In situ Elastic Recoil Detection Analysis of Tungsten Surfaces - - PowerPoint PPT Presentation

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In situ Elastic Recoil Detection Analysis of Tungsten Surfaces - - PowerPoint PPT Presentation

In situ Elastic Recoil Detection Analysis of Tungsten Surfaces during ITER-like Helium Irradiation Kevin Woller , D. Whyte, G. Wright Center for Science and Technology with Accelerators and Radiation Plasma Science and Fusion Center


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SLIDE 1

Background - “Tungsten Fuzz”

In situ Elastic Recoil Detection Analysis of Tungsten Surfaces during ITER-like Helium Irradiation

Kevin Woller, D. Whyte, G. Wright

Center for Science and Technology with Accelerators and Radiation

Plasma Science and Fusion Center

Massachusetts Institute of Technology

Cambridge, Massachusetts, USA

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SLIDE 2

Why and How

i. Motivation for the development of in situ Elastic Recoil Detection Analysis (isERDA)

  • ii. Implementation of isERDA in the Dynamics
  • f ION Implantation and Sputtering Of

Surfaces (DIONISOS) experiment

  • iii. Evolution of the Helium concentration depth

profile in Tungsten under ITER-like conditions

June 2, 2015

  • K. Woller, 26th SOFE, Austin, TX

2

slide-3
SLIDE 3

Why and How

i. Motivation for the development of in situ Elastic Recoil Detection Analysis (isERDA)

  • ii. Implementation of isERDA in the Dynamics
  • f ION Implantation and Sputtering Of

Surfaces (DIONISOS) experiment

  • iii. Evolution of the Helium concentration depth

profile in Tungsten under ITER-like conditions

June 2, 2015

  • K. Woller, 26th SOFE, Austin, TX

3

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SLIDE 4

Helium bubbles modify materials in intriguing ways

June 2, 2015

  • K. Woller, 26th SOFE, Austin, TX

4

  • 1. Tungsten is desirable as a plasma-facing material
  • 2. Tungsten surface morphology becomes nanometer-sized

filiform structure under ITER-like Helium irradiation (900- 1500K, 1022 He m-2 s-1, 30-90 eV) commonly referred to as W fuzz Start Helium irradiation Increasing Helium Fluence 1024 He ions/m2

*transition from shadowed region into fuzzy region on same target *Helium plasma on tungsten target in DIONISOS

Ts = 1100K ΓHe ~ 1022 He m-2 s-1 EHe ~ 60 eV

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SLIDE 5

Tungsten fuzz is both interesting and terrifying

June 2, 2015

  • K. Woller, 26th SOFE, Austin, TX

5

  • 1. Tungsten is desirable as a plasma-facing material
  • 2. Tungsten surface morphology becomes nanometer-sized

filiform structure under ITER-like Helium irradiation (900- 1500K, 1022 He m-2 s-1, 30-90 eV) commonly referred to as W fuzz

  • 3. Modified surface properties (emissivity, sputtering,

conductivity, etc.)

Ts = 1100K ΓHe ~ 1022 He m-2 s-1 EHe ~ 60 eV

inch

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SLIDE 6

Helium Perspective: A view from inside W fuzz

June 2, 2015

  • K. Woller, 26th SOFE, Austin, TX

6

  • 1. Tungsten is desirable as a plasma-facing material
  • 2. Tungsten surface morphology becomes nanometer-sized

filiform structure under ITER-like Helium irradiation (900- 1500K, 1022 He m-2 s-1, 30-90 eV) commonly referred to as W fuzz

  • 3. Modified surface properties (emissivity, sputtering,

conductivity, etc.)

  • 4. He concentration depth profile measured after exposure

shows a uniform distribution of He through the W fuzz layer

  • 5. Concentrations are an order of magnitude lower than

expected for modeling of He bubbles Measured* Expected

*Samples from PILOT-PSI, PISCES-A, Alcator C-MOD

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SLIDE 7

What is the helium doing during the growth process?

June 2, 2015

  • K. Woller, 26th SOFE, Austin, TX

7

  • 1. Tungsten is desirable as a plasma-facing material
  • 2. Tungsten surface morphology becomes nanometer-sized

filiform structure under ITER-like Helium irradiation (900- 1500K, 1022 He m-2 s-1, 30-90 eV) commonly referred to as W fuzz

  • 3. Modified surface properties (emissivity, sputtering,

conductivity, etc.)

  • 4. He concentration depth profile measured after exposure

shows a uniform distribution of He through the W fuzz layer

  • 5. Concentrations an order of magnitude higher were

expected for modeling the He bubbles

  • Measurement during exposure needed to test discrepancy

View of helium irradiation of tungsten from 90° viewport of DIONISOS Charged particle detector Interaction region

slide-8
SLIDE 8

Why and How

i. Motivation for the development of in situ Elastic Recoil Detection Analysis (isERDA)

  • ii. Implementation of isERDA in the Dynamics
  • f ION Implantation and Sputtering Of

Surfaces (DIONISOS) experiment

  • iii. Evolution of the Helium concentration depth

profile in Tungsten under ITER-like conditions

June 2, 2015

  • K. Woller, 26th SOFE, Austin, TX

8

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SLIDE 9

Use high energy ion beams to interrogate a material surface

June 2, 2015

  • K. Woller, 26th SOFE, Austin, TX

9 Low energy injection

1.7 MV Solid state Power Supply

General IONex tandem ion accelerator Modus operandi:

  • High vacuum < 10-4 Pa (10-6 torr)
  • Minimize electromagnetic and thermal noise
  • Flexibility in geometry

Target Detector  Continuous operation  Energy up to 10.5 MeV  Current up to 3 μA on target

High energy Output

Elastic Recoil Detection (ERD) Analysis

Grazing incidence high-Z ion forward scatters low-Z atoms (e.g. H, He) in substrate.

N2 Gas Stripper Positive Terminal Potential

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SLIDE 10

Side note: Fix high energy ion beam machine

June 2, 2015

  • K. Woller, 26th SOFE, Austin, TX

10 Low energy injection

1.7 MV Solid state Power Supply

General IONex tandem ion accelerator Continuous operation Energy up to 10.5 MeV Current up to 3 μA on target The terminal power supply was limited to half its full potential

  • We desired full operational

capabilities for improved measurement

High energy Output

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SLIDE 11

Many areas to check…

June 2, 2015

  • K. Woller, 26th SOFE, Austin, TX

11

25 year old components, Limited documentation, «Proceed with caution» SF6 gas insulation Capacitor-diode voltage multiplier network Bleed resistor chains Control Circuit 6 kV plate power supply 40 kHz Electron tube oscillator 40 kV step up transformer

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SLIDE 12

June 2, 2015

  • K. Woller, 26th SOFE, Austin, TX

12

Start

Start at ground and meet in the middle

Checked and replaced many components along the way, but still could not reach full potential, until…

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SLIDE 13

June 2, 2015

  • K. Woller, 26th SOFE, Austin, TX

13

Final Diagnosis: Push-Pull oscillator feedback capacitor made of 2.5” diameter copper cylinder and 3/8” copper tubing was arcing across a 1/16” gap that should have been 1”

Insulator rings allowed outer conductor to slip vertically

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SLIDE 14

June 2, 2015

  • K. Woller, 26th SOFE, Austin, TX

14

Final Diagnosis: Push-Pull oscillator feedback capacitor made of 2.5” diameter copper cylinder and 3/8” copper tubing was arcing across a 1/16” gap that should have been 1”

Share in our tiny triumph

Thank you to: Dave Terry, Pete Stahle, Dennis Whyte, Regina Sullivan, Graham Wright, Harold Barnard, and Alcator C-MOD electrical and RF engineering team Machine nominal terminal potential = 1.7 MV

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SLIDE 15

DIONISOS - Dynamics of ION Implantation and Sputtering Of Surfaces

June 2, 2015

  • K. Woller, 26th SOFE, Austin, TX

15

Helicon linear plasma device

 Continuous operation  Differential pumping allows up to 5 Pa with accelerator at 10-4 Pa  Up to 0.1 T  Flux densities 1020 - 1023 He m-2 s-1  He Ion Energies up to 300 eV by target biasing  Target temperature controlled from RT to 1400K by ceramic heater

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SLIDE 16

Plasma exposure chamber is non- ideal for Elastic Recoil Detection

June 2, 2015

  • K. Woller, 26th SOFE, Austin, TX

16

Challenges: 1. RF plasma generates electromagnetic noise in exposure chamber (unstable grounding introduces noise into detection circuit) 2. Heat from target and plasma get to detector, which loses stability at elevated temperatures (leakage current through detector is bad for detector resolution) 3. Lorentz force bends ion trajectories (.5-1.5 degree change) plus magnetic field limits material choices for fabrication 4. Background neutral gas pressure introduces additional component to ERD Spectra (2-5 Pa)

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SLIDE 17

Challenges: 1. RF plasma generates electromagnetic noise in exposure chamber (unstable grounding introduces noise into detection circuit) 2. Heat from target and plasma get to detector, which loses stability at elevated temperatures (leakage current through detector is bad for detector resolution) 3. Lorentz force bends ion trajectories (.5-1.5 degree change) plus magnetic field limits material choices for fabrication 4. Background neutral gas pressure introduces additional component to ERD Spectra (2-5 Pa)

Plasma exposure chamber is non- ideal for Elastic Recoil Detection

June 2, 2015

  • K. Woller, 26th SOFE, Austin, TX

17

Solution: Add shielding to protect detector

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SLIDE 18

Challenges: 1. RF plasma generates electromagnetic noise in exposure chamber (unstable grounding introduces noise into detection circuit) 2. Heat from target and plasma get to detector, which loses stability at elevated temperatures (leakage current through detector is bad for detector resolution) 3. Lorentz force bends ion trajectories (.5-1.5 degree change) plus magnetic field limits material choices for fabrication 4. Background neutral gas pressure introduces additional component to ERD Spectra (2-5 Pa)

Plasma exposure chamber is non- ideal for Elastic Recoil Detection

June 2, 2015

  • K. Woller, 26th SOFE, Austin, TX

18

Solution: Add shielding to protect detector

slide-19
SLIDE 19

Challenges: 1. RF plasma generates electromagnetic noise in exposure chamber (unstable grounding introduces noise into detection circuit) 2. Heat from target and plasma get to detector, which loses stability at elevated temperatures (leakage current through detector is bad for detector resolution) 3. Lorentz force bends ion trajectories (.5-1.5 degree change) plus magnetic field limits material choices for fabrication 4. Background neutral gas pressure introduces additional component to ERD Spectra (2-5 Pa)

Plasma exposure chamber is non- ideal for Elastic Recoil Detection

June 2, 2015

  • K. Woller, 26th SOFE, Austin, TX

19

Solution: Add shielding to protect detector

  • Actively cooled detector holder minimizes thermal

leakage current

  • EMI mitigated by triple conductor system for detector

hardware inside the exposure chamber.

  • EMI effectively shorted to ground before infiltrating

the detection circuit.

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SLIDE 20

Challenges: 1. RF plasma generates electromagnetic noise in exposure chamber (unstable grounding introduces noise into detection circuit) 2. Heat from target and plasma get to detector, which loses stability at elevated temperatures (leakage current through detector is bad for detector resolution) 3. Lorentz force bends ion trajectories (.5-1.5 degree change) 4. Background neutral gas pressure introduces additional component to ERD Spectra (2-5 Pa)

Plasma exposure chamber is non- ideal for Elastic Recoil Detection

June 2, 2015

  • K. Woller, 26th SOFE, Austin, TX

20

Solution: Add shielding to protect detector

slide-21
SLIDE 21

Challenges: 1. RF plasma generates electromagnetic noise in exposure chamber (unstable grounding introduces noise into detection circuit) 2. Heat from target and plasma get to detector, which loses stability at elevated temperatures (leakage current through detector is bad for detector resolution) 3. Lorentz force bends ion trajectories (.5-1.5 degree change) 4. Background neutral gas pressure introduces additional component to ERD Spectra (2-5 Pa)

Plasma exposure chamber is non- ideal for Elastic Recoil Detection

June 2, 2015

  • K. Woller, 26th SOFE, Austin, TX

21

Solution: Add shielding to protect detector Solution: Account for changes during data analysis

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SLIDE 22

ERD Analysis with magnetic field calibration and background subtraction

June 2, 2015

  • K. Woller, 26th SOFE, Austin, TX

22

  • 1. Channel axis calibrated to energy scale with magnetic field on
  • 2. Data taken before plasma generated but with magnetic field and

gas feed on for background subtraction Experiment Simulation

  • ERD Raw spectrum

x Background

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SLIDE 23

Interpreting Spectrum as Concentration Depth Profile

June 2, 2015

  • K. Woller, 26th SOFE, Austin, TX

23

Uniform layer concentration One He/W layer in simulation gives absolute values for composition of that layer Take data on 30 second time resolution Result:

  • Time resolved He

measurements during plasma exposure Simulated ERD profile Plasma- Surface Interface He and W layer Bulk W

slide-24
SLIDE 24

Why and How

i. Motivation for the development of in situ Elastic Recoil Detection Analysis (isERDA)

  • ii. Implementation of isERDA in the Dynamics
  • f ION Implantation and Sputtering Of

Surfaces (DIONISOS) experiment

  • iii. Evolution of the Helium concentration depth

profile in Tungsten under ITER-like conditions

June 2, 2015

  • K. Woller, 26th SOFE, Austin, TX

24

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SLIDE 25

Dynamic He concentration is similar to frozen-in values seen before

  • K. Woller, 26th SOFE, Austin, TX

25 June 2, 2015

Sharp rise in He concentration right at start of exposure He concentration reaches some saturation level dependent on exposure conditions (material temperature, flux density, etc.)

  • Absolute measurement of average He

concentration measured dynamically

  • Fundamentally limits how models

incorporate He influence

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SLIDE 26

Dynamic W Fuzz layer thickness follows diffusion-like time dependence

  • K. Woller, 26th SOFE, Austin, TX

26 June 2, 2015

Post Exposure Focused Ion Beam Milling allows us to interpolate the fuzz layer thickness dynamically

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SLIDE 27

Summary

isERDA was developed to study the He concentration depth profile in Tungsten under ITER-like conditions i. Detection system can withstand extreme DIONISOS environment with active cooling and insulation from EMI ii. Magnetic field and background neutral gas modify ERDA in a predictable way and are thus be accounted iii. Dynamic He concentrations rise sharply at the beginning of exposure, then level off at a certain saturation value iv. Dynamic W fuzz layer thickness can be inferred and shows similar diffusion-like time dependence as previous static measurements

June 2, 2015

  • K. Woller, 26th SOFE, Austin, TX

27

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SLIDE 28

Future work

June 2, 2015

  • K. Woller, 26th SOFE, Austin, TX

28

Single Tendrils and tendril bundles grown in DIONISOS suggest nanostructure is supplied by surface diffusion

52 degree tilt

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SLIDE 29

Future work

June 2, 2015

  • K. Woller, 26th SOFE, Austin, TX

29

New W fuzz variant is under active investigation, with current measurements indicating growth is sensitive to ion energy and ion energy distribution

52 degree tilt

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SLIDE 30

Future work

June 2, 2015

  • K. Woller, 26th SOFE, Austin, TX

30

New W fuzz variant is under active investigation, with current measurements indicating growth is sensitive to ion energy and ion energy distribution

52 degree tilt

slide-31
SLIDE 31

Future work

June 2, 2015

  • K. Woller, 26th SOFE, Austin, TX

31

New W fuzz variant is under active investigation, with current measurements indicating growth is sensitive to ion energy and ion energy distribution

52 degree tilt