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(1)

T opics in Fusion and Plasma Studies 2

(459.667, 3 Credits)

Prof. Dr. Yong-Su Na

(32-206, Tel. 880-7204)

(2)

Week 1-2. The MHD Model, General Properties of Ideal MHD Week 3. Equilibrium: General Considerations

Week 4. Equilibrium: One-, Two-Dimensional Configurations Week 5. Equilibrium: Two-Dimensional Configurations

Week 6-7. Numerical Solution of the GS Equation Week 9. Stability: General Considerations

Week 10-11. Stability: One-Dimensional Configurations Week 12. Stability: Multidimensional Configurations

Week 14-15. Project Presentation

Contents

(3)

Week 1-2. The MHD Model, General Properties of Ideal MHD Week 3. Equilibrium: General Considerations

Week 4. Equilibrium: One-, Two-Dimensional Configurations Week 5. Equilibrium: Two-Dimensional Configurations

Week 6-7. Numerical Solution of the GS Equation Week 9-10. Stability: General Considerations

Week 11-12. Stability: One-Dimensional Configurations Week 13-14. Stability: Multidimensional Configurations Week 15. Project Presentation

3

Contents

(4)

Stability: One-Dimensional Configurations

- Results can be unreliable because the geometric effects associated with toroidicity are of the same order as the field ratio: contribution of

toroidicity in δW are of the same order as those of the straight tokamak.

- Providing very useful frame of reference for the understanding of tokamak stability.

- Most dangerous instabilities: internal and external current-driven modes (pressure-driven modes do not play a major role due to the combination

of finite shear and low β)

- Good MHD stability if the total toroidal current is limited and the current profile is peaked: valid for the fully toroidal case

- No important restrictions on β or the pressure profile: not valid for

• Introduction

1

~ ,

~ /

, 1

/ R

0

B B q

a

z

  

~

~ /

2

0

p B

z2 2: Ohmically heated tokamak : high-β tokamak

(5)

5

Stability: One-Dimensional Configurations

• The “Straight” Tokamak

0 2 4

4 /

0 8

8

2

0 2

2

0 2 2 2

0 2

 

 

 

  

 

 

 

 

 

 

 

  

 

 

 

 

 

q r q r B

r p q

q r

r p B q

q p r

q q rB

z

z z

or

2

~

1

~ / 1

~ ,

~

q q r q

r

q   

• Internal Pressure-Driven Modes: localised interchange instabilities Substituting the tokamak expansion into Suydam’s criterion

2 2

0 2

2 0

2 2 2

or

~ ) ~

/ ( 8

~ ,

~

 

z z

z z

B p q

q rB

p

a p p

a B q

rB q

 

 

 

Over most of the plasma the destabilising term << the stabilising term Suydam’s criterion satisfies over most of the plasma.

(6)

Stability: One-Dimensional Configurations

• The “Straight” Tokamak

0 2 4

4 /

0 8

8

0 2

0 0 0

2 2

0 0

0 0

2 2

0 0 0

2

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

q q r B

p q

q r

r rB p

q q p r

q q rB

z

z z

r q

r q

q r

q q

r q

r p

r p

) 0 ( )

(

) 0 ( 2

/ ) 0 ( )

0 ( )

(

) 0 ( )

(

2

 

 

 

• Internal Pressure-Driven Modes: localised interchange instabilities Exception: near the axis

r q/ q ~ 0

1

~ )

2 ( 1/2 1/2

0

0  



 

q a

q a

r

- If the pressure profile is flattened over a distance Δr, then the modes are stabilised.

(7)

7

Stability: One-Dimensional Configurations

• The “Straight” Tokamak

- In toroidal case there are important modifications to Suydam’s criterion: Mercier criterion. These corrections can eliminate the need for flattening the pressure profile for stability.

0 ) 1

(

4

2

2

 

 

 

  r q

q q

r

simple, low β circular limit of Mercier criterion

toroidal correction

- Localised interchange modes are not very important in a straight tokamak because β is very small.

- Near the axis, we need either flattening or q(0) > 1 (toroidal).

For q(0)>1, pressure term is stabilising: average curvature is formable.

(8)

Stability: One-Dimensional Configurations

• The “Straight” Tokamak

z z

B B

R a

R L

/ /

2

0

0

• Internal Current-Driven Modes

0

0

/ /

2 /

2 kR nk   n R

  

 

 

 

 

 

 

 

 

  

m n q R

mB m

n q R

mB

rB R B m

n R

mB R

nB r

kB mB r

F mB

z

z z

z z

1 1

0 0 0

0 0

0

) (

1 ~

1

2

0 2

2 2

2 0 2 3

2 2 0 2 2 3 2

2

m aB n q R

B r m

n q R

B m m

r k

f rF 

 

 

 

 

 

2 2 2

2 2

0 2 2

2 2

2

0

r

m r

m R

n r

k m

k     

Substituting the tokamak expansion into δWF

n F

F

W W W W

W     

 

0

2

4

  , ~

asymptotic expansion

(9)

9

Stability: One-Dimensional Configurations

• The “Straight” Tokamak

• Internal Current-Driven Modes

r F kB mB

rk rF k

r k

r p k

k

g k

z

 

 

 

 

 

 

 

4

0 2 2

2 2 0

2 2 0 2 0

0

2

1 2

) 2 (

a B q

m n m

R r B n B

r B R m

n R

B m m R

r F n

r kB mB

rk g k

a B m

n q R

m rB m

n q R

B r m r r

m r r m r rF

k r g k

a p B

R r m p n

m r R p n

k g k

z

2 0 4 2

2 2 2

4 0

3 2 0 2 2

2 0 2

2 2 0 2

2 2

0 2 0 2 4 2 0

3 2 4

0 2 3

2 0 2 2

2 0

2 2 0

2 2

0 2 0 2

2 2

2 2 2

2 2

2 2 0

2 2 0 2

2 0 2 0

2 2 0

2 2 0

2 2 0

0 2 1

1 ~ 2

2 2

1 ~ )

1 1 (

1 1

~ 2 2

) 2 (

 



 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

< <

(10)

Stability: One-Dimensional Configurations

• The “Straight” Tokamak

• Internal Current-Driven Modes

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

a a a F a

rdr m

q r m

n a

W W

rdr m

q r m

n R

B

m dr n q R

m rB m

n q R

B r

dr g

R f W

0

2 2

2 2 2 2

0 2

0

2 2

2 2 2 2

0 2 0 0

2 2 2

0 2 2 0

2 2 2

0 2 0 3 0

2 2

0 0

) 1 1 (

1

) 1 1 (

) 1 1 1 (

) / (

2

 

 

m ≥ 2: stable, both terms positive

m = 1: nq(r) > 1 (n = 1 worst)

1 0

1 1 0

1

2

2

 

 

 

 

 

q q

0 0 2 0 2 2

0

2 a B / R

W   

(11)

11

Stability: One-Dimensional Configurations

m = 1: q(r) < 1 somewhere

• The “Straight” Tokamak

• Internal Current-Driven Modes

(12)

Stability: One-Dimensional Configurations

• The “Straight” Tokamak

• Internal Current-Driven Modes

) (

0

) (

2 1

1

) 0

( 1

 

 

 

 

s

s s

s

r r

r r x r

r r

) )(

( 1

) (

) )(

( )

( 1 )

( 1

2

s s

s s s

s

r r r q

r q

r r r q r

q r

q

 

 

r

s

r x  

δWF → 0 as δ → 0

 

 

 

 

s s

r r F a

q R r

B

dx x

q R r

B

rdr r

x R q

B

rdr m

q r m

n R

B R

W

2 3 2 2 0

2 2

2 3 2 0 2 0

2 2 2 2

0 2 0

0

2 2

2 2 2 2

0 2 0 0

0

6

2 1

) 1

1 (

) 1 1 (

/ 2

 

 

 

 

 

 

 

 

 

 

- With an m = 1 resonant surface (i.e. if q(0) < 1), marginally stable in leading order

- For this case, stability is determined by the higher-order corrections to δWF .

(13)

13

Stability: One-Dimensional Configurations

• The “Straight” Tokamak

• Internal Current-Driven Modes

 

 

 

m

n q R

F mB 1

0 0 2

2 0 2 2 2

2 0

2 0 2 3 2

0

2

1

) /

( 

 

 

 

n q

R r

n m

R

B m r k

f rF

2 2 2

0 2 2

0

r

m R

kn

Calculate next order δW for m = 1, n = 1 mode

4 2

0 2 0 2 0

0 2 2

2 0

2 0 2 0

0 2 2

4 0

2 2

2 2 0

2 2 0 2 0

0 2

1 ~ 1 3

2

2 2 1

2 1

2 ) 1

2 (

 

 

 

 

 

 

 

 

 

 

 

 

 

   

 

 

 

 

 

 

 

 

 

 

 

n q q n

R p rB R

r n

n q q n

q n R

p rB R

r n

r F kB mB

rk rF k

r k

r p k

k

g k

z

(14)

Stability: One-Dimensional Configurations

• The “Straight” Tokamak

• Internal Current-Driven Modes

 

 

 

 

 

 

 

 

 

 

rs

F a

q rdr q

R r r

a W

W

dr g

R f W

0 2

0 2 2

2 0 0

4

0

2 2

0 0

3 1 1 1

) / (

2

 

 

- Contributions from both the pressure and parallel current are destabilising

→ unstable

- Often referred to as the m = 1 internal kink mode. But the mode can also be driven by the pressure gradient, particularly in the high-β tokamak regime.

- The nonlinear evolution of the m = 1 internal kink mode, including the

effects of dissipation is believed to be an important component in sawtooth oscillations observed in many tokamaks.

- If the energetic particle effect is included, a modified m = 1 mode thought to be responsible for the so-called fishbone oscillations.

Use the same trial function as before

(15)

15

Stability: One-Dimensional Configurations

• Sawtooth

time (s)

0 2 4 6 8

8 6 1 10 1

Ip(MA)

PNBI(MW) PRF(MW)

WMHD(MJ)

Nel x1.1019

Ti(keV) Te(keV)

ASDEX Upgrade pulse 20438

(16)

Stability: One-Dimensional Configurations

• Sawtooth

1. T(0) and j(0) rise 2. q(0) falls below 1

→ kink instability grows 3. Fast reconnection event:

T, n flattened inside q = 1 surface q(0) rises slightly above 1

kink stable

• Sawtooth

(17)

Stability: One-Dimensional Configurations

• Sawtooth

• Stable m/n=0/1 mode in the initial stage

• m/n=1/1 mode develops as the instability grows (kink or tearing instability)

and reconnection occurs - Tearing mode instability

(slow evolution of the island/hot spot)

- Kink mode instability (sudden crash)

• Reconnection time scale is any different in these two types?

17

(18)

Stability: One-Dimensional Configurations

• Sawtooth

• Comparison with the full reconnection model

• Comparison with the quasi-interchange mode model

J. Wesson (1986) B. Kadomtsev (1976)

(19)

Stability: One-Dimensional Configurations

• Sawtooth

19

• Comparison with the ballooning mode model

Low field side

(20)

Stability: One-Dimensional Configurations

• Sawtooth

• 2-D ECE imaging diagnostic

H.K. Park et al, PRL

(21)

21

Stability: One-Dimensional Configurations

• The “Straight” Tokamak

• Summary of internal modes

- m ≥ 2 stable for both the ohmically heated and high-β orderings - m = 1 internal mode exhibiting a weak instability (i.e. δW ~ ε4)

which can be prevented if q(0) > 1

Kink mode

(22)

Stability: One-Dimensional Configurations

• The “Straight” Tokamak

• External Modes

- The most dangerous ideal MHD instability in a straight tokamak - Current-driven modes in which the k∙B = 0 singular surface lies

in the vacuum region.

- More dangerous energetically than internal modes:

stability determined by the 2nd order contribution to δW

- Stability boundaries unaffected by the pressure gradient in the straight model

(23)

23

Stability: One-Dimensional Configurations

• The “Straight” Tokamak

 

 

  

 

 

 

 

 

 

 

 

 

 

 

 

 

a a

a a

q m

n q

m m n q

m n

rdr m

q r m

n a

W W

1 1

1

] ) 1 (

1 [ 1

2 0

0

2 2

2 2 2 2

0 2

 

• External Modes (The m = 1 Kruskal-Shafranov Limit)

- Examining the first nonvanishing contribution to δW of order ε2 - In the limit where the conducting wall moves to infinity

For either ohmically heated or high-β expansion

q

a

m

n 1

0  

necessary condition for instability:

Resonance surface for an external mode q = m/n lies in the vacuum region.

m n

q

a

0 , 0 ,

Examining the boundary term

(24)

Stability: One-Dimensional Configurations

• The “Straight” Tokamak

• External Modes (The m = 1 Kruskal-Shafranov Limit)

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

a a

a

a

n n q

n q n q

n q W

W 1

1 2 1

1

2

0 2

0 0

2

 

Considering the m = 1 mode

- Minimising eigenfunction by ξ(r) = ξa = const (independent of q profile)

→ integral contribution vanished

Kruskal-Shafranov criterion:

stability condition for the m = 1 external kink mode for the worst case, n = 1

 1 q

a

] MA [ / 5

/

2 a

2

B

0 0

R

0

a

2

B

0

R

0

I

KS

    1

2 /

0

R I a

q

a

aB

Imposing an important constraint on tokamak operation:

toroidal current upper limit (I < IKS)

(25)

25

Stability: One-Dimensional Configurations

• The “Straight” Tokamak

• External Modes (The m = 1 Kruskal-Shafranov Limit)

• Effects of addition of a toroidal field:

- Jz current driving the instability largely flowing parallel to the filed:

The mode described as a current-driven, rather than pressure-driven instability.

- Bending the toroidal magnetic lines: strong stabilising effect

(in order for line bending not to dominate, the modes can only become unstable for sufficiently long wavelengths)

- Tension in the poloidal field increases in the tighter portion of the column when the plasma develops an m = 1 kink perturbation.

- The resulting force is in the direction to enhance the perturbation, thus causing an instability.

(26)

Stability: One-Dimensional Configurations

• The “Straight” Tokamak

• External Modes (The m = 1 Kruskal-Shafranov Limit)

- The stability boundary qa = 1 not depending on the existence of

a pressure gradient, the shape of the Jz profile, or the position of the wall - Very dangerous instability but difficult to observe experimentally

because higher m modes, ideal and resistive, posing even stronger requirements on qa (more sensitive to profile and slower growth rates) - Resistive tearing mode being thought to be responsible for the rapid

termination of tokamak discharge by means of a “major disruption”

when qa ~ 2-3, well below the current required to excite the Kruskal-Shafranov mode.

(27)

27

Stability: One-Dimensional Configurations

• The “Straight” Tokamak

) 1 )(

2 (

2

2

  

nq m nq m

q W

W

a a

a

a

• External Modes (m ≥ 2 External Kinks): imposing more stringent conditions on qa and the current profile than m = 1

)

1

/ ( )

( r  

a

r a

m

 

 

  

 

 

 

 

 

 

 

 

 

 

 

 

 

a a

a a

q m

n q

m m n q

m n

rdr m

q r m

n a

W W

1 1

1

] ) 1 (

1 [ 1

2 0

0

2 2

2 2 2 2

0 2

 

n q m

n m

a

1 

regions of stability bounded

For the uniform current density profile, q(r) = qa = const (n = 1)

(28)

Stability: One-Dimensional Configurations

• The “Straight” Tokamak

- Shafranov (1970) pointed out that this pessimistic result is strongly dependent on the shape of the current density profile.

- For more realistic profiles, as m increases, the mode structure for external kinks becomes progressively more localised in the

vicinity of the plasma surface.

- The plasma contribution to W depends sensitively on the local behaviour of the current density near r = a when J(a), J’(a), etc.

are small, the instabilities diminish.

- The m = 1 mode is determined solely by the total current.

• External Modes (m ≥ 2 External Kinks)

(29)

29

Stability: One-Dimensional Configurations

• The “Straight” Tokamak

0 )

( )

( 

2

2

    

dr f g f g

 

 

  

 

 

 

 

 

 

 

 

 

 

 

 

 

a a

a a

q m

n q

m m n q

m n

rdr m

q r m

n a

W W

1 1

1

] ) 1 (

1 [ 1

2 0

0

2 2

2 2 2 2

0 2

 

1 0 )

1

1

2

(

2 2

3

  

 

 

 

 

 

 

   

q m m n

dr r d q

m r n dr

d

The trial function which minimises the plasma term satisfies

 

 

 

 

  

 

 

  

 

 

 

 

 

  

m

nq m

nq m a

m nq q

W

W

a a

a a a

a

a2

1 1 1

2

0

2

• External Modes (m ≥ 2 External Kinks) Asymptotic Analysis

(30)

Stability: One-Dimensional Configurations

• The “Straight” Tokamak

• External Modes (m ≥ 2 External Kinks)

1 0 1

2 2 2

2 2

2

 

 

  

b

dr K d K r

m dr

b d Kr

b ( ) 

Simplifying the analysis by considering the limit of large m

- Instability occurs only when the resonant surface lies just outside the plasma.

- The corresponding plasma displacement is highly localised just inside the plasma, allowing one to perform a high m asymptotic analysis of the Euler-Lagrange equation.

1 0 )

1

1

2

(

2 2

3

  

 

 

 

 

 

 

   

q m m n

dr r d q

m r n dr

d

 

 

 

m q

r n r

K 1

)

(

3/2

(31)

31

Stability: One-Dimensional Configurations

• The “Straight” Tokamak

assuming m >> 1

• External Modes (m ≥ 2 External Kinks)

m z a

r

1  2

 

 

 

 

 

 

 

 

 

 

 

 

  

 

 

  

m z a m

n m z z

m a a

K

m z a m

a n K

a a

a

a a

2 ˆ ˆ

4 3 8

ˆ

2 ˆ ˆ

2 2 2 2

/ 3 2

2 / 3 1

 

  m

m

nq

a

1

~ 1 

 

K

1

K

2

K

0 ≤ z ≤ 1 for localisation of the mode

small if the resonance surface is near the plasma

K1 ~ 1/m, K2 ~ 1/m2 Expand the function K

a a

1 / q ˆ 

(32)

Stability: One-Dimensional Configurations

• The “Straight” Tokamak

can be more conveniently expressed in terms of the

properties of the current profile at the plasma edge.

• External Modes (m ≥ 2 External Kinks)

) 0 (

4 1

0 2

2

 

 

 

b

z z m dr

b

d

 

 

  

 

 

 

 

 

a

a a a a

m n i

a z m

a a

a

  , 2 ˆ ˆ

ˆ 3 ˆ ˆ 2

1

0 2

 

 

 

 

J J

a q

a

a

a

2 1

 ˆ

J q

J a a

a

a a a

a

 

 

 3 ˆ 2 ˆ

2

 

0 0 0

2

0

/ a 2 B ˆ / R

I

J    

a

 ) (

),

( a J J a

J

J

a

a

  

 

 

 

 

  

 

 

 

a a

a a

J J

J m

m nq J z

J J

a , 1 2

1

0

J r

rB rB

B

R

0

/

0

, ( ) /

0

ˆ 

 

 

(33)

33

Stability: One-Dimensional Configurations

• The “Straight” Tokamak

• External Modes (m ≥ 2 External Kinks)

 

 

  

 

  

 

 

  

 

 

  

J

J m

b b m

m nq m

nq q

W

W

a a a

a

a

2 1 2

1 1

1

0 0 2

2

0

2

0 0

0

 / b  [( db / dz ) / b ]

z

b

) 0 (

4 1

0 2

2

 

 

 

b

z z m dr

b

d

Desired form of the high-m external kink stability problem

The case Ja ≠ 0: calculate the leading-order contribution to b

2

)

/

( z e

z

b

4 0

2

2

bdr

b

d

solution corresponding to

a localised eigenfunction

(34)

Stability: One-Dimensional Configurations

• The “Straight” Tokamak

• External Modes (m ≥ 2 External Kinks)

 

 

  

 

 

  

m J

J m

nq m

nq q

m W

W

a a a

a

a

1 1

2

2 2

0

2

instability

n q m

J m J

n

a

a

   

 

  1

- The most unstable case occurs for uniform current, Ja/<J> = 1:

neighbouring bands touch and all qa values are unstable.

- As the current at the boundary decreases, the unstable bands become narrower, forming windows of stability.

(35)

35

Stability: One-Dimensional Configurations

• The “Straight” Tokamak

b → 0 as z → ∞

• External Modes (m ≥ 2 External Kinks)

 

 

  

 

 

  

b m

b m

nq q

m W

W

a

a

a

2 1

1 1

0 0 2

2 2

0

2

U ye

b

y z

z

y 2/ 0

0 1

) 2

2

(

2

 

 

  

U

m dr

y dU dr

U

y d

)

; 2 , / 1

/

(

y m ye

b

y s

  

The case Ja = 0: 1/m corrections to b(r) taken into account

1 )

/ 1

(

0

 1  mnq m 

z

a

) 0 (

4 1

0 2

2

 

 

 

b

z z m dr

b

d

(36)

Stability: One-Dimensional Configurations

• The “Straight” Tokamak

condition for instability

• External Modes (m ≥ 2 External Kinks)

0 ln

1   z

0

n q m

J a

J m m

n

a

a

 

 

 

 

 2  1 exp

The case Ja = 0: 1/m corrections to b(r) taken into account

- Instability can only exist over exponentially narrow bands of qa. - When the current vanishes at r = a the range of unstable qa values

is greatly reduced.

- If Ja’ vanishes, the high-m external kinks can be completely stabilised.

(37)

37

Stability: One-Dimensional Configurations

• The “Straight” Tokamak

• External Modes (m ≥ 2 External Kinks)

1 1 2 2 0

] ) 1 ( 1 [

) / 1

(

v a

v

u u

q q

a r J

J

2 2 0

, / /

1 q q u r a

v  

a

- Unshaded region is stable to both internal and external ideal MHD modes. Most existing tokamaks operate in this regime.

- ν > 2.5 or qa/q0 ≥ 3.5 all m ≥ 2 modes are stable for any qa. - Windows of stability in qa also exist for 1 < ν <2.5.

- Complete external-mode stability is achieved by the additional requirement qa > 1 to stabilise the m =1 mode.

Numerical results by Wesson (1978)

(38)

Stability: One-Dimensional Configurations

• The “Straight” Tokamak

• Summary

- m ≥ 2 external-kink modes are sensitive to the features of the current density profile near the edge of the plasma.

- A combination of rapidly vanishing current gradient and a limit on the total current is sufficient to completely stabilise all high- and low-m number external modes, respectively.

- The dual requirements of q0 > 1 for internal-mode stability and peaked current density profiles for high-m external-kink stability can only be simultaneously satisfied if qa ≥ 3.

- Therefore, m ≥ 2 kinks impose stronger constraints on than the m = 1 Kruskal-Shafranov mode.

(39)

39

Stability: One-Dimensional Configurations

• The “Straight” Tokamak

• The Effect of a Resistive Wall

- We have seen that a perfectly conducting wall, placed in close proximity to the plasma can have a strong stabilizing effect on external kink modes.

- In actual experiments, the metallic vacuum chamber surrounding the plasma is a good approximation to a perfectly conducting wall.

- However, its conductivity is not infinite but is finite.

- In fact we do not want the conductivity too high and/or, too thick because it would take too long externally applied feedback fields to penetrate the shell and interact with the plasma.

- Also, higher resistivity, smaller currents are induced in the chamber during transients, alleviating power supply requirements.

- The question raised here concerns the effect of finite resistivity of the wall on external kink stability.

(40)

Stability: One-Dimensional Configurations

• The “Straight” Tokamak

• The Effect of a Resistive Wall

- There are three possible situations and only one is really interesting.

- In the first case the plasma is stable to external kinks with the wall at ∞.

Here, since the plasma is already stable, a wall, either ideal or resistive does not affect stability. This case is uninteresting.

- In the second case, the plasma is unstable with the wall at ∞ and with the wall at its actual position, assuming the wall is perfectly conducting.

Since the plasma is unstable with a perfectly conducting wall as r = b, making the wall resistive does not help. This case is also uninteresting.

- The interesting case is when the plasma is unstable with the wall at ∞, but stable with a perfectly conducting wall at r = b.

Does the resistivity of the wall destroy wall stabilization?

- To address this issue we investigate the problem in a straight cylindrical geometry. However, the results are valid for a general toroidal geometry as well.

(41)

41

Stability: One-Dimensional Configurations

• The “Straight” Tokamak

• The Effect of a Resistive Wall Plan of attack

- The analysis of the resistive wall mode is carried out in four steps.

1. Reference values of δW are calculated for an ideal wall located as r = ∞ (δW) and at r = b (δWb)

2. The full eigenvalue problem is solved region by region assuming slow growing modes: on the scale of the wall diffusion time.

3. The fields within the resistive wall are calculated using the BCs.

then wall approximation. This gives rise to a set of jump conditions across the wall.

4. The resulting set of coupled equation and boundary conditions are solved yielding the dispersion relation.

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