Title: Experiments on electrostatic turbulence in the TCV edge
1Experiments on electrostatic turbulence in the
TCV edge
Jan Horacek with help from R.A. Pitts, J. Graves
- Outline
- Introduction to SOL turbulence
- SRAP the diagnostic
- Statistical analysis of density fluctuations
- Radial particle flux
- Study of ELMs
- Parallel flows
Head of Sonde Langmuir RAPide
B-field
4mm
Grand merci a P.Conti, P.Gorgerat, X. Llobet
2Why ELM and bursty studies on TCV?
- ELMy H-mode is a standard scenario for ITER
- Recent indications that SOL radial power flux is
too large for ITER first wall which is not
designed for such high power flux. - Thats not only during ELMs but also continuously
by radial propagating plasma bursty events. - Why such study on TCV? Excellent edge diagnostic
is available ?
3Edge turbulence diagnostic in TCV
- Reciprocating Langmuir probe SRAP, very fast
6-10MHz sampling - Pins measure
- Te (flt3kHz)
- floating potential Vflf-3Te (plasma potential
f, temperature Te) - ion saturation current IsatneTe1/2 (density ne)
- Since fast Te (ETEF project) is still not
available we must assume dTe/Teltlt 2dne/ne
3dTe/Teltlt df/f to get plasma physics relevant
quantities - Different settings on 5 pins allows also Eq,
vpol, Gr - 90 of presented data are from SRAP. Analysis of
ELMy shot is done in the inter-ELM period only.
Wall shadow
SOL
4Main plasma parameters
- ohmic L/H-mode, ELMs, density limit, change in
Btor direction, Ip260-400kA, density ramp
5DC edge profiles
- Edge Thomson scattering, confirmed SRAP profiles
of Te, ne. - Excellent match of absolute values and space
position - density ramp discharges gt typically 1st/2nd rcp.
at 22 and 45-55 of Greenwald density limit,
respectively
6SOL plasma is bursty
Plasma in wall shadow SOL LCFS Confined
plasma
- Positive density bursts become dominant (larger
and less frequent) far away from LCFS.
7Density fluctuation analysis
- Autocorrelation time ltn(t)n(ttAC)gtt 1/e
characterizes time scale of turbulent structures - inside LCFS the PDF of density is Gaussian,
however, nearby wall not at all.
8Density fluctuations
- tAC constant inside LCFS but strongly increases
(longer memory) towards the wall - High S indication that bursty behavior is more
important approaching wall. Also shows that
bursts are not created in the wall shadow.
9Stochastic modeling of density fluctuations
- In progress with J. Graves gt J.Horacek, PPCF
2004. - Statistical approach based on Gamma process in
analogy with the sandpile model - Time evolution and PDF of skewed
Gamma-distribution PGm,s(ne) of no free parameter
fits well neSOL in any TCV Ohmic discharge
10Model predictions
11Poloidal velocity and turbulence dimension on TCV
- Cross-correlation of Isat and Vfl results in the
same vpol ? - VSL position confirms well the LCFS (Liuque) wrt.
absolute SRAP position ? - Direction change in reversed B-field but not in
the whole SOL! - Turbulent structure size lpol-dpol/log(C) to do!
Vfl1
B-field
Vfl4
12Radial particle flux
- Frequencies fgt300Hz only
- GrvExBn (df1-df4)dne/(Bd14)
- ltGrgt increases with density, not due to different
PDF (S equal), not due to correlation C but due
to SOL s(ne) increase - When structure size is smaller than pin distance
(dmidlt10mm) the Gr has no more meaning - Reversed B-field reverses C(Epol,ne) field gt Gr
stays positive! - VSL moves outwards when ltnegt increases. Has it
ever been published?
13(No Transcript)
14Average ELM temporal behavior
Da peak defines tELM0
- Conditional average (wrt. Da peak) of SRAP
density and potential. Very well reproducible - ne rises quickly and decays slowly its really
IsatneTe1/2 (Te changes during an ELM) - Potential starts to oscillate 1ms before its
time-symmetric
Isat
15ELM details
Da
- Detail time evolution of Isat during an ELM shows
a complex structure, explosive growth
Isat (mA)
dmid
16Post ELM oscillation
600kHz gt -80dB!
- Found post ELM oscillations of 600kHz, visible
regularly on floating potential (Vfl) but never
on particle flux (Isat) - Link to sawtooth ST releases free energy into
the edge which is later triggered by an ELM that
starts electrostatic and MHD fluctuations with
frequencies 14,15,16,x37kHz. - 600kHz is too fast to be visible by MHD probes ?.
They see, however, the fundamental 40kHz,
correlated in time and localized on HFS (in
contrary to ELM being localized on LFS).
17Oscillation appears only if a sawtooth anticipates
sound
SRAP floating potential fluctuations
Frequency (kHz)
Time-correlation with 37kHz oscillation on HFS
MHD probe
Help from A.Scarabosio, D.Raju, F.M.Poli
Time (s) during SRAP reciprocation
18Mach number
- 2003 Mach probe installed on TCV gt
- parallel plasma flow Mach number
Mv/csClog(Isat,5/Isat,2) - Radial density (potential) gradients
(Isat3-Isat5)/dr and velocities
Magnetic field
Isat2
Isat5
Isat3
19Parallel flow
Density increase
- Deuterium profile is much flatter (and values
lower) than the Helium one. As density approaches
density limit, the flow slows down and flattens
up to the wall (in D)! - Confirmed classical drifts prediction that M
decreases with density - Strong outside midplane wall sink action
- Too high for classical flow mechanisms gt
ballooning instability plays role - Prediction of important wall sputtered material
migration for ITER!
ELMy H-mode
Density increase
To present at PSI-16 gt Horacek, JNM 2005
20Parallel flows during ELMs
- ELMs do perturb M in the wall shadow only. Why
not in SOL?
SRAP close to LCFS at wall
at wall shadow
21ELM poloidal radial velocity
- At LCFS the vpol is strongly accelerated upwards
(surprise!), however vpol/cs may not change (Te
fast required) - vrad shows no significant change during an ELM
Velocity (km/s)
poloidal radial, radial
22Probable 2D flow
- In total a 2D flow is present, assuming vpol
corresponds to flow velocity (i.e. turbulence is
frozen in), together with vcsM - Inside VSL vpol Bz/Btor csM gt rather
parallel flow - Outside VSL vpol ? -vpol gt strong flow ? B
B
234-parameter cross-correlation fit
Allows finally structure size l, life time tlife
and velocity v proper calculation
- Assuming correlation in form
- Cezcos(z), where
- z-(t/tlife)2d-vt/l)2H
- tAC-2 tlife-2 (l/v) -2
24Radial velocity results from oblique turbulent
structures
25Impossible to derive radial velocity from
cross-correlation
- Radial velocity shear stretches out turbulent
structures gt oblique gt virtual radial
propagation - vradvpol/(dvpol/drtlife).
- 4 space points allows to reconstruct a blob
described by vpol,vrad, lpol, lrad
26- Summary
- 2003 1st systematic edge turbulence
investigation on TCV - Evaluation of Eq, ne, f, M, vpol, Gr during
L/H-mode, ELMs, density limit, deuterium/helium,
change in Btor direction, very high
time-resolution - Clear evidence of non-diffusive transport
intermittent bursts dominate density far away
from LCFS - SOL profile flattening of ne, M while
approaching density limit as well as strong
increase of radial particle transport - Found post-ELM-oscillations, its link to MHD and
saw tooth - Small effect of ELMs on M and vrad but large on
vpol - Outlook
- Discussion on Post-ELM-oscillation is it Alfven
wave? important? - Compute radial propagation of ELMs, IPOs, link
between M and vrad - Continue Ne and start Gr stochastic modeling with
J. Graves, apply on other tokamaks - Experiments in Btorlt0 and with new probe head at
another poloidal positions - This talk is at http//crppwww.epfl.ch/horacek/pu
blications/ - Thank you for your attention ?
27 28Density fluctuations
29Density profile
- For very different shots the mean mltnegt and std
s2 lt(ne -m)2gt are different, however, the
relative density fluctuation 1/A is a quite
universal quantity - m and s are the only parameters of the ne-PDF
description used by J. Graves
30Edge turbulence description I
- SOL electrostatic (fluctuations in ne, Fpl, Te)
is dominant for turbulent transport (magnetic
turb. plays minor role) - ?rne ?rTe provides the free energy to drive the
turbulence - Transport on microscopic scale is non-diffusive
even though on macroscopic scale it looks like
diffusive GRD?dn/dr gt nn0e-r/l.
31Edge turbulence description II
- Turbulent structures characterized by
- PDF, (autocorrelation) life-time t
- Poloidal lpol and radial lrad scale lengths
toroidally very long - Velocities vpol,vrad,vtor
- Universality SOL turbulence character is rather
independent on device size magnetic
configuration tokamaks, stellarators,
limiter/divertor, e.g. C.Hidalgo, PPCF 2002 1557