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Shin KUBO, Masaki NISHIURA, Kenji TANAKA, Takashi SHIMOZUMA, Yasuo YOSHIMURA, Hiroe IGAMI,
Hiromi TAKAHASHI, Takashi MUTOHNational Institute for Fusion Science
Collective Thomson Scattering Study using Gyrotron in LHD
Research Center for Development of FIR Region, Univ. of FukuiYoshinori TATEMATSU, Teruo SAITO
Namiko TAMURA,Dept. Energy Science & Technology, Nagoya Univ.
US-Japan Workshop on RF Physics2010.03.8-10 General Atomics, San Diego
Contents
•ECRH System in LHD --> Potential as a diagnostic tool•Collective Thomson Scattering•Receiver•Preliminary results•Scattering Volume and CTS spectrum•Sub-Tera Hz Gyrotron Development•Future Plan•Summary
ECRH System
Design of the Antenna System of ECRH in LHD
• Two sets of upper antennas from 5.5U and 9.5 U port for 82.7GHz and 168GHz
• Two 84 GHz Antenna from 1.5 L port
• All antennas can focus and deposit the power within r<0.2 for Rax=3.53m,B=2.951 T
• Antenna Scan Range– U antenna
• R=-3.2-3.8m, t=±0.2m on mid plane
– L antenna• R=-3.0-4.2m,t= ±1.5m
6
Elliptical Gaussian Beam Focusing Scheme
168GHz Beam
SteeringMirror
FocusingMirror
from Waveguides
84GHz Beam
SteeringMirror
FocusingMirror
mid-plane Focusing MirrorBi-focal Mirror
Waveguide mouth
Hot test of beam steering/focusing• Errors of steering for tor/rad-directions notably affect deposition profile• Beam steering/focusing were checked in vacuum vessel of LHD by using
Kapton film and IR-camera.
ECRH Beam as a Scattering Probe Beam• Well defined beam for heating is also suitable
for probe beam for scattering measurement.– High power density, High Frequency
Modulation• Good S/N Ratio
– Controllable• Scattering Cross Section Position• Scattering Angle
• Promising Candidate for– Density Fluctuation Measurement
• Structure study of micro-turbulence– Wave detection
• EC wave, LH wave, IC wave, Alfven wave– Collective Thomson Scattering
• Ion temperature measurement• Alpha particle distribution study
EC wave, LH wave, IC wave, Alfven wave
9
Collective Scattering using
ECRH System
10
Collective Scattering Condition
3
θ =10 deg θ =90 deg
11
LHD ECH Antenna Configuration (2008)
9.5U Antennaout 82.7 GHzin 77 GHz
5.5U Antennaout 82.7 GHzin 168 GHz
1.5L Antennaout 84 GHzin 84 GHz
2-O Antennaright 77 GHzleft 168 GHz
3.5 inch corrugated WG
3.5 inch corrugated WG
3.5 inchcorrugated WG
1.25 inch corrugatedWG
12
LHD ECH Antenna used for probe and receiving beams
3
9.5U Antennaout 82.7 GHzin 77 GHz
5.5U Antennaout 82.7 GHzin 168 GHz
1.5L Antennaout 84 GHzin 84 GHz
2-O Antennaright 77 GHzleft 168 GHz
3.5 inch corrugated WG
3.5 inch corrugated WG
3.5 inchcorrugated WG
1.25 inch corrugatedWG
waist size 0.015 mwaist size 0.02 m 0.8 MW/5s, 0.24 MW/CW
13
Present ECRH System in LHD
•Two sets of transmission line/ antenna are installed on the ports. •9.5U, 5.5U 1.5L and 2O
14
Proposed Scattering Probe/Receiving transmission Line
•A set of transmission line/ antenna on the 9.5U port is used for CTS.•A line which 77GHz 1MW power available is used for probe beam
15
Receiver Setting Configuration
16
Attached Receiver System
plasma
f0+df
f0+df+fs
gyrotrondf~200MHz
power monitor
ECRH Transmission line(corrugated waveguide)
fixed local oscillatorstability < 10 MHz
pin SW
Notchfilter
Att. BPF
WG SW
Filtek HPF
fl=78 GHz
Mixer
A1
A2A3
Isolator
Two way divider 1
Two way divider 2
high freq.
low freq.
500-200
900-200
1300-200
1700-200
1900-100
2100-100
2300-100
2500-100
Four way divider Diodes
Video Amps.(x1000)
monitor port
measure port
A1: Cernex CBLU1103030-01A2: Cernex CBLU1103050-01A3: Amplitek apt4_SN104331
Heterodyne Receiver for Collective Thomson Scattering in LHD (2008)
Filter CombinationLocal Oscillator 74 GHz
•Filter combination•Center freq.
•IF 3 GHz•sensitive low freq. IF
•for high energy ions•narrow band dense near center freq. IF
•for bulk ion•wide band sparse at peripheral IF
•for high energy ions
Actual Receiver Configuration
IF Amps.
WaveguideSwitch
Splitters
Filters
Mixer
Local Oscillator
PIN Switch
Notch Filter
Horn Antenna
Waveguidefor Probe
Beam
From 77 GHz Gyrotron
During the first trial of CTS measurement,the local oscillator of 74 GHzwas damaged,
Actual Filter Combination
and switched tentatively to78 GHz Courtesy of Dr. T. Tokuzawa
Ch.1,4,5 double side bandCh.2,3,6-8 lower side band
Background, calib.
CTS componentAll channel lower side band Ch2,3 almost notched
10-3
10-2
10-1
100
0 1 2 3 4 5 6 7 8 9
%) /# &)*312!( $,( "'.0-/, '.+, &)*312 !( $,( "
Cal.
Fact
or(V
/eV)
Channel
2009.01.23ΔT=210 deg. lock-in factor=3.0
Effect of Notch Filter
Actual Filter Combination and Calibration with Liq N2
78GHz local combination
Measured Notch FilterCharacteristics Courtesy of Prof. A. Mase
FilterCharacteristics Courtesy of Prof. Y. NagayamaDr. T. YoshinagaMr. D. Kuwabara
Actual Measurement Configuration
B=2.75 TR=3.6 mrho=0.7±0.2k ~ perpendicular
25
Preliminary Results
✴B=2.75T, R=3.6m✴Fundamental ECRH Plasma
Fundamental ECRH plasma ✴B=2.75T, R=3.6m✴Fundamental ECRH Plasma• Noise well suppressed•Spikes at every modulation turn-on, off
•due to spurious mode oscillation from gyrotron•removable by pin switch
Fundamental ECRH plasma (double side band factor)
Expanded in time (#91758)
Expanded in time (#91758)
CTS #91758 (double side band factor)
✴B=2.75T, R=3.6m✴Fundamental ECRH Plasma• Noise well suppressed•Spikes at every modulation turn-on, off
•due to spurious mode oscillation from gyrotron•removable by pin switch
CTS #91758 (double side band factor)
✴B=2.75T, R=3.6m✴Fundamental ECRH Plasma• Noise well suppressed•Spikes at every modulation turn-on, off
•due to spurious mode oscillation from gyrotron•removable by pin switch
Analysis ECRH plasma
Decompositionof scattering
component from heating/heat
wave componentis necessary
Method of analysis• Raw data of several modulation periods are
rearranged in time relative to the turn on/off time
• These rearranged data are fitted with the function
• δa corresponds to background increments/decrements due to heating (change in slope)
• δb corresponds to increment/decrement due to scattered signal over background (stepwise change)
Example of deduced raw signal change
Spectrum change in time
Example of deduced scattered power spectrum
36
Receiver Improvements
Heterodyne Receiver for Collective Thomson Scattering in LHD (2009)
fixed local oscillatorstability < 10 MHz
pin SW
Notchfilter
Att.
BPF
WG SW
fl=74 GHz
MixerIsolator
HPF
A1 A2
A3
A4A4
A4A4
A4A4
A4A4
A3
n
ECRH Transmission line(corrugated waveguide)
5th-HarmonicMixer
n
fl1-ndf
A5
HPF
Att A5
HPF *
HarmonicMixer
Error AmpVoltage Controlled
Oscillator
plasma
f0+df
f0+df+fs
gyrotrondf~200MHz
power monitor
ADC
ADC
ADC
ADC
32 channel VideoAmp.(x100)
LPF
Filters
Low NFAmps
PowerAmps
2<f<8GHz
f<6GHz
f>0.3GHz
0.5<f<4GHz
0.5<f<18GHz
Increased IF bands local frequency = 74.00 GHz
IF filter characteristics
40
Scattering Volume• Key to confirm scattering signal
confirmation• Necessary for absolute calibration
Beam Cross Section Controlled by beam steering
receiving beamprobing beamprobing beam receiving beam
ρ=1.0
ρ=0.19.5U in 77GHz injection9.5U out receiving
Max cross section at ρ=0.75 Zero cross section
• Scattering power
is obtained using scattering form factor
Γ: geometrical factorre: classical electron radiusne: electron densitydω: band widthrR: beam radiusλs0: wavelength of scattered
radiationS(k,ω): scattering form factor
Probebeam
Scatteredbeam
fromGyrotron
toReceiver
SN ratio of CTS
43
Scattered Power
U-antenna for 168 GHz used for 77 GHz Scattering
•Beam evolution is recalculated with the 168 GHz antenna mirror configuration radiated from the same waveguide mouth for 77 GHz beam •Resultant beam sizes on the mid-plane are •20 mm in radial •99 mm in toroidal
If the configuration of the mirrors and optical axis are the same,i. e. cosφ and ρ are kept ,relation between Rin and Rout are defined by
even for different frequency, or beam size
77 GHz168 GHz
bi-focal mirrorfinal focus mirror
7777
45
Scattering using Gaussian Beam
46
Cross Volume of Gaussian Beam
47
Surface of Cross Volume
48
Cross Volume and resolution
49
Scattering using Gaussian Beam
Scattering Length
50
Scattered intensity and effective scattering length well scale
center
top
bottom
Scattered spectrum are fitted with offset-Gaussian to subtract ECE background
Intensity ratio of the scattered power well scales to the calculated effective scattering length
Comparison of Exp. / Cal. Spectrum
51
Measured data are used for calculation.• Te=0.6keV• TAr=0.7keV• ne=2.5x1019m-3
• nfast=0.1x1019m-3
• Ti=0.7keV is better fitting than Ti=2keV.
• Measured data seems to have an offset of +0.1GHz.
• P(3.6,0,0), R(3.6,0,0)• Vsc=153.3cm3
1
10
100
1000
-3 -2 -1 0 1 2 3
Calculated CTS spectrumscattered radiation
Scat
tere
d Po
wer
(eV)
frequency (GHz)
52
Sub-Tera Hz Gyrotron
Development
FIR FUCTS in LHD
fi > 4fce suppression of ECE400 GHz band is one choice. Salpeter Parameter
Linked with slide 15
R along scattered wave path (m)
FIR FU
Achieved 50 kW
• More than 50 kW at 349 GHz and about 40 kW at 390 GHz have been achieved. These are highest powers as second harmonic oscillation of gyrotron.
• Oscillation efficiency decreases for large beam current possibly due to degradation of the quality of the electron beam.
From Notake PRL paper
Vk = 57 kV
Future Plan• Establish Calibration/Analysis procedure
• Scattering Volume
• CTS spectrum and reduction of ion/fast ion temperature
• Calibration including polarizer/waveguide coupling
• Multi receiver / fast volume scan• Precise background subtraction
• Simultaneous measurement in 2-D velocity space
• Expansion in real/velocity space
• Sub-Tera Hz Gyrotron Application to CTS
57
LHD ECH Antenna used for probe and receiving beams
3
9.5U Antennaout 82.7 GHzin 77 GHz
5.5U Antennaout 77 GHzin 168 GHz
1.5L Antennaout 84 GHzin 84 GHz
2-O Antennaright 77 GHzleft 168 GHz
3.5 inch corrugated WG
3.5 inch corrugated WG
3.5 inchcorrugated WG
1.25 inch corrugatedWG
waist size 0.03 m 0.8 MW/5s, 0.24 MW/CW
ECRH Horizontal Antennafor parallel component
• 2 sets of• Focusing Mirror
• Symmetric Gaussian Beam
• 35 mm waist size at plasma center
• Steering Plane Mirror• Toroidally +/- 30
degree• Poloidally +/- 10
degree
Summary•Started CTS utilizing ECRH system in LHD77GHz ( P~1MW) Gaussian beam is used as a probe.Injection ECRH antenna is used as a receiver. Backward, perpendicular 8/32 channel receiver system is attached to ECRH transmission line 3 s, 50 Hz modulated injection at 0.7 MWPreliminary results with 8/32 channel show promising CTS signals
•32 channel•Higher reliability in ion velocity distribution reduction
•Examining possible use of horizontal antennas•Backward, parallel components
•Sub-THz gyrotron developed for CTS in LHD