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Spectra of Gravity Wave Turbulence in a Laboratory Flume S Lukaschuk1, P Denissenko1, S Nazarenko2 1 Fluid Dynamics Laboratory, University of Hull – PowerPoint PPT presentation

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Title: Spectra of Gravity Wave Turbulence in a Laboratory Flume


1
Spectra of Gravity Wave Turbulence in a
Laboratory Flume
S Lukaschuk1, P Denissenko1, S Nazarenko2
1 Fluid Dynamics Laboratory, University of Hull 2
Mathematics Institute, University of Warwick
WTS workshop, Warwick- Hull, 17-21 September
2
Theoretical prediction forenergy spectra of
surface gravity waves
  • Phillips (JFM 1958, 1985)
  • sharp wave crests
  • strong nonlinearity
  • dimensional analysis
  • 1K. Kuznetsov (JETP Letters, 2004)
  • slope breaks occurs in 1D lines
  • wave crests are propagating with a preserved
    shape

3
2. Weak turbulence theory(Theory and numerical
experiment - Hasselman, Zakharov, Lvov,
Falkovich, Newell, Hasselman, Nazarenko 1962 -
2006)
  • Kinetic equation approach for WT in an ensemble
    of weakly interacted low amplitude waves
    (Hasselmann)
  • Assumptions weak nonlinearity
  • random phase (or short correlation length)
  • spatial homogeneity
  • stationary energy flow from large to small
    scales
  • Zakharov Filonenko spectrum for gravity waves
    in infinite space
  • is an exact solution of Hasselmann equation
    which describes a steady state with energy
    cascading through an inertial range from large to
    small scale (Kolmogorov - like spectrum) for
    gravity waves in infinite space

4
3. Finite size effects (mesoscopic wave
turbulence) Theory Kartashova (1998), Zakharov
(2005), Nazarenko (2006) et al
  • For the WTT mechanisms to work in a finite box,
    the wave intensity should be strong enough so
    that non-linear resonance broadening is much
    greater than the spacing of the k-grid (?2?/L ).
    This implies a condition on the minimal angle of
    the surface elevation
  • Discrete scenario (Nazarenko, 2005)
  • For weaker waves the number of four-wave
    resonances is depleted. This arrests the energy
    cascade and leads to accumulation of energy near
    the forcing interval. Such accumulation will
    proceed until the wave intensity is strong enough
    to the nonlinear broadening to become comparable
    to the k-grid spacing. At this point the
    four-wave resonances will get engage and the
    energy will propagate towards lower k. Mean
    spectrum settles at a critical slope
  • determined by dk 2?/L

5
Numerical experiments
  • Confirmation of ZF spectra
  • Zakahrov et al (2002-5),
  • Onorato (2002),
  • Yokyama (2004),
  • Nazarenko (2005).
  • Results are not 100 satisfying because no
    greater than 1 decade inertial range
  • Phillips spectrum
  • could not be expected in direct numerical
    simulations because
  • nonlinearity truncation at cubic terms,
  • artificial numerical dissipation at high k to
    prevent numerical blowups.

6
Field experiments P.A. Hwang, D.W.Wang,
Airborne Measurements of surface elevation
k-spectra, (2000)
7
Goals Long-term to study transport and mixing
generated by wave turbulence Short-term to
characterize statistical properties of waves in a
finite system
  • Advantages of the laboratory experiment
  • Wider inertial interval two decades in k
  • Possibility to study both weakly and strongly
    nonlinear waves
  • No artificial dissipation natural wavebreaking
    dissipation mechanism.

8
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9
Small amplitude
10
Large amplitudes
11
Typical spectra E? for small and large wave
amplitudes
A3.95 cm (??0.16)
A1.85 cm (??0.074)
12
Spectrum slopes vs the wave spectral density
Ef(f is from the inertial interval)
Inset spectral density Efvs the energy
dissipation rate
?0 avalanches and also Phillips ?1/3 WTT
13
Estimation of the Dissipation Rate
14
PDF of the wave crests
Tayfun M.A. J Geophys. Res. (1980)
15
PDF of the spectral intensity band-pass filtered
at f 6 Hzwith ??f 1 Hz
16
PDF of the spectral intensity Ef (f6 Hz, ?f1Hz)
17
Conclusion
Random gravity waves were generated in the
laboratory flume with the inertial interval up to
1m - 1cm. The spectra slopes are not universal
they increase monotonically from about -6 to -4
with the amplitude of forcing. At low forcing
level the character of wave spectra is defined by
the nonlinearity and discreteness effects, at
high and intermediate forcing - by the wave
breaking. PDFs of surface elevation are
non-gaussian at high wave nonlinearity. PDF of
the squared wave elevation filtered in a narrow
frequency interval (spectral energy density)
always has an intermittent tail.
Acknowledgements Hull Environmental Research
Institute References P. Denissenko, S.
Lukaschuk and S. Nazarenko, PRL, July 2007
18
Cross-section images water boundary detection
19
Boundary detection
20
k-spectrum
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