2267-10 Joint ITER-IAEA-ICTP Advanced Workshop on Fusion and...
Transcript of 2267-10 Joint ITER-IAEA-ICTP Advanced Workshop on Fusion and...
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2267-10
Joint ITER-IAEA-ICTP Advanced Workshop on Fusion and Plasma Physics
JENKO Frank
3 - 14 October 2011
Max Planck Institut fuer Plasmaphysik, Boltzmannstrasse 2 D-85748 Garching bei Muenchen
GERMANY
On the nature of plasma microturbulence
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Frank Jenko
Max-Planck-Institut für Plasmaphysik, GarchingUniversität Ulm
Advanced Workshop on “Fusion and Plasma Physics”October 3 – 14, 2011
Trieste, Italy
On the nature ofplasma microturbulence
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Some introductory remarks
There is a great body of work on fluid turbulence; to whichdegree is plasma microturbulence similar or different?
I will attempt to present the material in an accessible way
Please feel free to interrupt me if you have a question
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Turbulence in fluids and plasmas
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What is turbulence?
Turbulence…
• is a nonlinear phenomenon
• occurs (only) in open systems
• involves many degrees of freedom
• is highly irregular (chaotic) in space and time
• often leads to a (statistically) quasi-stationarystate far from thermodynamic equilibrium
These properties make it a very complicated problem –neither Dynamical Systems Theory nor Statistics applies!
Leonardoda Vinci
(1529)
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According to a famous statement by Richard Feynman…
…and a survey by the British “Instituteof Physics” among many of the leadingphysicists world-wide…
TURBULENCE:A challenging topic for both basic and applied research
Turbulence – one of the most important unsolved problems in physics
“Millennium Issue”(December 1999)
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How to approach turbulence?Many physicists – including Heisenberg, von Weizsäcker,Onsager, Feynman, and many others – have attemptedto tackle turbulence purely analytically but with onlyvery limited success.
Today, supercomputers helpto unravel the “mysteries” ofturbulence in the spirit ofJohn von Neumann:
„There might be some hope to 'break the deadlock' byextensive, but well-planned, computational efforts...“
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The Navier-Stokes equation
The NSE in its ‘classical’ form:
Expressed in terms of vorticity :
Reynolds number as single dimensionless parameter:
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Turbulence as a local cascade in wave number space…
„Big whorls have little whorls, little whorls have smaller whorlsthat feed on their velocity, and so on to viscosity“
Much turbulence research addresses the cascade problem
The Richardson cascade
kE
ηk k
energy flux
fk
driverange
dissipationrangeinertial
rangeComputationaleffort
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E = v2 d3x = E(k) dk⌠⌡
∞12V
⌠⌡0
Kolmogorov’s theory from 1941
K41 is based merely on intuition and dimensional analysis –it is not derived rigorously from the Navier-Stokes equation
Key assumptions:
• Scale invariance – like, e.g., in critical phenomena• Central quantity: energy flux ε
E(k) = C ε2/3 k-5/3
This is the most famous turbulence result: the “-5/3” law.However, K41 is fundamentally wrong: scale invariance is broken!
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Plasma microturbulence:Linear drive
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trapped electron modes
ETG modes
ITG modesNot shown here:- drift waves- ballooning modes
Some important microinstabilities
Wide drive range
Universality?
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Perpendicular dynamics: de-/stabilization in out-/inboard regions
stable
unstable Rayleigh-Taylor instabilityAnalogy in a plasma:
Parallel dynamics: localization in outboard regions
Gradient-driven microinstabilities
G. Hammett
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Basic properties of microturbulence
In the context of fusion energy,gaining a better understandingof plasma turbulence is crucial
Existence of critical temperature gradients
Temperature profiles tend to be ‘stiff’ (cp. solar convection zone).
Typical space scales: several ion gyroradii (not system size)
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ETG / ITG modes: Critical gradients
Linear gyrokinetic simulations:
Linear stability of ETG / ITG modes [Jenko et al. 2001]
Thousands of linear GK simulations condense into one simple formula…
Limiting cases (analytical results):- Hahm & Tang 1989 (for high s/q)- Romanelli 1989 (for low s/q)
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Plasma microturbulence:Nonlinear saturation?
F. Jenko, Physics Letters A 351, 417 (2006)
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2D Hasegawa-Mima equations: ZFs
Standard HME(ETG)
Modified HME(ITG)
Hasegawa & Mima, PRL 1977
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4-mode analysis
ITG-type HME in Fourier space
Reduction to just 4 modes (and their CC’s)
streamer
zonal flowsi
deba
nds
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In the context of fusion energy,gaining a better understandingof plasma turbulence is crucial
Resulting amplitude equations
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In the context of fusion energy,gaining a better understandingof plasma turbulence is crucial
Zonal flow growth rate
If the streamer amplitude exceeds a certain threshold,the zonal flow becomes unstable.
Its growth rate is given by:
ITG case
ETG case
Strintzi & Jenko, PoP 2007
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Secondary instabilities & ZF generation
Strintzi & Jenko, PoP 2007Xanthopoulos et al., PRL 2007
• Large-amplitude streamers are Kelvin-Helmholtz unstable[Cowley at al. 1991; Dorland & Jenko PRL 2000]
• This secondary instability contains a zonal-flow component• Near-equivalence to 4-mode and wave-kinetic approaches
Simpletokamak
W7-Xstellarator
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A different story: TEM turbulence
Saturated phase of TEM turbulence simulations:
- In the drive range, nonlinear and linear frequencies are identical
- In the drive range, there is no significant shift of cross phases w.r.t. linear ones
– No dependence of transport level on zonal flows [Dannert & Jenko 2005]
Zonal flows suppressed
linear
nonlinear
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ZF / Non-ZF regimes
Ernst et al., PoP 2009
ExB shearing rates exceed thegrowth rate only for ηe < 1
For mainly temperature gradientdriven TEM turbulence, ZFs(and GAMs) are “unimportant”
Thus, in a wide region of parameterspace, the standard drift-wave / ZFparadigm does not hold
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Low-ky drive range: large transport contributions, but small random noise; here, one finds:
Saturation of TEMs: “eddy damping”
~ky2
Merz & Jenko, PRL 2008
This is in line with various theories, including Resonance Broadening Theory (Dupree), MSR formalism (Krommes), Dressed Test Mode Approach (Itoh).
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Dissipation & cascadesin plasma microturbulence
Hatch, Terry, Jenko, Merz & Nevins, PRL 2011
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Turbulence in fluids and plasmas –Three basic scenarios
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Saturation via damped eigenmodes
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Excitation of damped eigenmodes
Using GENE as a linear eigenvalue solver to analyzenonlinear ITG runs via projection methods, one finds…
unstableeigenmode
least damped eigenmode
ky=0.3drive range
strongly dampedeigenmodes
(fine-scale structurein v║ and z)
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Energetics
Turbulent free energy consists of two parts:
Drive and damping terms:
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Energetics in wavenumber space
Damped eigenmodes are responsible forsignificant dissipation in the drive range (!)
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Some energy escapes to high k
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Resulting spectrum decays exponentially @lo k, asymptotes to power law @hi k
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Banon Navarro et al., PRL 2011
Shell-to-shell transfer of free energy
ITG turbulence (adiabatic electrons);logarithmically spaced shells
Entropy contribution dominates;exhibits very local, forward cascade
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Banon Navarro et al., PRL 2011
Free energy wavenumber spectra
Asymptotic self-similaritycoincides with power lawspectra
Measured exponents arerelatively close to those ofa 2D GK scaling theory[Schekochihin et al., 2009]
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Morel et al., submitted
Application: Gyrokinetic LES models
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Multiscale wavenumber spectra
Poloidal wavenumber spectraof density fluctuations for pureTEM / ITG / ETG turbulence
Poloidal wavenumber spectraof density fluctuations for mixed
TEM / ITG – ETG turbulence
NL (!) ETG drive
L ETG drive
Universality? Görler & Jenko, PoP 15, 102508 (2008)
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Summary and outlook
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Some outroductory remarks
Goal of this second lecture:Introduction to the physics of plasma microturbulence
Key insights:Nonlinear saturation may have different facesDrive and dissipation ranges overlap (damped modes!)Question of universality in plasma microturbulence
Topic of next lecture:On multi-scale aspects of plasma microturbulence
More info: http://gene.rzg.mpg.de