Title: PKENefedov Symposium 2004
1PKE-Nefedov Symposium - 2004
Institute for High Energy Densities of RAS
2Objectives
1. Diagnostics of concentrations of excited neon
atoms. 2. Developing of combined diagnostic
probe-optic methods. 3. Control of plasma
impurities.
Institute for High Energy Densities of RAS
3Optical Diagnostics of Plasma in PK-4 Project
Spectral Diagnostics
Glow Image Diagnostics
Institute for High Energy Densities of RAS
4Glow Image Diagnostics
Phantom-5 ? 1
Institute for High Energy Densities of RAS
5The spectral transmittance of the PK4-chamber
glass.
Institute for High Energy Densities of RAS
6Emission Intensity of Ne
Institute for High Energy Densities of RAS
7Intensity vs Electron Density in DC-mode
Ne 50 Pa
Institute for High Energy Densities of RAS
8Intensity vs Electron Density in DC/RF(i)-mode
Institute for High Energy Densities of RAS
9Intensity Distribution in 2RF(i)-mode
10Temporal Behavior of DC Discharge 20000 fps ? 20
fps
10 Pa
50 Pa
300 Pa
Institute for High Energy Densities of RAS
11Spectral 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
12Emission spectroscopy measurements of
concentration of highly excited neon atoms by the
method of absolute intensities
Institute for High Energy Densities of RAS
13Emissive spectrum of Ne in DC discharge 3 mA 50
Pa.
2p ? 1s
3p ? 1s
Institute for High Energy Densities of RAS
14Emission spectroscopy measurements of
concentration of highly excited neon atoms by the
method of absolute intensities
Institute for High Energy Densities of RAS
15Absolute concentrations of 2p and 3p levels of
neon in RF(i) discharge at 10, 100 and 1000 Pa.
1000 Pa
100 Pa
10 Pa
2p-levels
3p-levels
Institute for High Energy Densities of RAS
16Local Thermal Equilibrium of 2p-levels of Neon in
RF(i) discharge at 10, 100 and 1000 Pa
p1000 Pa
p100 Pa
p10 Pa
Institute for High Energy Densities of RAS
17Absorption spectroscopy measurements of
concentration of metastable and resonance neon
atoms by the method of one mirror.
Mirror
Chopper
PK4 chamber
Lens
C
Spectrometer translation
CM
High voltage
PMT
Institute for High Energy Densities of RAS
18Measurements of concentration of metastable and
resonance neon atoms by the method of one mirror.
Institute for High Energy Densities of RAS
19Typical Spectrogram.
R0.92
For Doppler shape of line
Institute for High Energy Densities of RAS
20Population of 1s-Levels vs Direct Current (at
50 Pa)
IDC 5 mA
IDC 15 mA
IDC 1 mA
Institute for High Energy Densities of RAS
21Total Density of Ne-3S Atoms vs Direct Current
Institute for High Energy Densities of RAS
22Population of 1s Levels vs Ne Pressure
p 50 Pa
p 12 Pa
p 25 Pa
p 100 Pa
Institute for High Energy Densities of RAS
23Emission spectroscopy - Diagnostics of Gas
Mixtures
1. Ne 2Xe. 2. Ne O2. 3. Ne Air Leakage.
Institute for High Energy Densities of RAS
24Emission Spectra of pure Ne and Ne2Xe-mixture
50 Pa of Ne, 3 mA_433V
Ne(2p ? 1s)
50 Pa of Ne2Xe, 3 mA_400V
Xe(2p ? 1s)
Institute for High Energy Densities of RAS
25Reference Spectra of Pollutants O2 and N2
O2
H?
N2
Institute for High Energy Densities of RAS
26UV Reference Spectra of Pollutants O2 and N2
O2
Used O2-band
N2
Institute for High Energy Densities of RAS
27OH Spectra of Pollutant H2O
Old Ne balloon
N2
OH
New Ne balloon
N2
Institute for High Energy Densities of RAS
28Emission Spectra of pure Ne and Ne0.05O2,
Ne0.15O2 -mixtures
N2-band
N2-band
N2-band
O2-band
O2-band
Institute for High Energy Densities of RAS
29Comparison of Spectroscopic and Probe Data for
Ne, Ne0.05O2 and Ne0.15O2 -mixtures
ne
INe
E
IO2
Institute for High Energy Densities of RAS
30Spectral Intensities of Ne, N2 and O2 vs Air
Addition
Ne
Ne
Ne
N2
N2
N2
N2
N2
N2
Ne
Ne
Ne
O2
O2
Institute for High Energy Densities of RAS
31Comparison of Spectral and Probe Data Drifts at
Air Leakage
N2
Ne
O2?10
Institute for High Energy Densities of RAS
32Conclusion
1.. 2.. 3..
Institute for High Energy Densities of RAS
33Thank you for your attention