F usion Reactor Technology I
(459.760, 3 Credits)
Prof. Dr. Yong-Su Na
(32-206, Tel. 880-7204)
Week 1. Magnetic Confinement
Week 2. Fusion Reactor Energetics (Harms 2, 7.1-7.5)
Week 3. How to Build a Tokamak (Dendy 17 by T. N. Todd) Week 4. Tokamak Operation (I): Startup
Week 5. Tokamak Operation (II):
Basic Tokamak Plasma Parameters (Wood 1.2, 1.3) Week 7-8. Tokamak Operation (III): Tokamak Operation Mode Week 9-10. Tokamak Operation Limits (I):
Plasma Instabilities (Kadomtsev 6, 7, Wood 6) Week 11-12. Tokamak Operation Limits (II):
Plasma Transport (Kadomtsev 8, 9, Wood 3, 4) Week 13. Heating and Current Drive (Kadomtsev 10)
Week 14. Divertor and Plasma-Wall Interaction
Contents
Week 1. Magnetic Confinement
Week 2. Fusion Reactor Energetics (Harms 2, 7.1-7.5)
Week 3. How to Build a Tokamak (Dendy 17 by T. N. Todd) Week 4. Tokamak Operation (I): Startup
Week 5. Tokamak Operation (II):
Basic Tokamak Plasma Parameters (Wood 1.2, 1.3) Week 7-8. Tokamak Operation (III): Tokamak Operation Mode Week 9-10. Tokamak Operation Limits (I):
Plasma Instabilities (Kadomtsev 6, 7, Wood 6) Week 11-12. Tokamak Operation Limits (II):
Plasma Transport (Kadomtsev 8, 9, Wood 3, 4) Week 13. Heating and Current Drive (Kadomtsev 10)
Week 14. Divertor and Plasma-Wall Interaction
Contents
Heating and Current Drive
http://iter.rma.ac.be/en/img/Heating.jpg
Ohmic Heating
Electric blanket
• Intrinsic primary heating in tokamaks due to Joulian dissipation generated by currents through resistive plasma:
thermalisation of kinetic energies of energetic electrons
(accelerated by applied E) via Coulomb collision with plasma ions
• Primary heating due to lower cost than other auxiliary heatings
6
Ip
ICS
Φ
ICS Ip
φ
p+
p p=
p= −
p
I I R V
L
Vp
Ohmic Heating
φ
p+
p p=
p= −
p
I I R V
L
• Total change in magnetic flux needed to induce a final current
f p f i
p p t
ind
l I
k a R R
I L
f
dt
⎥ ⎦
⎢ ⎤
⎣
⎡ ⎟ + −
⎠
⎜ ⎞
⎝
≈ ⎛
=
=
Δ φ ∫
0φ μ
0 0ln 8
02 2
[ 1 . 65 0 . 89 ( 1 ) ]
ln +
95−
≈ q
l
i4 . 0
0
,
0
≈
=
Δ φ
resC
Eμ R I
pfC
Et d R
t
I
p f p
burn
= ′
Δ φ ∫
0• Additional magnetic flux needed to overcome resistive losses during start up
• Further change in magnetic flux needed to maintain Ip after start up
internal inductance
Ejima coefficient
OH
v
B
r Δ
≈ Δ φ π
2• Technological limit to the maximum value of BOH
Tokamak is inherently a pulsed device.
Ohmic Heating
8
: Neoclassical resistivity
2 2 1
1 ⎟⎟
⎟
⎠
⎞
⎜⎜
⎜
⎝
⎛
⎟ ⎠
⎜ ⎞
⎝
− ⎛
=
R r
s n
η η
] /
[
2
2
W m
j P
Ω= j ⋅ E = η
• Ohmic heating density
ηs: Spitzer resistivity
) 1 2
/(
) ) / ( 1 ( )
(
2 0 2
2 0
+
=
−
=
v j
j
a r j
r
j
v⎥ ⎥
⎦
⎤
⎢ ⎢
⎣
⎡
⎟⎟ ⎠
⎜⎜ ⎞
⎝
⎛ − + −
=
+1 2 2 0
2
0
1 1
) 1 (
) 2 (
v
a r r
v j r a
B μ
θ Ampère’s law
0 0 0
0
1 , 2 /
/ ,
/
θ φμ
φ
RB q q v j B Rq
aB
q
a=
a= + =
⎟ ⎠
⎜ ⎞
⎝ ⎛ −
⎟⎟ ⎠
⎜⎜ ⎞
⎝
= ⎛
0 0
2
0 2
2 1 2 1
q q
R q j B
a
μ
φ
Ohmic Heating
,
2
∑ ∑
=
=
s
s s e
e s
s s
eff n n Z
n Z n Z
Zs: charge number for the s-type ion
) 3 /
, 2 / (
/
10
8
23
8
= =
×
≈
−Z
effT
er a R a
η
Ohmic Heating
Magnetic field limited by engineering
→ compact high-field tokamak
2 2
/ 3 5
2
) 2 / (
10 1 0
.
1 ⎟⎟
⎠
⎜⎜ ⎞
⎝
⎥ ⎛
⎦
⎢ ⎤
⎣
⎡
⎟⎟ −
⎠
⎜⎜ ⎞
⎝
× ⎛
=
Ω
=
R B q
q q T
j Z P
o a
o
eff φ
η
qa limited by instabilities
R j B
R j B a
a R j
aB a
R I aB RB
q aB
p a
0
0 2 0 0
2 2 2 2
μ
μ π
π μ π
μ
φ
φ φ
φ θ
φ
<
>
=
=
=
=
- Zeff limited by radiation losses
- High T required for enough fusion reactions
L
E
P
nT =
= 3 / τ
5 4 5
2
0
10
87 .
2 ⎟⎟
⎠
⎜⎜ ⎞
⎝
⎟⎟ ⎛
⎠
⎜⎜ ⎞
⎝
× ⎛
= R
B q
nq T Z
a E
eff
τ
φ2 / ) 10 /
( n
20a
2E
= τ
5 4
87 .
0 B
φT =
5 .
=1
Zeff qaqo =1.5
Alcator scaling
Average temperatures above ~ 7 keV are necessary before alpha heating is large enough to achieve a significant fusion rate.
Ohmic Heating
2 2
/ 3 5
2
) 2 / (
10 1 0
.
1 ⎟⎟
⎠
⎜⎜ ⎞
⎝
⎥ ⎛
⎦
⎢ ⎤
⎣
⎡
⎟⎟ −
⎠
⎜⎜ ⎞
⎝
× ⎛
=
Ω
=
R B q
q q T
j Z P
o a
o
eff φ
η
It seems unlikely that tokamaks that would lead to practical reactors can be heated to thermonuclear temperatures by Ohmic heating!
259-Car Autobahn pile-up near Braunschweig,
largest in German history:
(20 July 2009)
Neutral Beam Injection
- More than 300 ambulances, fire engines and police cars
rushed to the scene to tend to the 66 people injured in the crash.
- The crash was blamed on cars aquaplaning on puddles and a low sun hindering drivers.
Neutral Beam Injection
259-Car Autobahn pile-up near Braunschweig,
largest in German history:
(20 July 2009)
13 Andy Warhol http://www.nasa.gov/mission_pages/galex/20070815/f.html
Plasma
NBI
Neutral beam
Neutral Beam Injection
• Supplemental heating by energy transfer of neutral beam to the plasma through collisions
• Requirements
- Enough energy for deep penetration - Enough power for desired heating
- Enough repetition rate and pulse length > τE - Allowable impurity contamination
Beam particles confined⇓
Collisional slowing down⇓
Injection of a beam of neutral fuel atoms (H, D, T)
at high energies (Eb > 50 keV)*
Ionisation in the plasma⇓
Neutral Beam Injection
* Eb = 120 keV and 1 MeV for KSTAR and ITER, respectively
B H,D,T
Neutraliser
D
D D2
Low
temperature D plasma,
5 eV
Ion source
D+, e-
100 kV -3 kV 0 kV Extraction acceleration grids
D+ D+ D2+
Beam dump
B
D+
Deflection magnet
Vacuum valve
Beam duct
Ex) W7-AS: V=50 kV, I=25 A, power deposited in plasma: 0.4 MW
•
Generation of a Neutral Fuel Beam
Neutral Beam Injection
•
Ion Source
Neutral Beam Injection
•
Ion Acceleration
Neutral Beam Injection
•
Ion Neutralisation
Neutral Beam Injection
•
Ion Deflection
Neutral Beam Injection
•
Neutral Injection
Neutral Beam Injection
•
JET NBI System
Neutral Beam Injection
•
JET NBI System
Neutral Beam Injection
23
•
JET NBI System
JET with machine and Octant 4 Neutral Injector Box
Neutral Beam Injection
•
JET NBI System
Octant 4 Neutal Injector Box
Neutral Beam Injection
•
Ion source
Neutral Beam Injection
• Requirements
- Large-area uniform quiescent flux of high-current ions
- Large atomic ion fraction (D+, D-) > 75 % → adequate penetration - Low ion temperature ( << 1 eV ) to minimize irreducible divergence
of extracted ion beams due to random thermal motion of ions
•
Ion source
Neutral Beam Injection
• Ion generation
- Positive ion generation by electric discharge
D D
D D
e e D
e D
e e D D
e D
+
→ +
+ +
→ +
+ + +
→ +
+ +
+ +
3 2
2
2 2
2
Electron attachment (Double electron capture)
M: alkali or alkali-earth metal vapor (Cs, Rb, Na, Sr, Mg)
+
−
+ +
−
− +
−
−
+
→ +
+
→ +
→ +
+
→ +
+
+
→ +
+
→ +
M D
M D
M D
M D
D Cs
surface cathode
D
D Cs
surface cathode
D
D D
e D
h D
e D
0 0
0 0
0
* 2
) (
) (
ν
Radiative attachment in high density gas (Ebinding = 0.75 eV) Dissociative electron attachment by electric discharge (~eV)Surface production by electric discharge (~100 eV range)
- Negative ion generation
• 3-lens system
Positive electrode
V1
Negative electrode
V2
Earth electrode
potential lines
Grid system at ASDEX Upgrade
0.5m 0.2m
•
Beam Forming System: Extraction and steering
Neutral Beam Injection
2
1
V
V >>
Source Plasma
- Ion extraction + acceleration + minimum beam divergence (≤ 1°)
Neutral Beam Injection
•
Ion sources
RF Source
0.4 - 0.8 m
Cathodes difficult to replace, finite life time Duopigatron
N N N N
fast slow fast gas
D D
D
D
++
2→ +
2+- Charge exchange:
- Re-ionisation:
N D + N D → N N D
++ D + e
−fast gas fast gas
2 2
- Efficiency: (outgoing NB power)/(entering ion beam power)
•
Neutraliser
Neutral Beam Injection
- Negative ion beam development in JT-60U
Neutral Beam Injection
•
Ion Beam Dump and Vacuum Pumps
Neutral Beam Injection
• Beam dump
- Deflect by analyzing magnet - Minimize reionisation losses
- Prevent local power dump at undesirable place (~kW/m2) - Possible application to direct energy conversion
• Pumping
- Minimise reioninsaton losses
- Prevent cold neutral particles from flowing into reactor plasma - Liquid He cryopumps ( ~106 l/s for ~MW system)
32
•
Energy Deposition in a Plasma
Neutral Beam Injection
Andy Warhol
http://www.nasa.gov/mission_pages/galex/20070815/f.html
n: density
σ: cross section
NBI
beam energy
Attenuation of a beam of neutral particles in a plasma Charge exchange:
D
fast+ D
+→ D
+fast+ D
Ion collision:
D
fast+ D
+→ D
fast++ D
++ e
Electron collision:
D
fast+ e → D
fast++ e + e
33
•
Energy Deposition in a Plasma
Neutral Beam Injection
Ex. beam intensity:
( / λ )
exp
) ( )
(
0
x
I
v x N x
I
b b−
⋅
=
=
2
10
205 m
tot
⋅
−σ =
3
1020
5⋅ −
= m
n
m
n 1
tot0 . 4
≈
= σ λ
In large reactor plasmas, beam cannot reach core!
tot b
b
N x n x
dx x
dN ( ) = − ( ) ( ) σ
Penetration (attenuation) length
keV Eb0 = 70
Charge exchange:
D
fast+ D
+→ D
+fast+ D
Ion collision:
D
fast+ D
+→ D
fast++ D
++ e
Electron collision:
D
fast+ e → D
fast++ e + e
Attenuation of a beam of neutral particles in a plasma
•
Energy Deposition in a Plasma
Neutral Beam Injection
4 ) /
( ) (
) (
10 5
. 5 1
3 17
Z a m
n amu A
keV E
Z
n
effb eff
tot
× ≥
=
≡
γ − γλ σ
General criterion for adequate penetration
γ eff
b
AnaZ
E ≥ 4 . 5 × 10
−19Charge exchange:
D
fast+ D
+→ D
+fast+ D
Ion collision:
D
fast+ D
+→ D
fast++ D
++ e
Electron collision:
D
fast+ e → D
fast++ e + e
Attenuation of a beam of neutral particles in a plasma
•
Energy Deposition in a Plasma
Neutral Beam Injection
Charge exchange:
D
fast+ D
+→ D
+fast+ D
Ion collision:
D
fast+ D
+→ D
fast++ D
++ e
Electron collision:
D
fast+ e → D
fast++ e + e
Attenuation of a beam of neutral particles in a plasma
] [keVs
ˆ 1 10
71 .
1 1
2 / 3
2 / 3
18 −
− ⎟⎟
⎠
⎞
⎜⎜
⎝
⎛
⎟⎟⎠
⎜⎜ ⎞
⎝ +⎛
×
=
b c e
b b e
T A P n
ξ ξ ξ
3 /
)
2( 8 ˆ . 14
i i
e b
c
Z A
T
= A ξ
Neutral Beam Injection
•
Slowing down
- Critical energy: The electron and ion heating rates are equal
81 4
/ 3
, 6
ln
2
21 2
3 2 2
1
2 1 2
3 2
0 2 3
2 1 4 2 2
1
≈
⎟ =
⎟ ⎟
⎠
⎞
⎜ ⎜
⎜
⎝
⎛ Λ +
=
+
=
=
−
i e b
b e
b
b e b
e
i e
b
m m A
Z C C
T A
m e Z n
P P
dt P d
π ξ
ξ ε
π
ξ
22 1
b b
b
= m v
ξ
e b
/ T ˆ ξ
Ion heating fraction
3 /
)
2( 8 ˆ . 14
i i
e b
c
Z A
T
= A ξ
Neutral Beam Injection
•
Slowing down
Critical energy
] [keVs
ˆ 1 10
71 .
1 1
2 / 3
2 / 3
18 −
− ⎟⎟
⎠
⎞
⎜⎜
⎝
⎛
⎟⎟⎠
⎜⎜ ⎞
⎝ +⎛
×
=
b c e
b b e
T A P n
ξ
ξ
ξ
38
1. ξb > ξc: Slowing down on electrons no scatter
v||
v ⊥
vb
v||
v
⊥vb 2. ξb < ξc: Slowing down on ions
scattering of beams
1
0 ξb/ξc 10 Fraction of initial beam energy
going to ions
Neutral Beam Injection
•
Slowing down
after before
B Tangential injection
Radial (perpendicular, normal) injection
• standard ports
• shine-through
• particle loss
B
∇ B
. Radial injection:
•
Injection Angle
Neutral Beam Injection
B Tangential injection
Radial (perpendicular, normal) injection
•
Injection Angle
KSTAR NB shine-through armor
Neutral Beam Injection
41
Better heating efficiency
. B Ip
Worse heating efficiency
Projected
particle drifts
- At low magnetic fields heating efficiency depends on NBI direction.
- Best injection angle for maximum penetration and minimum orbital excursion = 10-20° off perpendicular in co-injection direction
•
Injection Angle
Neutral Beam Injection
r B
v
F = e × θ = −ˆ r
B v
F = e × θ = ˆ
outward shift of orbit center inward shift → bad drift orbits
→ energetic ion loss to wall/limiters
• JET
• ASDEX Upgrade
Neutral Beam Injection