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Millimeter Wave Polarimetry Modeling on NSTX
Jie ZhangN. A. Crocker, W. A. Peebles, T. A. Carter, S. Kubota (UCLA)
W. Guttenfelder (PPPL)and the NSTX Research Team
Joint EU-US Transport Task Force WorkshopSan Diego, CAApril 6-9, 2011
NSTX Supported by
College W&MColorado Sch MinesColumbia UCompXGeneral AtomicsINLJohns Hopkins ULANLLLNLLodestarMITNova PhotonicsNew York UOld Dominion UORNLPPPLPSIPrinceton UPurdue USNLThink Tank, Inc.UC DavisUC IrvineUCLAUCSDU ColoradoU IllinoisU 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
NSTX 2011 TTF–mm-wave polarimetry modeling on NSTX (J. Zhang) Apr. 6-9, 2011, San Diego, CA 2
Results of polarimetry modeling on NSTX
• An interaction between Faraday rotation and Cotton-Mouton effect is clearly identified– Faraday rotation modifies elliptization (Cotton-Mouton effect)
• elliptization is most sensitive to angle between “polarization direction” and “perpendicular magnetic field” in high-field region
• Faraday rotation modifies the “polarization direction”, so it MUST affect elliptization
– Cotton-Mouton effect intrinsically causes polarization rotation
• Polarimetry calculations for Neoclassical Tearing Modes (NTM) and MicroTearing modes (MT) indicate direct B measurements possible– Calculations based on simple magnetic island model show ~0.4°
phase response caused by 0.1% Br of NTM– Calculations based on MT data from GYRO simulation show
polarimeter sensitive to primarily Br for chords near plasma center
~
~
~
NSTX 2011 TTF–mm-wave polarimetry modeling on NSTX (J. Zhang) Apr. 6-9, 2011, San Diego, CA 3
Planned polarimeter for NSTX aims to measure B
• Polarimetry measures change of wave polarization caused by magnetized plasma
• Polarimetry on NSTX can investigate B of various modes– Microtearing modes– (Neoclassical) Tearing modes– Alfvén eigenmodes
• 288 GHz polarimeter planned for NSTX– Horizontal retroreflection from Center
Stack– Polarimetry modeling calculates phase
response for equilibrium and MHD modes– Laboratory testing underway
Faraday rotation:
mirror
polarimeter
nB dlψ ∝ ⋅∫
nB dl nB dlψ ∝ ⋅ + ⋅∫ ∫
~
~
NSTX 2011 TTF–mm-wave polarimetry modeling on NSTX (J. Zhang) Apr. 6-9, 2011, San Diego, CA 4
Model of Polarimetry Calculations
NSTX 2011 TTF–mm-wave polarimetry modeling on NSTX (J. Zhang) Apr. 6-9, 2011, San Diego, CA 5
Assumptions are made to simplify modeling of polarization evolution along wave path
• Cold collisionless plasma model– no dissipation of beam
– relativistic finite temperature polarimetry effects are neglected
• WKB (G. Wentzel, H.A. Kramers, and L. Brillouin) approximation used– plasma parameters is slowly varying
• Ion motion ignored
• Refraction neglected
, ,pi ci pe ceω ω ω ω ω
1 1,d B dnB nk dz k dz
NSTX 2011 TTF–mm-wave polarimetry modeling on NSTX (J. Zhang) Apr. 6-9, 2011, San Diego, CA 6
Polarization properties are characterized by “polarization direction” & “elliptization angle”
Ψ
χ
Ex
Ey
Ψ: polarization direction angle
χ: elliptization angle (+/- sign means Right/Left handedness)
NSTX 2011 TTF–mm-wave polarimetry modeling on NSTX (J. Zhang) Apr. 6-9, 2011, San Diego, CA 7
Modeling treats polarization state as pointon Poincaré sphere
s3
s2
s1
2ψ
2χs
Poincaré sphere
-45o Linear
Horizontal
Vertical
Right Circular
Left Circular
1
2
3
cos 2 cos 2cos 2 sin 2
sin 2
ss s
s
χ ψχ ψ
χ
= =
• Opposing poles represent orthogonal polarizations, e.g.–Horizontal & Vertical linear polarization (s1 poles)–Left- & Right-handed circular polarization(s3 poles)
NSTX 2011 TTF–mm-wave polarimetry modeling on NSTX (J. Zhang) Apr. 6-9, 2011, San Diego, CA 8
Evolution of polarization can be described by a trajectory on Poincaré sphere
( ) ( ) ( )ds z z s zdz
= Ω ×
s3
s2
s1
sΩ
2 2 22
22
1
( ) /1 2 /
21
2 /
x y
pex y
ce
cez
B B B
B B Bc
B B
ωωω ω
ωωω
−
−
−
Ω = −
Cotton-Mouton effect
Faraday Rotation
• Each small step along trajectory is a small rotation of s around Ω axis
• Ω depends on local plasma parameters (electron density, B-field)
• Using realistic NSTX equilibria (Thomson Scattering, EFIT)indicates interaction between Faraday rotation & Cotton-Mouton effect is important to polarization evolution
∆ s
NSTX 2011 TTF–mm-wave polarimetry modeling on NSTX (J. Zhang) Apr. 6-9, 2011, San Diego, CA 9
Interaction between Faraday Rotation &
Cotton-Mouton Effects
NSTX 2011 TTF–mm-wave polarimetry modeling on NSTX (J. Zhang) Apr. 6-9, 2011, San Diego, CA 10
INTERACTION—theoretical approach
• Interaction seen clearly from the geometrical description of polarization evolution – e.g. how s3 (relates to elliptization) changes depends on direction of s
relative to Ω
• Interaction can also be seen from differential expressions– elliptization is sensitive to ψ– Faraday rotation (FR) modifies ψ, so it affects elliptization– Cotton-Mouton effect (CM) also intrinsically causes polarization rotation
1 sin 22
1 tan 2 cos 22
CM
FR CM
d d
d d d
χ ψ δ
ψ ψ χ ψ δ
= = −
2
3 2
eFR
eCM
d n B dz
d n B dz
ψ λ
δ λ ⊥
∝
∝
NSTX 2011 TTF–mm-wave polarimetry modeling on NSTX (J. Zhang) Apr. 6-9, 2011, San Diego, CA 11
Elliptization most sensitive to polarization direction in high-field region
• Initial polarization direction determines direction in high-field region for mid-plane chord–Faraday rotation very weak in mid-plane
• Figure shows elliptization is sensitive to initial polarization direction
horizontal (ψ=0°) and ψ=45° linear launch (mid-plane)(shot# 124764, EFIT01, 0.325 s)
χ,
Ψχχ
NSTX 2011 TTF–mm-wave polarimetry modeling on NSTX (J. Zhang) Apr. 6-9, 2011, San Diego, CA 12
Faraday rotation modifies elliptization
• In general, Faraday rotation & initial polarization direction determine the polarization direction in high-field region
• Figure shows weak elliptization along chord 0.1 m above mid-plane with Faraday rotation, but strong elliptization without–Faraday rotation is counter-clockwise; turned off by setting BD=0
horizontal linear launch with/without Faraday rotation(shot# 124764, EFIT01, 0.325 s)
f = 288 GHz, λ = 1.04 mm
χ,
NSTX 2011 TTF–mm-wave polarimetry modeling on NSTX (J. Zhang) Apr. 6-9, 2011, San Diego, CA 13
Polarimetry Modeling of NTM & MT
NSTX 2011 TTF–mm-wave polarimetry modeling on NSTX (J. Zhang) Apr. 6-9, 2011, San Diego, CA 14
NTM—Realistic magnetic islands structureused in polarimetry modeling
• Magnetic island structure determined using Te profile and USXR
• On NSTX, typical 2/1 magnetic island – island width w ~ 0.1 m– radial location
2/1 magnetic islands
(Both figures courtesy to S. P. Gerhardt)2,1ˆ ~ 0.15r
USXR array
NSTX 2011 TTF–mm-wave polarimetry modeling on NSTX (J. Zhang) Apr. 6-9, 2011, San Diego, CA 15
Polarimetry modeling shows ~0.4° phase response caused by 0.1% Br
• m/n=2/1 island is modeled: (w~0.1 m, )– beam propagates along chord 0.1 m below midplane
• Phase change of |ETOR| modulation is ~0.4° with 0.1%• Phase change dominated by Faraday rotation
– amount of phase change approximately proportional to fluctuation amplitude
m/n=2/1 magnetic island
0 0/rB B
Equilibrium from shot #133959, t=0.882s• Model assumes helically
perturbed B-field around q=m/n rational surface
2,1 ~ 5ˆ 0.1r
2,
2
ˆ( )
( / )
ˆ
0 cos( )m nr
r
rw a
rB B e m nφ−
−
Θ −=
~
NSTX 2011 TTF–mm-wave polarimetry modeling on NSTX (J. Zhang) Apr. 6-9, 2011, San Diego, CA 16
MT—Modeling used to evaluate polarimetry sensitivity to microtearing modes
• Br and ne of microtearing modes from GYRO simulations• Chord heights varied to evaluate polarimetry sensitivity to Br, ne respectively
~0.2% Br /B~ ~1% Br /B
~
+0.2 m +0.2 m
-0.05 m-0.05 m
~ ~~~
GYRO(W. Guttenfelder)
Br(Gauss)
~ ne /n0 ~1%~
NSTX 2011 TTF–mm-wave polarimetry modeling on NSTX (J. Zhang) Apr. 6-9, 2011, San Diego, CA 17
Polarimeter sensitive to primarily Brfor chords near plasma center
~
0.2 m above midplane
nB dl nB dlψ ∝ ⋅ + ⋅∫ ∫
• φ ~1—2°, expected to be detectable~
for chords near plasma center
0B dl⋅
2φ ψ≈
0.05 m below midplane(through plasma center)
NSTX 2011 TTF–mm-wave polarimetry modeling on NSTX (J. Zhang) Apr. 6-9, 2011, San Diego, CA 18
Summary—Results of polarimetry modeling on NSTX
• An interaction between Faraday rotation and Cotton-Mouton effect is clearly identified– Faraday rotation modifies elliptization (Cotton-Mouton effect)
• elliptization is most sensitive to angle between “polarization direction” and “perpendicular magnetic field” in high-field region
• Faraday rotation modifies the “polarization direction”, so it MUST affect elliptization
– Cotton-Mouton effect intrinsically causes polarization rotation
• Polarimetry calculations for Neoclassical Tearing Modes (NTM) and MicroTearing modes (MT) indicate direct B measurements possible– Calculations based on simple magnetic island model show ~0.4°
phase response caused by 0.1% Br of NTM– Calculations based on MT data from GYRO simulation show
polarimeter sensitive to primarily Br for chords near plasma center
~
~
~
NSTX 2011 TTF–mm-wave polarimetry modeling on NSTX (J. Zhang) Apr. 6-9, 2011, San Diego, CA 19
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