Gamma-to-Electron Magnetic Spectrometer (GEMS) Update · Gamma-to-Electron Magnetic Spectrometer...

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Gamma-to-Electron Magnetic Spectrometer (GEMS) Update Yongho Kim, Hans Herrmann, Carl Young, Justin Jorgenson, Frank Lopez, David Barlow, Michelle Espy, Mandie Gehring (LANL) Terry Hilsabeck (GA) Wolfgang Stoeffl, Dan Casey, Todd Clancy (LLNL) Ken Moy (NSTec) 2015 National Diagnostic Workshop, Los Alamos, NM October 6 - 8, 2015 LA-UR-15-27669

Transcript of Gamma-to-Electron Magnetic Spectrometer (GEMS) Update · Gamma-to-Electron Magnetic Spectrometer...

Page 1: Gamma-to-Electron Magnetic Spectrometer (GEMS) Update · Gamma-to-Electron Magnetic Spectrometer (GEMS) Update ... Todd Clancy (LLNL) Ken Moy ... Gamma-to-Electron Magnetic Spectrometer

Gamma-to-Electron Magnetic Spectrometer (GEMS) Update

Yongho Kim, Hans Herrmann, Carl Young, Justin Jorgenson, Frank Lopez, David Barlow, Michelle Espy, Mandie Gehring (LANL)

Terry Hilsabeck (GA)Wolfgang Stoeffl, Dan Casey, Todd Clancy (LLNL)

Ken Moy (NSTec)2015 National Diagnostic Workshop, Los Alamos, NM

October 6 - 8, 2015

LA-UR-15-27669

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Motivation for GEMS Review of Conceptual Design of GEMS Detector Simulation Benchmarking (in progress)

Outline

Slide 2

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The ICF -ray Energy Spectrum provides ‘burn-averaged’ observables, providing a global reference for the line-of-sight-specific measurements

Slide 3

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The ICF -ray Energy Spectrum provides ‘burn-averaged’ observables, providing a global reference for the line-of-sight-specific measurements

Slide 4

Burn-averaged observables Total YDT

• YDT = B/n YDT

Total Down Scattering Fraction (TDSF)• TDSF = 1 - (Yn(13-15)/YDT-)

Existing yield measurements compromised by:• Yn: neutron downscattering• GRH: interfered by D(n,)

and 12C(n,)

DT0-rays could provide Total DT yield• Negligible DT- down-

scattering (unlike DT-n)• in-situ calibrations using DT

Expl Pshr (R 0)GEMS total DSF will provide additional R data independent of line of sight

Page 5: Gamma-to-Electron Magnetic Spectrometer (GEMS) Update · Gamma-to-Electron Magnetic Spectrometer (GEMS) Update ... Todd Clancy (LLNL) Ken Moy ... Gamma-to-Electron Magnetic Spectrometer

The ICF -ray Energy Spectrum provides ‘burn-averaged’ observables, providing a global reference for the line-of-sight-specific measurements

Slide 5

Burn-averaged observables Total YDT

• YDT = B/n YDT

Total Down Scattering Fraction (TDSF)• TDSF = 1 - (Yn(13-15)/YDT-)

Cold fuel R• D(n,)

( , )( , )

( , )

6 2

( )

~1.44 10 [ / /( / )]

D n aD n DT

D t n D T

Y NR

Y MW MW

n g cm

Direct measurement of Fuel R

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The ICF -ray Energy Spectrum provides ‘burn-averaged’ observables, providing a global reference for the line-of-sight-specific measurements

Slide 6

Burn-averaged observables Total YDT

• YDT = B/n YDT

Total Down Scattering Fraction (TDSF)• TDSF = 1 - (Yn(13-15)/YDT-)

Cold fuel R• D(n,)

Ablator R• 12C(n,n’)• 12C(n,)

GEMS can improve Ablator R accuracy (GRH ~ 20 %) even at today’s NIF yield

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Slide 7Slide 7

Need measure 4.4 MeV signal while in high energy (10 to 20 MeV) range

4.4 MeVdetector

10 to 20 MeV @ 1200 G(3 to 6 MeV) @ 400 G

coil

detectorplane

-to-e-

Compton converter

Gamma-to-Electron Magnetic Spectrometer (GEMS) concept has been proposed to measure the ICF spectrum

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GEMS Design Challenges at NIF

To minimize NIF background radiation– X-ray filter + Background e-filter– Locating magnet & detector

array outside NIF chamber– Fast electron detector (< 1.5ns)– Quartz Cherenkov radiator (>

175 keV) To improve sensitivity

– Large gap electromagnet– Locating Compton converter

inside NIF chamber

Slide 8

1.E+10

1.E+11

1.E+12

1.E+13

1.E+14

1.E+15

1.E+16

1.E+17

1.E+18

1.E+19

1.E+20

1.E+21

1.E-03 1.E-02 1.E-01 1.E+00 1.E+01 1.E+02

Ph

/M

eV

MeV

LPI X-rays and LPI e-

-ray

~105x more LPI X-ray than the DT fusion gamma-ray (looking at stars on sunny day!)

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GEMS detection efficiency () was also calculated by Monte-Carlo simulations with constant magnet efficiency assumed

Slide 9

e

magnetd dd

Kinematic (converter & magnet aperture size and location)

Compton conversion

Magnet focusing

Constant Resolution E = 0.5 MeV

Sensitivity constrained by E/E and foil distance from TCC

Proposed foil location

Geant4 (GA), CYLTRAN (LANL)

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GEMS Conceptual Design (June 2013)

Slide 10

SweeperMagnet Reentrant Tube Port

Cover

AnalyzingMagnet

SupportStructure

(modified from MRS)

Electron Beam

“Get Lost” Tube

e‐ GraphiteCollimator

DetectorArray

(Cherenkov to PMT)

X-ray Filter & -Collimator(2m from TCC)

-to-e-

Converter(3 foil thicknesses)

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Physics-based Performance Goals (June 2013)

Slide 11

Topic Requirement

Energy Resolution E/E = 3-5% (e.g., 0.5 MeV @ 16.7 MeV, 0.2 MeV @ 4 MeV)

Energy Range Total: 2-25 MeVSingle Shot: E033% (e.g., 10-20, 3-6 MeV)Separate 4.4 MeV channel when operating in 10-20 MeV mode

Binning 20 energy bins (+1 for 4.4 MeV when tuned to 10-20 MeV)

Temporal Response (fwhm)

< 1.5 ns (discriminate against LPI x-rays ~2 ns early and Chamber wall n- 100 ns later)

SNR > 5 for 100

Dynamic range > 100

Accuracy Statistical <11%; Systematic < 10%; Total <15%

Sensitivity CH ablator R Y>5e14 for RCH >200 mg/cm2

Total DT yield Y>2e15 for 0

Fuel R Y>1e16 for Rfuel >1 g/cm2

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Motivation of GEMS Review of Conceptual Design of GEMS Detector Simulation Benchmarking (in progress)

Outline

Slide 12

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Slide 13

Current Layout of GEMS Design Codes

Magnet

TOSCA(EM code)

-to-eConverter

ACCEPT(Monte-Carlo)

ElectronDetector

ACCEPT

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Slide 14

Final Goal of Layout of GEMS Design Codes

Magnet

TOSCA(EM code)

-to-eConverter

ACCEPT(Monte-Carlo)

ElectronDetector

ACCEPT

CAD model

electron

B-field

electron

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Slide 15

Initial Coupling in Progress

Magnet

TOSCA(EM code)

-to-eConverter

ACCEPT(Monte-Carlo)

ElectronDetector

ACCEPT

CAD model

electron

B-field

electron

Initial coupling: converter & magnet only

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LANL’s Pretzel Spectrometer data can be used for benchmarking purpose

Slide 16G. Morgan (LANL, 1991) A. Gehring and M. Espy (LANL, 2015)

TOSCA simulation

showing a set of tacks for a 10 MeV beam of electrons (D.

Barlow)

Magnet (Sm-Co)Focal plane

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Operated by Los Alamos National Security, LLC for the U.S. Department of Energy’s NNSA

U N C L A S S I F I E D LA-UR-14-26491

Storage phosphor images (A. Gehring and M. Espy)

Slide 17

10 MeV e- 15 MeV e- 20 MeV e-

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Operated by Los Alamos National Security, LLC for the U.S. Department of Energy’s NNSA

U N C L A S S I F I E D LA-UR-14-26491

Reconstructed spectra (A. Gehring and M. Espy)

Slide 18

Raw Data Post-processed Data

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ACCEPT simulation incorporating B-field tested with 15 MeV electron energy (C. Young)

Slide 19

W-collimator

Sweeper magnet

Be-converter

Focal plane

Brem. target

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Slide 20

Electron profile at focal plane from 15 MeV endpoint energy x-ray source striking converter (C. Young)

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Summary

Slide 21

• GEMS can support high R implosions by providing unique observables:

- burn-averaged observables, providing a global reference for the line-of-sight-specific measurements

- Individual, direct measurement of Fuel R, Ablator R, and Total R

• GEMS conceptual design was completed (June 2013)

• Monte-Carlo simulation incorporated with B-field is in progress