q; AC

frequency sensitive to qmin

– Vary toroidal rotation shear: gives relative Doppler shift between TAE in edge and AC in core

– Vary : controls elevation of AC into TAE gap

• Test dependence of coupling with multi-machine “aspect ratio scan”