aries workshop 20010607 dry wall response to the hib (close-coupled) ife target presented by d. a....

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ARIES Workshop 20010607 Dry Wall Response to the HIB (close- coupled) IFE target Presented by D. A. Haynes, Jr. for the staff of the Fusion Technology Institute HIB (458M J) n fusion products x-rays D T p He C Au Be Fe Br Gd

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Page 1: ARIES Workshop 20010607 Dry Wall Response to the HIB (close-coupled) IFE target Presented by D. A. Haynes, Jr. for the staff of the Fusion Technology Institute

ARIES Workshop20010607

Dry Wall Response to the HIB (close-coupled) IFE target

Presented by

D. A. Haynes, Jr.

for the staff of the

Fusion Technology Institute

University of Wisconsin

HIB (458MJ) n

fusion products

x-rays

D

T

p

He

C

Au

Be

Fe

Br

Gd

Page 2: ARIES Workshop 20010607 Dry Wall Response to the HIB (close-coupled) IFE target Presented by D. A. Haynes, Jr. for the staff of the Fusion Technology Institute

ARIES Workshop20010607

Summary/Outline

The target output from the close-copled HIB target is substantially different from that of the direct-drive laser driven targets, in that its

dominant non-neutronic threat component is from x-rays. Protecting the first wall from these x-rays requires more buffer gas than either

SOMBRERO or the AU-coated NRL targets.

The target output from the close-copled HIB target is substantially different from that of the direct-drive laser driven targets, in that its

dominant non-neutronic threat component is from x-rays. Protecting the first wall from these x-rays requires more buffer gas than either

SOMBRERO or the AU-coated NRL targets.

•Comparison of threat spectra

•First wall survival

•Future work

Page 3: ARIES Workshop 20010607 Dry Wall Response to the HIB (close-coupled) IFE target Presented by D. A. Haynes, Jr. for the staff of the Fusion Technology Institute

ARIES Workshop20010607

Though the total yields of the SOMBRERO and high yield closely-coupled HIB targets are similar, the partitioning and

spectra of the non-neutronic output differ significantly.

SOMBRERO (423MJ)

n

fusion products

x-rays

D (90keV)

T

p

He

C (1.6MeV)

Au (N/A)

•Over 25% of the yield from this target is in x-rays, compared with 5% of SOMBRERO’s, or 1% of the NRL Au-coated targets’.

HIB (458MJ) n

fusion products

x-rays

D

T

p

He

C

Au

Be

Fe

Br

Gd

Page 4: ARIES Workshop 20010607 Dry Wall Response to the HIB (close-coupled) IFE target Presented by D. A. Haynes, Jr. for the staff of the Fusion Technology Institute

ARIES Workshop20010607

X-ray Spectra

•The x-ray spectrum of the HIB target is harder than that of the SOMBRERO, but not so hard as the NRL Au-coated target.

•“Quantity has a certain quality all its own.”

If our goal is to prevent vaporization in a 6.5m chamber, we must include a buffer gas at pressures above those

required for SOMBRERO.

Target output x-ray spectra

0.0

0.2

0.4

0.6

0.8

1.0

0.01 0.1 1 10 100

Energy (keV)

Spe

ctra

(pe

ak n

orm

aliz

ed)NRL165(LASNEX)

SOMBRERO(legislated)

HIB (LASNEX)

22.5MJ

2.14MJ

115MJ

Page 5: ARIES Workshop 20010607 Dry Wall Response to the HIB (close-coupled) IFE target Presented by D. A. Haynes, Jr. for the staff of the Fusion Technology Institute

ARIES Workshop20010607

0

500

1000

1500

2000

2500

3000

3500

0 0.1 0.2 0.3 0.4 0.5 0.6

Xe Density (Torr)

Max

.Equ

ilibr

ium

Wal

l Tem

p. to

Avo

id

Vap

oriz

atio

n (C

)

SOMBRERO Target

NRL160 Target

Graphite Chamber Radius of 6.5m

•The gas density and equilibrium wall temperature have been varied to find the highest wall temperature that avoids vaporization at a given gas density.

•Vaporization is defined as more than one mono-layer of mass loss from the surface per shot.

•The use of Xe gas to absorb and re-emit target energy increases the allowable wall temperature substantially.

6.5m Graphite chamber results:

Chamber survives at 1000C, at 240mTorr, 1450C at 300mTorrChamber survives at 1000C, at 240mTorr, 1450C at 300mTorr

Page 6: ARIES Workshop 20010607 Dry Wall Response to the HIB (close-coupled) IFE target Presented by D. A. Haynes, Jr. for the staff of the Fusion Technology Institute

ARIES Workshop20010607

Surface Temperature and Temperature Profiles for 6.5m Graphite chamber, T_equilibrium=1000C

The first peak in temperature is due to the prompt x-rays. The second is due to the re-radiation of the x-ray and ion energy by the Xe buffer gas.

Wall surface temperature, 6.5m Graphite chamber, CC/HIB target

1000

1500

2000

2500

3000

3500

1.E-08 1.E-07 1.E-06 1.E-05

Time (s)

Tem

pera

ture

(C) 200mTorr Xe

240mTorr Xe

280mTorr Xe

Vaporizes 42g/shot

Wall temperature as a function of depth (CC HIB target, 6.5m C

Chamber)

1000

1500

2000

2500

3000

1.E-05 1.E-04 1.E-03 1.E-02 1.E-01 1.E+00Depth (cm)

Tem

pera

ture

(C)

t=1.83e-7 s

Page 7: ARIES Workshop 20010607 Dry Wall Response to the HIB (close-coupled) IFE target Presented by D. A. Haynes, Jr. for the staff of the Fusion Technology Institute

ARIES Workshop20010607

The amount of Xe necessary to prevent wall vaporization for the 6.5m graphite chamber and the CC HIB target is also

sufficient to stop all the ions except the knock-ons.

Per shot accumulation:

(240mTorr, 1000C T_eq.)

D 6.698E+16

T 7.020E+16

P 5.596E+15

3He 7.592E+11

4He 2.515E+13Does the accumulation of hydrogen and helium isotopes in the 1st mm of the wall at this rate pose a problem?

1.E+09

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-05 1.E-03 1.E-01 1.E+01

Depth

# o

f io

ns

D

T

p

3He

4He

Page 8: ARIES Workshop 20010607 Dry Wall Response to the HIB (close-coupled) IFE target Presented by D. A. Haynes, Jr. for the staff of the Fusion Technology Institute

ARIES Workshop20010607

The x-ray deposition length in W is considerably shorter than that of C. To avoid first wall degradation, between 0.3 and 1 Torr of Xe is

required to protect a W first wall at 6.5m from the CC HIB target, and a T_eq of 1000C.

X-ray Attenuation Lengths (NIST)

1.E-07

1.E-06

1.E-05

1.E-04

1.E-03

1.E-02

1.E-01

1.E+00

1.E+01

0.01 0.1 1 10 100

Energy (keV)

Att

enuatio

n le

ngth

(cm

)

C

W

Surface T as a function of time (CC HIB target, 6.5m W chamber)

1000

1500

2000

2500

1.E-08 1.E-07 1.E-06 1.E-05time (s)

Tem

per

atu

re (

C) 940 mTorr Xe

Page 9: ARIES Workshop 20010607 Dry Wall Response to the HIB (close-coupled) IFE target Presented by D. A. Haynes, Jr. for the staff of the Fusion Technology Institute

ARIES Workshop20010607

Conclusion and future work

•Xe density-T_equilibrium operating windows for the closely coupled HIB indirect drive target have been defined.

•The large fraction of this targets yield in x-rays (115MJ) necessitates some form of first wall protection for a 6.5m C or W wall.

•The amount of Xe required to protect the first wall from vaporization by x-rays is sufficient to stop all but the energetic knock-on ions. Is the accumulation of H and He isotopes in the first mm of the wall a problem?

•Xe density-T_equilibrium operating windows for the closely coupled HIB indirect drive target have been defined.

•The large fraction of this targets yield in x-rays (115MJ) necessitates some form of first wall protection for a 6.5m C or W wall.

•The amount of Xe required to protect the first wall from vaporization by x-rays is sufficient to stop all but the energetic knock-on ions. Is the accumulation of H and He isotopes in the first mm of the wall a problem?

•Future work:•Finish write up of dry wall chamber physics work.