This document summarizes research characterizing and optimizing an electron cyclotron resonance ion source (ECRIS). Key findings include:
1) X-ray spectroscopy showed the electron distribution in the plasma varies with parameters like RF power, pressure, and bias voltage. The ion charge state distribution is also affected.
2) Emittance measurements of the extracted ion beam found values around 0.166 mm-mrad, depending on beamline optics. Better emittance may be possible with improved measurement techniques.
3) While bias enhanced the charge states extracted, it did not change the underlying plasma properties. Gas mixing also impacted the ion current.
In summary, extensive testing optimized the ECRIS
This paper compares the performances of standard surrogate models in the development of an optimal control framework. The optimal control strategy is implemented on an Active Thermoelectric (ATE) window design. The ATE window design uses thermoelectric units to actively regulate the overall thermodynamic properties of the windows. The optimization of the design is a multiobjective problem, where both the heat transferred through the window and electric power consumption are minimized. The power supplies and the heat transfer are optimized under a reasonable number of randomly sampled environmental conditions. The subsequent optimal designs obtained are represented as functions of the corresponding environmental conditions using surrogate models. To this end, four types of surrogate models are used, namely, (i) Quadratic Response Surface Methodology (QRSM), (ii) Radial Basis Functions (RBF), (iii) Extended Radial Basis Functions (E-RBF), and (iv) Kriging. Their performances are compared using two accuracy measurement metrics: Root Mean Squared Error (RMSE) and Maximum Absolute Error (MAE). We found that any one of the surrogate modeling methods is not superior to the others over the whole domain for the optimal control of the ATE window.
First results from the full-scale prototype for the Fluorescence detector Arr...Toshihiro FUJII
The Fluorescence detector Array of Single-pixel Telescopes (FAST) is a design concept for the next generation of ultrahigh-energy cosmic ray (UHECR) observatories, addressing the requirements for a large-area, low-cost detector suitable for measuring the properties of the highest energy cosmic rays. In the FAST design, a large field of view is covered by a few pixels at the focal plane of a mirror or Fresnel lens. Motivated by the successful detection of UHECRs using a prototype comprised of a single 200 mm photomultiplier-tube and a 1 m2 Fresnel lens system [Astropart.Phys. 74 (2016) 64-72], we have developed a new full-scale prototype consisting of four 200 mm photomultiplier-tubes at the focus of a segmented mirror of 1.6 m in diameter. In October 2016 we installed the full-scale prototype at the Telescope Array site in central Utah, USA, and began steady data taking. We report on first results of the full-scale FAST prototype, including measurements of artificial light sources, distant ultraviolet lasers, and UHECRs.
35th International Cosmic Ray Conference — ICRC2017 18th July, 2017
Bexco, Busan, Korea
This paper compares the performances of standard surrogate models in the development of an optimal control framework. The optimal control strategy is implemented on an Active Thermoelectric (ATE) window design. The ATE window design uses thermoelectric units to actively regulate the overall thermodynamic properties of the windows. The optimization of the design is a multiobjective problem, where both the heat transferred through the window and electric power consumption are minimized. The power supplies and the heat transfer are optimized under a reasonable number of randomly sampled environmental conditions. The subsequent optimal designs obtained are represented as functions of the corresponding environmental conditions using surrogate models. To this end, four types of surrogate models are used, namely, (i) Quadratic Response Surface Methodology (QRSM), (ii) Radial Basis Functions (RBF), (iii) Extended Radial Basis Functions (E-RBF), and (iv) Kriging. Their performances are compared using two accuracy measurement metrics: Root Mean Squared Error (RMSE) and Maximum Absolute Error (MAE). We found that any one of the surrogate modeling methods is not superior to the others over the whole domain for the optimal control of the ATE window.
First results from the full-scale prototype for the Fluorescence detector Arr...Toshihiro FUJII
The Fluorescence detector Array of Single-pixel Telescopes (FAST) is a design concept for the next generation of ultrahigh-energy cosmic ray (UHECR) observatories, addressing the requirements for a large-area, low-cost detector suitable for measuring the properties of the highest energy cosmic rays. In the FAST design, a large field of view is covered by a few pixels at the focal plane of a mirror or Fresnel lens. Motivated by the successful detection of UHECRs using a prototype comprised of a single 200 mm photomultiplier-tube and a 1 m2 Fresnel lens system [Astropart.Phys. 74 (2016) 64-72], we have developed a new full-scale prototype consisting of four 200 mm photomultiplier-tubes at the focus of a segmented mirror of 1.6 m in diameter. In October 2016 we installed the full-scale prototype at the Telescope Array site in central Utah, USA, and began steady data taking. We report on first results of the full-scale FAST prototype, including measurements of artificial light sources, distant ultraviolet lasers, and UHECRs.
35th International Cosmic Ray Conference — ICRC2017 18th July, 2017
Bexco, Busan, Korea
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Master thesis: Characterization and Optimization of an Electron Cyclotron Resonance Ion Source
1. Characterization and Optimization of an Electron
Cyclotron Resonance Ion Source
J.Rabinder Henry
External: Dr. Stefhan Facsko(FZR Rossendorf)
Dip-Ing. Gerald Staats
Professor: Prof. Dr.-Ing. Christian Schäffer
2. Outlook
• Introduction
Electron Cyclotron Resonance Ion Source (ECRIS)
FZR 14.5 GHz source
• Characterization and Optimization
Plasma –X-ray Spectroscopy
Results
• Beam Emittance
Results
• Summary and outlook
3. RFce meB ωω == /
Principle of ECRIS
●Electron Cyclotron Resonance Heating
●Electron impact ionization
●Magnetic confinement
Magnetic Field
FZR 14.5 GHz Supernanogan
RF Power
3
RF Power
ECR Zone
Gas Inlet
ECR Source Working Principle
Extraction Electrode
Electron Cyclotron Emission
5. RF Power (x)
Pressure (y)
Biased disc (z)
I extracted (Iex)ECRIS
Characterization and Optimization
Max f (Iex) = min (x, y, z)
5
Gas mixing (a)
Plasma Characterization
X-ray Spectroscopy
Ion beam quality
Emittance
Electron Distribution
Charge State Distribution } Source Parameters
x, y, z, a
6. X-ray Spectroscopy
Electron –Bremsstrahlung Measurement
Ion charge state –Characteristics X-ray Measurement
Germanium Detector Attenuation of Radiation
Be window
Air column
Collimation
Extraction Voltage
6
Analyzing
Magnet
HPGe Detector
ECRIS
Faraday Cup
Beryllium
Window
19. X-ray Spectra For Varying Bias
6000
8000
10000
XeLSeries
Counts
-50V
-250V
-400V
-600V
Xenon plasma
Pressure1.03 x 10-4 mbar
Power 100 W
19
0 10000 20000 30000 40000
0
2000
4000
XeKSeries
Counts
E (eV )
20. 200 0
FeKα
CuKα1,2
β
XeLα1,2
Counts
X e 27 % /O 2 0%
X e 27 % /O 2 1.50%
X e 27 % /O 2 5.20%
X-ray Spectra For Gas Mixing
Xenon and Oxygen
Pressure 1.6x 10-6 mbar
Power 100 W
Bias voltage -200 V
20
0 10000 2000 0 300 00 4 0000
0
100 0
XeKβ
CuKβ
FeKβ
XeLβ
Counts
E (eV )
22. 200 250 300 350 400 450 500
0
20
40
60
80
Ar9+
Ar8+
Ar7+
Ar6+
Ar5+
Ar4+
Ar3+
Ar2+
IextracteduA
B m T
1x10
-5
m bar
1x10
-4
m bar
5x10
-5
m bar
Mass Spectra For Varying Pressure
Argon
Power 100 W
Bias voltage -400 V
22
B m T
2 3 4 5 6 7 8 9
0
20
40
60
80
IuA
Charge State
1x10
-5
mbar
5x10
-5
mbar
1x10
-4
mbar
Charge State Distribution
23. 200 250 300 350 400 450 500
0
10
20
30
40
50
60
70
80
Ar2+
Ar3+
Ar4+
Ar5+
Ar6+
Ar7+
Ar8+
Ar9+
IextracteduA
0V
-400V
-200V
Mass Spectra For Varying Bias
Argon
Power 100 W
Pressure 1x 10-4 mbar
23
B m T
1 2 3 4 5 6 7 8 9 10
0
10
20
30
40
50
60
70
80
IuA
C harge State
Ar
0V
-200V
-400V
Charge State Distribution
25. 0 2 4 6 8
0,0
0,2
0,4
0,6
0,8
1,0
1,2
FCCurrentmA
Slit Position mm
Slit +X
Slit -X
Slit +Y
Slit -Y
-x
+x
Z
+y
-y
Emittance Measurement
250 2 4 6 8 10 12 14 16
0,00
0,05
0,10
0,15
0,20
0,25
Peak3
Peak 2
Peak1
M1S1
dI/dx
Current Profile
σ =0.24149
σ =0.40832
σ =0.35993
σ =0.4551
RelativeIntensitymA
Slit position mm
Pea
ks
Peak width
2σ mm
Peak half width
σ mm
Divergenc
e Angle α
Phase
space
area
2σ* α
mmrad
1 0.72 0.36 0.147 0.001
2 0.92 0.46 0.188 0.003
3 0.80 0.40 0.163 0.002
Mea
n = 0.81 = 0.40
=0.166
0.002
26. Summary
Plasma
Two different population of electrons below 30 keV and 100 keV
Stable plasma at nominal power
Unstable plasma at very low pressure
Charge state distribution
Enhanced with bias voltage but no change in plasma characteristics
Ion current extracted depends on gas mixing ratio
Emittance
26
Emittance
Ion beam emittance depends on extraction and beam line elements
Outlook
Longmuir probe measurements
Better emittance with pin hole and CCD camera