pke-nefedov symposium - 2004
DESCRIPTION
PKE-Nefedov Symposium - 2004. Optical Diagnostics of Discharge Plasma in PK-4 Project. Alexander Usachev. Institute for High Energy Densities of RAS. Objectives:. 1. Diagnostics of concentrations of excited neon atoms. 2. Developing of combined diagnostic probe-optic methods. - PowerPoint PPT PresentationTRANSCRIPT
PKE-Nefedov Symposium - 2004
Institute for High Energy Densities of RAS
Optical Diagnostics of Discharge Plasma
in PK-4 Project
Alexander Usachev
Institute for High Energy Densities of RAS
1. Diagnostics of concentrations of excited neon atoms.
2. Developing of combined diagnostic probe-optic methods.
3. Control of plasma impurities.
Objectives:
Optical Diagnostics of Plasma in PK-4 Project
Spectral Diagnostics
Glow Image Diagnostics
Institute for High Energy Densities of RAS
Institute for High Energy Densities of RAS
Glow Image Diagnostics
Phantom-5 = 1
Institute for High Energy Densities of RAS
300 350 400 450
0
0.2
0.4
0.6
0.8
1
The spectral transmittance of the PK4-chamber glass.
Institute for High Energy Densities of RAS
0
0
000
)()(
~
eeeek
keek
df
NNZ
Emission Intensity of Ne
0
ik
ekNe NNI ~~
In the case of Te= const,
Intensity vs Electron Density in DC-mode
-10 0 10PK-4 Tube R adius, m m
0
200
400
600
800
Ima
ge
In
ten
sity
, a.
u.
0
1
2
3
4
5
Ele
ctro
n D
en
city
, 1
08
cm-3250 Pa
15 Pa
100 Pa
Institute for High Energy Densities of RAS
mm
Scale
Ne:50 Pa
Institute for High Energy Densities of RAS
Intensity vs Electron Density in DC/RF(i)-mode
-10 -5 0 5 10H , cm
0
4
8
12
16
n e, 1
08 cm
-3, T
e, e
V,
Iin
t, ar
b. u
.
n eTe
In tensity
Intensity Distribution in 2RF(i)-mode
Institute for High Energy Densities of RAS
Temporal Behavior of DC Discharge20000 fps 20 fps
10 Pa
50 Pa
300 Pa
Spectral Diagnostics:
1. Emission spectroscopy: measurements of concentration of highly excited neon atoms.
2. Absorption spectroscopy: measurements of concentration of metastable and resonance neon atoms.
3. Emission spectroscopy: control of plasma impurities.
Institute for High Energy Densities of RAS
Emission spectroscopy: measurements of concentration of highly excited neon atoms
by the method of absolute intensities
Institute for High Energy Densities of RAS
Institute for High Energy Densities of RAS
Emissive spectrum of Ne in DC discharge: 3 mA; 50 Pa.
500 550 600 650 700 750 800W avelength, nm
0
2
4
6
8
10
300 350 400 450 500W avelength, nm
0
2
4
6
8
10
2p 1s
3p 1s
Institute for High Energy Densities of RAS
22121 NhvAP
Emission spectroscopy: measurements of concentration of highly excited neon atoms
by the method of absolute intensities
Absolute concentrations of 2p and 3p levels of neonin RF(i) discharge at 10, 100 and 1000 Pa.
Institute for High Energy Densities of RAS
1 8 1 8 . 5 1 9 1 9 . 5 2 0 2 0 . 5 2 1
E , eV
1e+004
1e+005
1e+006
1e+007
1e+008
N/g
, c
m-3
2p-levels
3p-levels
1000 Pa
100 Pa
10 Pa
Institute for High Energy Densities of RAS
Local Thermal Equilibrium of 2p-levels of Neonin RF(i) discharge at 10, 100 and 1000 Pa
18.3 18.4 18.5 18.6 18.7 18.8 18.9
E, eV
1e+005
1e+006
1e+007
1e+008
N/g
, cm
-3
0.21 eV
0.42 eV
0.55 eV
Tn = 0.026 eV
Te = 3 eV
p=1000 Pa
p=100 Pa
p=10 Pa
Institute for High Energy Densities of RAS
Absorption spectroscopy: measurements of concentration of metastable and resonance
neon atoms by the method of one mirror.
Spectrometertranslation
High voltage CM SM
CM
PMT
C
Lens
PK4 chamber
Mirror
Chopper
PC
Institute for High Energy Densities of RAS
Measurements of concentration of metastable and resonance neon atoms by the method of one mirror.
Institute for High Energy Densities of RAS
Typical Spectrogram.
626 628 630 632 634
W avelength, nm
0
1
2
3
Inte
nsity
, a.
u.
U2
U1
RU
U
lk
eff
11ln
1
1
2
R=0.92
112
2
0
2ln2Nf
cm
ek
eD
For Doppler shape of line:
Institute for High Energy Densities of RAS
16.6 16.65 16.7 16.75 16.8 16.85
E 1, eV
2e+009
4e+009
6e+009
8e+009
1e+010
N1
/ g1
,
cm-3
1 m A , 50 Pa
16.6 16.65 16.7 16.75 16.8 16.85
E 1, eV
1e+008
1e+009
1e+010
N1 /
g 1 ,
cm
-3
5 m A, 50 Pa
16.6 16.65 16.7 16.75 16.8 16.85
E 1, eV
1e+008
1e+009
1e+010
N1
/ g1
,
cm-3
15 m A , 50 P a
IDC = 1 mA
IDC = 5 mA
IDC = 15 mA
Population of 1s-Levels vs Direct Current (at 50 Pa)
Institute for High Energy Densities of RAS
0 4 8 12 16
IDC , m A
0
1e+010
2e+010
3e+010
N3S
, cm
-3
Total Density of Ne-3S Atoms vs Direct Current
4
13
iiiS NgN
Institute for High Energy Densities of RAS
Population of 1s Levels vs Ne Pressure
16.6 16.65 16.7 16.75 16.8 16.85E 1, eV
1e+008
1e+009
1e+010N
1/ g
1, c
m-3
12 Pa, 15 m A
16.6 16.65 16.7 16.75 16.8 16.85E 1, eV
1e+008
1e+009
1e+010
N1/
g1,
cm
-3
25 Pa, 15 m A
16.6 16.65 16.7 16.75 16.8 16.85E 1, eV
1e+008
1e+009
1e+010
N1/ g
1, c
m-3
50 P a, 15 m A
16.6 16.65 16.7 16.75 16.8 16.85E 1, eV
1e+008
1e+009
1e+010
N1/
g1,
cm
-3
100 Pa, 15 m A
p = 12 Pa
p = 25 Pa p = 100 Pa
p = 50 Pa
m m rm m rr
m m rrm m rr
Institute for High Energy Densities of RAS
Emission spectroscopy -Diagnostics of Gas Mixtures:
1. Ne + 2%Xe.
2. Ne + O2.
3. Ne + Air Leakage.
Institute for High Energy Densities of RAS
300 400 500 600 700
W avelength, nm
0
2
4
6
8
10
Intensity, a.u.
300 400 500 600 700
W avelength, nm
0
2
4
6
8
10
Intensity, a.u.
Emission Spectra of pure Ne and Ne+2%Xe-mixture
50 Pa of Ne, 3 mA_433V
50 Pa of Ne+2%Xe, 3 mA_400V
Ne(2p 1s)
Xe(2p 1s)
Institute for High Energy Densities of RAS
Reference Spectra of Pollutants: O2 and N2
200 300 400 500 600 700 800
nm
0
2
4
6
8
10
200 300 400 500 600 700 800
nm
0
0.4
0.8
1.2
1.6
2
H
O2
N2
Institute for High Energy Densities of RAS
UV Reference Spectra of Pollutants: O2 and N2
O2
N2
300 320 340 360 380 400
nm
0
0.4
0.8
1.2
1.6
2
300 320 340 360 380 400
nm
0
2
4
6
8
10
Used O2-band
Institute for High Energy Densities of RAS
OH Spectra of Pollutant H2O
OH
300 310 320 330
0
0.1
0.2
0.3
0.4
0.5
N e (10atm )
300 310 320 330
W avelength, nm
0
0.1
0.2
0.3
0.4
0.5
Intensity, a.u.
N e: N ew _ Ballon 150atm2200V , 50/50m km
Old Ne balloon
New Ne balloon
N2
N2
Emission Spectra of pure Ne and Ne+0.05%O2, Ne+0.15%O2 -mixtures
300 320 340 360 380 400
W avelength, nm
0
1
2
3
4
Inte
nsity
, a.
u.
N e: N ew _ Ballon 150atm2200V , 50/50m km
320 324 328 332 336 340
W avelength, nm
0
0.05
0.1
0.15
0.2
0.25
Inte
nsity
, a.
u.
N e: N ew _ Ballon 150atm2200V , 50/50m km
300 320 340 360 380 400
W avelength, nm
0
1
2
3
4
Inte
nsity
, a.
u.
N e + 0.15O 22200V , 50/50m km
320 324 328 332 336 340
W avelength, nm
0
0.05
0.1
0.15
0.2
0.25
Inte
nsity
, a.
u.
N e + 0.15O 22200V , 50/50m km
300 320 340 360 380 400
W avelength, nm
0
1
2
3
4
Inte
nsity
, a
.u.
N e + 0.05O 22200V , 50/50m km
320 324 328 332 336 340
W avelength, nm
0
0.05
0.1
0.15
0.2
0.25
Inte
nsity
, a.
u.
N e + 0.05O 22200V , 50/50m km
Ne Ne+0.05%O2 Ne+0.15%O2
Institute for High Energy Densities of RAS
O2-bandO2-band
N2-band N2-bandN2-band
Institute for High Energy Densities of RAS
Comparison of Spectroscopic and Probe Datafor Ne, Ne+0.05%O2 and Ne+0.15%O2 -mixtures
0 0.05 0.1 0.15
0
1
2
3
4
5
Spe
ctra
l Int
ensi
ty,
a.u.
0
4
8
12
Ele
ctro
n de
ncity
, 10
7 cm
-3
E
INe
ne
IO2
Institute for High Energy Densities of RAS
320 330 340 350
0
1
2
3
4
5
nn0
320 330 340 350
0
1
2
3
4
5
nn1
320 330 340 350
0
1
2
3
4
5
nn2
320 330 340 350
0
1
2
3
4
5
nn3
320 330 340 350
0
1
2
3
4
5
nn4
320 330 340 350
0
1
2
3
4
5
nn5
Spectral Intensities of Ne, N2 and O2 vs Air Addition
NeNe
Ne
NeNe
NeO2 O2
N2
N2N2
N2
N2
N2
Institute for High Energy Densities of RAS
0 0.01 0.02 0.03
Volum e part o f A ir
0
40
80
120
Spe
ctra
l Int
ensi
ty,
a. u
.Comparison of Spectral and Probe Data Drifts at Air Leakage
0 0.005 0.01 0.015 0.02 0.025
Partia l A ir P ressure in N e
0
2
4
6
8
10
E,
ne,
T
e
E
n e, 1m A
n e, 3m A
T e
O210
Ne
N2
Institute for High Energy Densities of RAS
1..
2..
3..
Conclusion:
Thank you for your attention