Kinetics of Neutral Beams in Fusion Plasmas: Charge …science-visits.mccme.ru/doc/ISAN_2011.pdf ·...
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Kinetics of Neutral Beams in
Fusion Plasmas:
Charge-Exchange Recombination
and Motional Stark Effect
Yuri Ralchenko National Institute of Standards and Technology
Gaithersburg, USA
ISAN, May 30 2011
Supported in part by the Office of Fusion Energy Sciences,
U.S. Department of Energy
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Collaborators
• O. Marchuk (Juelich, Germany)
• R.K. Janev (Juelich, Germany)
• A.M.Urnov (Moscow, Russia)
• W.Biel (Juelich, Germany)
• E. Delabie (FOM, The Netherlands)
• D.R.Schultz (ORNL)
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Fusion
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Nuclear Fusion
www.iter.org
ITER: 50 MW input, 500 MW output
First plasma: 2019 (?)
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Plasma Heating for Fusion Devices
Heating beams
ITER: 500 keV/amu
JET: ~140 keV/amu
Diagnostic beams
ITER: 100 keV/amu
TEXTOR: 50-100 keV/amu
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Neutral Beam Spectroscopy in Fusion Devices
Major reaction channels:
H0 + {e,H+,Xz} → H∗ + {e,H+,Xz} → ћω (1)
H0 + Xz → H+ + X*z-1 → ћω (2)
H+ + H0 → H∗ + H+ → ћω (3)
(1) beam-emission spectroscopy (BES) and
motional Stark effect (MSE)
(2) Charge exchange on impurities (CXRS)
(3) CXRS of fast ion diagnostics and fuel ion
ratio measurements (ACX: active charge
exchange)
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Hα(n=3 → n=2) spectrum from the JET tokamak
• Passive light from the
edge
• Emission of thermal
H+ and D+
• Cold components of
CII Zeeman multiplet
• Overlapping
components of MSE
spectra (E, E/2, E/3)
• Ratios among π- and σ- lines within the multiplet are well defined
and should be constant.
Delabie E. et al. PPCF 52 125008 (2010)
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Charge eXchange Recombination
Spectroscopy (CXRS) Ar18+ + H Ar17+ + p
Hung, Krstic and Schultz, CFADC-ORNL database
CX goes into high n’s:
n ~ Z3/4
H-like Ar:
n=14-15 at 428 nm
n=15-16 at 523 nm
Eb = 100 keV/u
Ti = 20 keV
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A
BBeam
Beam-free zone
Beam zone (ACX)
w
vp
tA B
p
ABV
w
Zone 1 Zone 2 Zone 1
Two-zone model
Vp ~ 200 km/s
tAB 4 s
tBA 40 s
nb/n; Eb
Goal: analyze time-dependent kinetics
of Ar impurities under CXRS conditions
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Collisional-radiative model
• Atomic states
▫ [Li] 14 terms 1s2nl 2L, n 5
▫ [He] 19 terms 1snl 1,3L, n 4
▫ [H] 210 nl terms, n 20 and
30 n-bundled Rydberg states,
21 n 50
• Radiative transitions
▫ Cowan + FAC
• Radiative recombination
▫ Rozsnyai & Jacobs (1988)
• Electron collisions
▫ Flexible Atomic Code (FAC)
for excitations from 1s
▫ Van Regemorter
▫ ATOM for [Li] and [He]
• Proton collisions
▫ Impact-parameter method
agrees well with the available close-coupling results
• Charge exchange
▫ Classical Trajectory Monte
Carlo (Hung, Krstic &
Schultz)
Time-dependent code NOMAD
Yu.Ralchenko and Y.Maron, JQSRT 71,
609 (2001)
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Strategy
• Steady-state condition w/ and w/o beam
• Time-dependent relaxation in a beam zone
• Complete time-dependent evolution
• TEXTOR
▫ ne = 5 1013 cm-3, Te = 2 keV
• ITER
▫ ne = 1014 cm-3, Te = 20 keV
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No beam: populations of high-n states
A. Only electrons
B. A + protons
C. B - excitations
from other n’s
5x1013 cm-3/2 keV
proton collisions
are responsible for
redistribution among
the nl excited states
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T=2 keV, Ne=5·1013 cm-3
n=16
w/o protons GS eXcitation
EXCitation
Radiative Decay
DeeXCitation
Radiative Recombination
nl
influx
outflux
with protons
Population flux analysis
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Steady state for the beam zone
w/o: T=2 keV, Ne =5·1013cm-3
w/ CX: ε =2·10-5, Eb= 100 keV
• Substantial change in nl distribution in the beam zone.
• Proton collisions can not „wake up“ the high l sublevels
• Statistical equilibrium is not achieved
•Charge exchange in the whole plasma
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Time-dependent relaxation
•Very long relaxation time
•High-l equilibrate by collisions (16u)
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Impurity entering and leaving the beam zone
A
BBeam
Beam-free zone
Beam zone (ACX)
w
vp
tA B
p
ABV
w
Zone 1 Zone 2 Zone 1
Populations are NOT the same
bfzIRRbzCX
n
n tRRtRN
N1
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Full non-stationary model
1000 cycles of 4e-5 s
Equilibration time:
Ground states
are slow
Excited states
are very fast
Effective CX rescaled by:
bfzbz
bz
tt
t
20 steps of 0.002 s give
the same ion populations
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Motional Stark effect for H beam • Hydrogen beam penetrates the plasma volume • The induced electric field E=v B mixes the spherical states and splits line
multiplets
[n, k, m]
E
z
„Good“ quantum numbers
n – principal quantum number
k=n1-n2 – electric quantum number
m – z-projection of orbital momentum
n=n1+n2+|m|+1, n1, n2>0 (parabolic states)
ΔE Δn=0,E=0 << ΔE Δn=0,E≠0 << ΔE Δn>0 (*)
n1l
ΔEΔn=0
E=0 E≠0
ΔEΔn=0
n1km
n2l n2km
ΔE Δn>0 ΔE Δn>0
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Beam emission
Delabie E. et al. PPCF 52 125008 (2010)
CR model for the H beam:
Major processes affecting level populations:
•Interaction with plasma electrons
•Interaction with plasma protons
•Can we do it for parabolic states?
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Cross sections for parabolic states,
part I
parabolic states
nikimi
nilimi – spherical states
Radiative channel
nikimi→ njkjmj
π – components with Δm=0
σ – components with Δm=
1
Classical excitation: nilimi→ njljmj
Only one axis: along projectile velocity
There is another axis: along the induced electric field E
E
v
= /2 for MSE
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Cross sections for parabolic states, part II
abbaF ˆ
Scattering amplitude between
parabolic states a (nkm)
Transformation 1:
parabolic along z into
spherical along z
1
2211
n
ml
nlm
lm
jjnkm CTransformation 2:
spherical along z into
spherical along z’ l
lm
nlm
l
mmnlm D'
'
)(
'
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m´
'l
m 1n
nkm 540
2
2'
2
3'
2
3'
2
2'
2
)()(
...)()(|ˆ|
ba
j
i
ba
j
i
ba
j
i
ba
j
i
nnm
b
aji
nnm
b
aji
nnm
b
aji
nnm
b
ajijjjiii
qFccqFcc
qFccqFccmknmkn
Final cross section:
Transformation between the spherical and parabolic states
For excitation from the ground state the expressions are still simple:
Density matrix elements
'nlm
i
inkm c
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Calculation of the cross sections in parabolic
states (4)
black - AOCC (present results)
green - GA(present results)
dashed - Born approximation
blue - SAOCC Winter TG, Phys. Rev. A 2009 80 032701
orange - SAOCC Shakeshaft R Phys. Rev. A 1976 18 1930
red - EA Rodriguez VD and Miraglia JE J. Phys. B: At. Mol. Opt.
Phys. 1992 25 2037
blue - AOCC (present results)
green - GA (present results)
dashed - Born approximation
orange - CCC Schöller O et al. J. Phys B.: At. Mol. Opt. Phys.
19 2505 (1986)
red - EA Rodriguez VD and Miraglia JE J. Phys. B: At. Mol. Opt.
Phys. 1992 25 2037
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Collisional-Radiative Code NOMAD in parabolic states
• Time dependent collisional radiative model for non-Maxwellian
plasma applied for studies at EBIT and spectroscopy of fusion
plasmas
Ralchenko Yu V and Maron Y 2001 J. Quant. Spectr. Rad. Transf. 71 609
• Full non-statistical simulations in parabolic m resolved states
• The model is extended up to n=10 states including 220 magnetic
levels.
• The cross sections are calculated up to Δmmax= 5 for first excited
states with n<6 and Δmmax= 3 for other states. In total ~5·105 cross
sections where AOCC and GA data are used.
• Level-crossing and ionization induced by electric field are included
for different values of electric field.
• Electron collisions are based on the Van-Regermorter formula with
reccomended Gaunt factors (high precision is not required)
• Collisional ionization from m levels of the same principal quantum
number is assumed to be the same
Time dependent
solution
Quasi-steady
state
calculations
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Populations of excited states
statistical
calculations
• Population of first excited states is much
closer to the coronal than to the Boltzmann
limit
• Only for n=6 and n=7 the populations
approach statistical case
• The states with m=0 have the highest
populations. The major channel of the
population remains the excitation from the
ground state and the cross sections with
Δm=0,±1 are the strongest ones:
650
540
320
760
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Theory vs Experiment
(1993)
(2010)
• Experiment 1993
• W. Mandl et al. PPCF 35,1373 (1993)
• Solid: Zeff = 1
• Horizontal dashed: statistical limit
• Dashed w/ symbols: Zeff = 2 (C6+)
• Experiment 2010
• E. Delabie et al. PPCF 53, 125008 (2010)
• Solid: Zeff = 1
• Horizontal dashed: statistical limit
• Dashed w/ symbols: Zeff = 2 (C6+)
Coun
ting
Phot
ons
28