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APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida Hard X-ray Diagnostics in the HSX A. E. Abdou, A. F. Almagri, D. T. Anderson, J. N. Talmadge, S. P. Gerhardt, R. R. O’Connell * The HSX Plasma Laboratory, University of Wisconsin-Madison, USA * MST Plasma Laboratory, University of Wisconsin-Madison, USA E-mail: [email protected]

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APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida Outline Abstract HSX Device Parameters. Detector and Hardware Description. Source of fast electrons in HSX. Pulse Height Analysis program. HXR measurement results: Density Scan. Magnetic Configuration Scan. Neutral Pressure Scan. Conclusion.

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Page 1: APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida Hard…

APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida

Hard X-ray Diagnostics in the HSXA. E. Abdou, A. F. Almagri, D. T. Anderson, J. N. Talmadge, S. P. Gerhardt, R. R. O’Connell*

The HSX Plasma Laboratory, University of Wisconsin-Madison, USA* MST Plasma Laboratory, University of Wisconsin-Madison, USA

E-mail: [email protected]

Page 2: APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida Hard…

APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida

AbstractA. E. Abdou, A. F. Almagri, D. T. Anderson, J. N. Talmadge, S. P. Gerhardt, R. R. O’Connell*

The HSX Plasma Laboratory, University of Wisconsin-Madison, USA* MST Plasma Laboratory, University of Wisconsin-Madison, USA

E: [email protected]

In the Helically Symmetric eXperiment (HSX), electrons are ECRH heated using 28 GHz, 2nd harmonic gyrotron. The normal configuration is Quasi-Helical Symmetric (QHS), it has a dominant n=4, m=1 components in the magnetic field spectrum. With a set of auxiliary coils, the quasihelical symmetry can be broken (MIRROR, HILL and WELL, modes). In this work the resolved hard X-ray emission in the HSX is analyzed using CdZnTl detector (1 s shaping time, Gain =50). The detector is housed is a lead box adjacent to the vacuum vessel, with 0.8 mm pinhole and 200 m SS filter placed in front of the detector. The hard X-ray pulse height spectrum was accumulated in a series of similar ECRH discharges. The behavior of the fast electrons has been studied for densities in the range of 0.2 to 0.9 x 1012 cm-3. The magnetic configuration has also been altered between QHS and MIRROR, and ANTI-MIRROR modes in order to determine the effect of magnetic ripple on characteristic energies and densities of fast electrons. Pulse height analysis of hard x-ray emission shows the presence of X-ray photons with energies as high as 650 KeV. Hard X-ray emission is strong function of plasma density; where at low density (0.2 x 1012 cm-3 ) the intensity is ~80 times higher than at higher density (0.9 x 1012 cm-3) for QHS mode. The hard X-ray intensity is higher in the QHS than in the MIRROR mode. Also the high energy tail of the spectrum extends to higher energies in QHS (~ 650 KeV). Future work will involve:transport calculation to determine fast electron energy distribution.

*This work is supported by US DOE grant number DE-FG02-93ER54222.

Page 3: APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida Hard…

APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida

Outline• Abstract• HSX Device Parameters.• Detector and Hardware Description.• Source of fast electrons in HSX.• Pulse Height Analysis program.• HXR measurement results:

Density Scan.Magnetic Configuration Scan.Neutral Pressure Scan.

• Conclusion.

Page 4: APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida Hard…

APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida

Conclusion• Hard X-ray signal last for at least 50 ms after the ECRH is turned off

indicating good confinement of fast electrons.

• Hard X-ray emission is a strong function of plasma density; where at low density (0.2 x 1012 cm-3) the intensity is ~80 times higher than at high density (0.9 x 1012 cm-3 ).

• Hard Hard X-ray intensity is very low in ANTI-MIRROR mode at all plasma densities (poor confinement).

• The hard X-ray spectrum extends to energies as high as 650 keV in the QHS mode.

• Increasing the neutral base pressure beyond 4.4 x 10-6 suppress the fast electrons that are produced by toroidal voltage.

Page 5: APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida Hard…

APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida

HSX Device ParametersMajor Radius 1.2 m

<r> 0.11 m

Volume ~.44 m3

Field Periods 4

iaxis 1.05

iedge 1.12

Coils/period 12

B0 (max.) 1.25 T

Magnetic Field Flattop Length

0.2 s

Auxiliary Coils 48

Page 6: APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida Hard…

APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida

QHS, MIRROR and ANTI-MIRROR Modes• QHS and

Mirror have different magnetic field spectra...

…but similar well depth, rotational transform, surface shape, and plasma volume.

QHS

n=4, m=1

Mirror

n=4, m=0

n=4, m=1

Page 7: APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida Hard…

APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida

Sources of Fast Electrons in HSX

Fast electrons in HSX are generated from two different mechanisms1- dB/dt source2- ECRH Heating source

780 800 820 840 860 880 900-4

-2

0

2

4

6

8

10

12

14

Time (ms)

HXR

Sig

nal (

Volts

)

HXR signal preionization off (Filament off)HXRECRH * 4Density/1.0E+11

780 800 820 840 860 880 900-2

0

2

4

6

8

10

12

14

Time (ms)H

XR S

igna

l (Vo

lts)

HXR signal with preionization (Filament On)HXRECRH * 4Density/1.0E+11

Page 8: APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida Hard…

APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida

Loop Voltage in HSX

• Loop Voltage time variation which gives rise to dB/dt source

0 1 2 3 4 5 6 7-0.2

0

0.2

0.4

0.6

0.8

1

1.2Poloidal Flux Change (2 toroidal turns)

Shot Time (s)

Loop

Vol

tage

(V)

Page 9: APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida Hard…

APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida

Detector• Detector Type: CdZnTl• Detector Characteristics:

Dimension: 10x10x2 mmPeak/Valley: > 8:1 @ 59.5 KevResolution: < 10% (6 KeV)@ 59.5 KeV (FWHM)Peak/Valley: > 3:1 @ 122 KevResolution: < 6% (8 KeV)@ 122 KeV (FWHM)Peak/Valley: > 1.8:1 @ 622 KevResolution: < 3% (20 KeV)@ 622 KeV (FWHM)

Page 10: APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida Hard…

APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida

Detector (continue)

• The detector has a built in pre-amplifier, it is connected to a high voltage power supply, and an Ortec EG&G 671 amplifier.

• The amplifier output signal is then connected to a data acquisition system.

• The raw signal is then processed using a pulse height analysis program.

Page 11: APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida Hard…

APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida

Detector Calibration

Page 12: APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida Hard…

APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida

Filter Transmission

I(x) = Io e - x

Transmission = I(x) / Io= e - X

Where: X = 200 m , Fe = 7.874 gm/cm2 and Fe mass absorption coefficient for Fe (cm2/gm)Transmission is calculated from the above formula using tabulated values for Fe (from

(http://physics.nist.gov/PhysRefData/FFast/html/form.html )

Page 13: APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida Hard…

APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida

Pulse Height AnalysisThe pulse height analysis program is written in IDL. The program mainly evaluate the following:1- Resolving the Gaussian signals (single & double).2- Least square fitting for the signals3- Spectral Analysis of the signal4- Calculation of the electron Temperature

Page 14: APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida Hard…

APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida

Pulse Heights Analysis (continue)

Page 15: APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida Hard…

APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida

HXR Spectrum at Low Density (QHS mode)

HXR Spectrum for QHS mode (n = 2x1011 cm-3)

y = 347.45 - 0.0046 xR 2 = 0.9706Temperature = 217.39 +/- 1.85 keV

1

10

100

1000

0 200 400 600 800 1000 1200 1400Energy (keV)

dN/d

E (M

eV -1

)

Page 16: APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida Hard…

APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida

HXR Spectrum at intermediate density (QHS mode)

HXR Spectrum for QHS mode (n = 5x10 11 cm -3)

y = 76.768 - 0.0061xR2 = 0.9443Temperature = 163.93 +/- 1.85

1

10

100

0 200 400 600 800Energy (keV)

dN/d

E (M

eV -1

)

Page 17: APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida Hard…

APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida

HXR Spectrum at High density (QHS mode)

HXR Spectrum for QHS mode (n =9x1011 cm-3)

1

10

100

0 50 100 150 200 250 300 350 400Energy (keV)

dN/d

E (M

eV -1

)

Page 18: APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida Hard…

APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida

HXR Spectrum at Low density (MIRROR mode)

HXR Spectrum for Mirror mode (n =2x1011 cm-3)

y = 16.53 - 0.0047xR 2 = 0.8209Temperature = 212.77 +/- 2.11

1

10

100

0 100 200 300 400 500 600Energy (keV)

dN/d

E (M

eV -1

)

Page 19: APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida Hard…

APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida

HXR Spectrum at Intermediate density (MIRROR mode)

HXR Spectrum for Mirror mode (n =6x1011 cm-3)

y = 134.06e -0.0062x

R 2 = 0.9735Temperature = 161.29 +/- 1.76

1

10

100

1000

0 200 400 600 800Energy (keV)

dN/d

E (M

eV -1

)

Page 20: APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida Hard…

APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida

HXR Spectrum at High density (MIRROR mode)

HXR Spectrum for Mirror mode (n =9x1011 cm-3)

1

10

100

0 100 200 300 400 500Energy (keV)

dN/d

E (M

eV -1

)

Page 21: APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida Hard…

APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida

HXR Spectrum at Low density (ANTI- MIRROR mode)

HXR Spectrum for Anti-Mirror mode (n = 2x1011 cm-3)

1

10

0 100 200 300 400 500Energy (keV)

dN/d

E (M

eV -1

)

Page 22: APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida Hard…

APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida

HXR Spectrum at Intermediate density (ANTI-MIRROR mode)

HXR Spectrum for Anti-Mirror mode (n =5x1011 cm-3)

1

10

0 100 200 300 400 500Energy (keV)

dN/d

E (M

eV -1

)

Page 23: APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida Hard…

APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida

HXR Spectrum at High density (ANTI-MIRROR mode)

HXR Spectrum for Anti-Mirror mode (n =9x1011 cm-3)

1

10

0 100 200 300 400 500Energy (keV)

dN/d

E (M

eV -1

)

Page 24: APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida Hard…

APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida

Summary

• Hard X-ray emission is strong function of plasma density; where at low density (0.2 x 1012 cm-3) the intensity is ~80 times higher than at high density (0.9 x 1012 cm-3 ).

• The HXR spectrum extends to energies as high as 650 keV.

Number of Counts Vs Density for Different Magnetic Configuration

1.0

10.0

100.0

1000.0

10000.0

0.0E+00 2.0E+11 4.0E+11 6.0E+11 8.0E+11 1.0E+12Density (cm-3)

Num

ber o

f Cou

nts

QHSAnti_MirrorMirror

Page 25: APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida Hard…

APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida

Base Pressure Scan

0 500 1000 1500 2000 2500 3000 3500-2

0

2

4

6

8

10

Time (ms)

HXR

Sig

nal (

Volts

)

HXR signal (Base pressure = 7.5 E-08)HXR

0 500 1000 1500 2000 2500 3000 3500-2

0

2

4

6

8

10

Time (ms)H

XR S

igna

l (Vo

lts)

HXR signal (Base pressure = 5.6 E-07)HXR

Increasing the tank base pressure decreases the the HXR intensity

Page 26: APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida Hard…

APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida

Base Pressure Scan (Continue)

0 500 1000 1500 2000 2500 3000 3500-2

0

2

4

6

8

10

Time (ms)

HXR

Sig

nal (

Volts

)

HXR signal (Base pressure = 6.5 E-07)HXR

0 500 1000 1500 2000 2500 3000 3500-1

-0.8

-0.6

-0.4

-0.2

0

0.2

0.4

0.6

0.8

1

Time (ms)H

XR S

igna

l (Vo

lts)

HXR signal (Base pressure = 4.4 E-06)

HXR

Increasing the tank base pressure beyond 4.4 x 10-06 will suppress the fast electrons (No HXR signal)

Page 27: APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida Hard…

APS, 44th Annual Meeting of the Division of Plasma Physics November 11-15, 2002; Orlando, Florida

Conclusion• Hard X-ray signal last for at least 50 ms after the ECRH is turned off

indicating good confinement of fast electrons.

• Hard X-ray emission is a strong function of plasma density; where at low density (0.2 x 1012 cm-3) the intensity is ~80 times higher than at high density (0.9 x 1012 cm-3 ).

• Hard Hard X-ray intensity is very low in ANTI-MIRROR mode at all plasma densities (poor confinement).

• The hard X-ray spectrum extends to energies as high as 650 keV in the QHS mode.

• Increasing the neutral base pressure beyond 4.4 x 10-6 suppress the fast electrons that are produced by toroidal voltage.