evolution of the pedestal on mast and the implications for elm power loadings
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Evolution of the pedestal on MAST and the implications for ELM power loadings Presented by Andrew Kirk EURATOM / UKAEA Fusion Association. - PowerPoint PPT PresentationTRANSCRIPT
A. Kirk, 21st IAEA Fusion Energy Conference, Chengdu, China, October 2006
Evolution of the pedestal on MAST and the implications for
ELM power loadings
Presented by Andrew KirkEURATOM / UKAEA Fusion Association
UKAEA authors were funded jointly by the United Kingdom Engineering and Physical Sciences Research Council and by the European Communities under the contract of Association between EURATOM and UKAEA. The views and opinions expressed herein do not necessarily reflect those of the European Commission.
A. Kirk, 21st IAEA Fusion Energy Conference, Chengdu, China, October 2006
ITER
Size of type I ELM Energy Loss
Understanding the size of ELM energy loss on future devices such as ITER is essential
Most predictions are based on scaling data from present devices
There is a large uncertainty due to our lack of understanding of the processes involved.
A. Kirk, 21st IAEA Fusion Energy Conference, Chengdu, China, October 2006
• Extension of MAST operational space to lower pedestal collisionality
• The filament structures observed during type I ELMs and their relevance to the ELM energy loss process
• Working towards a model for ELM energy losses
Outline
A. Kirk, 21st IAEA Fusion Energy Conference, Chengdu, China, October 2006
Contribution from MAST
Most MAST discharges have a high pedestal collisionality due to a low temperature pedestal and the energy losses due to ELMs
are up to 5 % of the pedestal energy
MAST data
A. Kirk, 21st IAEA Fusion Energy Conference, Chengdu, China, October 2006
Contribution from MAST
New data
A dedicated campaign using optimised fuelling and vessel conditioning has been used to increase the temperature
pedestal and extend the MAST data set to lower collisionalities
Agrees well with the scaling observed on
other devices
A. Kirk, 21st IAEA Fusion Energy Conference, Chengdu, China, October 2006
Pedestal profiles
The lowest pedestal collisionality shot (*ped ~ 0.08) produced to date has:
31910)05.062.2( mn pede eVT ped
e 20435 kJW ped 3.13
A. Kirk, 21st IAEA Fusion Energy Conference, Chengdu, China, October 2006
Stability analysis
Edge stability calculations, using the 2D ELITE code, have been performed on these profiles, which were obtained just before an ELM
A parameter scan shows that the point lies close to the ballooning boundary- Characteristics associated with type I ELMs
A. Kirk, 21st IAEA Fusion Energy Conference, Chengdu, China, October 2006
Comparison of the pedestal at high and low *
Low * High *
(kPa/N) 29.0 30.3 (N) 0.035 0.017
Nd
dP
Similar pressure gradient but low * case is > 2xbroader
A. Kirk, 21st IAEA Fusion Energy Conference, Chengdu, China, October 2006
Comparison of ELM losses at high and low *
Low * High *
No TeLarge Te
%12
pedW
W%3
pedW
W
But why are ELM losses greater at lower collisionality ?
A. Kirk, 21st IAEA Fusion Energy Conference, Chengdu, China, October 2006
What happens during the ELM energy loss process
A. Kirk, 21st IAEA Fusion Energy Conference, Chengdu, China, October 2006
Spatial structure during type I ELMs
MAST
DIII-DASDEX Upgrade
but what role do they play in the ELM loss mechanism ?
NSTX
At the last IAEA it was known that filament structures exist during ELMs
A. Kirk, 21st IAEA Fusion Energy Conference, Chengdu, China, October 2006
Studies of the evolution of the filaments during type I ELMs on MAST
MAST has installed new imaging systems and a new edge TS system to study the evolution of
the filaments
10 kHz frame rate
A. Kirk, 21st IAEA Fusion Energy Conference, Chengdu, China, October 2006
Analysis of the images
3-D field lines are mapped onto the 2-D
images taking into account the distortion
of the system.
A. Kirk, 21st IAEA Fusion Energy Conference, Chengdu, China, October 2006
Analysis of the images
3-D field lines are mapped onto the 2-D
images taking into account the distortion
of the system.
A. Kirk, 21st IAEA Fusion Energy Conference, Chengdu, China, October 2006
Comparison of type I ELMs at different *
Very little difference in the size, number or the behaviour of the filaments
5 s exposure 10 s exposure
A. Kirk, 21st IAEA Fusion Energy Conference, Chengdu, China, October 2006
Evolution of the filament during an ELM
A. Kirk, 21st IAEA Fusion Energy Conference, Chengdu, China, October 2006
Reduced views allows the evolution of the filaments to be studied
100 kHz frame rate
A. Kirk, 21st IAEA Fusion Energy Conference, Chengdu, China, October 2006
Evolution of the filaments
The filaments are observed to rotate in the co-current
direction, decelerate toroidally and accelerate out
radially The width of the filament is ~
constant in time
The toroidal and radial location of the filaments are tracked in consecutive frames
A. Kirk, 21st IAEA Fusion Energy Conference, Chengdu, China, October 2006
Evolution of the filaments
The filaments exist during the time that particles are lost from the pedestal
A. Kirk, 21st IAEA Fusion Energy Conference, Chengdu, China, October 2006
Summary of the evolution of ELM filaments
• Filaments exist for the entire “ELM loss” time
• Individual filaments detach from the LCFS at different times
• Follow the local field line, decelerate toroidally and accelerate radially.
• The width perpendicular to the field line is ~ constant in time
But what is the energy/particle content of the filaments?
A. Kirk, 21st IAEA Fusion Energy Conference, Chengdu, China, October 2006
The energy/particle content of the filaments
0. Pre-ELM pedestal
A. Kirk, 21st IAEA Fusion Energy Conference, Chengdu, China, October 2006
The energy/particle content of the filaments
0. Pre-ELM pedestal
1. Formation of tail
A. Kirk, 21st IAEA Fusion Energy Conference, Chengdu, China, October 2006
The energy/particle content of the filaments
0. Pre-ELM pedestal
1. Formation of tail
2. Radial expansion - no local
loss in pedestal density
Energy in largest filament < 2.5 % WELM
A. Kirk, 21st IAEA Fusion Energy Conference, Chengdu, China, October 2006
The energy/particle content of the filaments
0. Pre-ELM pedestal
1. Formation of tail
2. Radial expansion - no local
loss in pedestal density
3. Filament appears to detach
at mid-plane (leaving a
depression)
Energy in largest filament < 2.5 % WELM
A. Kirk, 21st IAEA Fusion Energy Conference, Chengdu, China, October 2006
The energy/particle content of the filaments
0. Pre-ELM pedestal
1. Formation of tail
2. Radial expansion - no local
loss in pedestal density
3. Filament appears to detach
at mid-plane (leaving a
depression)
4. Accelerates radially –
particle content decreases
exponentially with distance
A. Kirk, 21st IAEA Fusion Energy Conference, Chengdu, China, October 2006
A possible mechanism for type I ELM energy losses
A. Kirk, 21st IAEA Fusion Energy Conference, Chengdu, China, October 2006
A possible mechanism for type I ELM energy losses
• Filaments remain close to the LCFS for 50 - 200 s - during this time they enhance transport into the SOL.
• Individual filaments detach during this period - slow toroidally and accelerate radially.
• At the time of detachment each filament contains up to 2.5 % WELM
• As the filaments travel out radially this content is reduced by parallel transport to the targets
A. Kirk, 21st IAEA Fusion Energy Conference, Chengdu, China, October 2006
Energy lost through the filaments
ELMfilamentfilfilamentN #
Total particles down the filaments
Assume that during ELM the filament acts as a conduit for
losses from the pedestal region
ELM(MHD) ~(A2E)1/3 ~100 s (MAST)
21
841
41
dm
kTncn
Number of filaments Area of filament
A. Kirk, 21st IAEA Fusion Energy Conference, Chengdu, China, October 2006
Energy lost through the filaments
ELMfilamentfilfilamentN #
Total particles down the filaments
Assume that during ELM the filament acts as a conduit for
losses from the pedestal region
ELM(MHD) ~(A2E)1/3 ~100 s (MAST)
ELM energy loss filped
eped
iconv
ELM NTTkqW )(25
//
filament, #fil and pedestal T and n measured
A. Kirk, 21st IAEA Fusion Energy Conference, Chengdu, China, October 2006
Results from the simple model
MAST
Given the simplifications and approximations used there is
moderate agreement with the data
But what about other devices?
A. Kirk, 21st IAEA Fusion Energy Conference, Chengdu, China, October 2006
Results from the simple model
Assume #fil=10
and filament a
Size ~ 20 cm
The next step should be to use our improved knowledge of the ELM loss process to build a “real” model
Extrapolation of model to JET
A. Kirk, 21st IAEA Fusion Energy Conference, Chengdu, China, October 2006
Summary
• High temperature pedestal plasmas have been achieved on MAST with collisionalities one order of magnitude lower than in previous discharges.
• The structure and evolution of the filaments observed during type I ELMs is similar at both high and low collisionalities
• The evolution of the filaments have been tracked through individual ELMs showing how they remain attached to the LCFS, decelerate toroidally and accelerate radially and at the time of detachment each filament carries up to 2.5 % of WELM
• Based on this evolution a mechanism for ELM energy loss has been proposed and a simple ELM energy loss model derived – the next step is to build a “real” predictive model.