what happens when ra grows large: turbulent convection statistical approach

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What happens when Ra grows large: Turbulent convection Statistical approach amics of individual (coherent) plu

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What happens when Ra grows large: Turbulent convection Statistical approach Dynamics of individual (coherent) plumes. Turbulent convection ( s =0.71, a =2 p , Ra=10 7 ). Turbulent convection ( s =0.71, a =2 p , Ra=10 7 ). Turbulent convection ( s =0.71, a =2 p , Ra=10 7 ). - PowerPoint PPT Presentation

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Page 1: What happens when Ra grows large: Turbulent convection Statistical approach

What happens when Ra grows large:Turbulent convection

Statistical approach

Dynamics of individual (coherent) plumes

Page 2: What happens when Ra grows large: Turbulent convection Statistical approach

Turbulent convection (=0.71, a=2, Ra=107)

Page 3: What happens when Ra grows large: Turbulent convection Statistical approach

Turbulent convection (=0.71, a=2, Ra=107)

Page 4: What happens when Ra grows large: Turbulent convection Statistical approach

Turbulent convection (=0.71, a=2, Ra=107)

Page 5: What happens when Ra grows large: Turbulent convection Statistical approach

Turbulent convection (=0.71, a=2, Ra=107)

Page 6: What happens when Ra grows large: Turbulent convection Statistical approach

Turbulent convection:

Statistical properties andtransition from soft to hard turbulence

Scaling of the heat transport:Nu vs Ra

Nu =Qtotal / Qconduction= 1 + < w >

Page 7: What happens when Ra grows large: Turbulent convection Statistical approach

Turbulent convection

Page 8: What happens when Ra grows large: Turbulent convection Statistical approach

Turbulent convection

Page 9: What happens when Ra grows large: Turbulent convection Statistical approach

Turbulent convection

Page 10: What happens when Ra grows large: Turbulent convection Statistical approach

Turbulent convective plumes

Page 11: What happens when Ra grows large: Turbulent convection Statistical approach

Clustering of plumes andformation of large-scale order

Large-scale wind and generation of mean shear (rectification process, k=0):

Krishnamurti and Howard (1981)Howard and Krishnamurti (1986)

Massaguer, Spiegel and Zahn (1992)

Large-scale wind leads to plume clustering: Heslot et al (1987)

Kadanoff (2001)

Instability of the long-wave modes inturbulent convection: Elperin et al (2003)

Numerical simulation with periodic b.c.:No k=0 mode

Hartlep, Tilgner and Busse (2003)Parodi, von Hardenberg, Passoni, Provenzale, Spiegel, PRL (2004), PLA (2008)

Page 12: What happens when Ra grows large: Turbulent convection Statistical approach

Coarsening of the plume pattern:

Page 13: What happens when Ra grows large: Turbulent convection Statistical approach

Coarsening of the plume pattern:

Page 14: What happens when Ra grows large: Turbulent convection Statistical approach

Coarsening of the plume pattern:

Page 15: What happens when Ra grows large: Turbulent convection Statistical approach

Coarsening of the plume pattern:

Page 16: What happens when Ra grows large: Turbulent convection Statistical approach

The coarsening is due toclustering of convective plumes:

Page 17: What happens when Ra grows large: Turbulent convection Statistical approach

Turbulent RB convection undergoesa process of energy transfer

from the scales of the linear instabilityto the largest scales (box size).

At later times,the system becomes statistically stationary.

Page 18: What happens when Ra grows large: Turbulent convection Statistical approach

It is not a mean shear ( k = 0 )but rather a circulation at the largest scales (k=1)

The large-scale structures areclusters of individual plumes

Page 19: What happens when Ra grows large: Turbulent convection Statistical approach

The large-scale wind in closed containeris probably due to the same process,

with the energy piling up at the k=1/2 mode

It is not the large-scale circulation that generates plume clustering but viceversa

Page 20: What happens when Ra grows large: Turbulent convection Statistical approach

Is there an upper scale where the clustering is arrested ?

How does the clustering depend on theRayleigh number ?

Page 21: What happens when Ra grows large: Turbulent convection Statistical approach

Is there an upper scale where the clustering is arrested ?

Page 22: What happens when Ra grows large: Turbulent convection Statistical approach

Is there an upper scale where the clustering is arrested ?

Page 23: What happens when Ra grows large: Turbulent convection Statistical approach

Dependence on the Rayleigh number

Page 24: What happens when Ra grows large: Turbulent convection Statistical approach

What causes the clustering ?

Option 1: attraction of same-sign plumes

Option 2: the interaction of the lower and upper

boundary layers by the agency of plumes

Other view:The fixed-flux instability of a coarse-grained field

( with Reff << R )

Page 25: What happens when Ra grows large: Turbulent convection Statistical approach
Page 26: What happens when Ra grows large: Turbulent convection Statistical approach

In the fully turbulent regime, the system recovers a “statistical” roll pattern

Page 27: What happens when Ra grows large: Turbulent convection Statistical approach

Convection has still a lot to teach:

Effect of rotation

Transport

Predictability

Simplified models of moist convection

Page 28: What happens when Ra grows large: Turbulent convection Statistical approach
Page 29: What happens when Ra grows large: Turbulent convection Statistical approach

A summary of NS and fully-developed turbulence

(incompressible, homogeneous flow)

∇⋅r

u = 0

∂t+

r u ⋅∇

⎝ ⎜

⎠ ⎟r u = −∇p + ν 0∇

2 r u

Non dimensional version

∇⋅r

u = 0

∂t+

r u ⋅∇

⎝ ⎜

⎠ ⎟r u = −∇p +

1

Re∇ 2 r

u

Reynolds number : Re =UL

ν 0

Page 30: What happens when Ra grows large: Turbulent convection Statistical approach

A summary of NS and fully-developed turbulence

(incompressible, homogeneous flow)

In the limit :

formation of boundary layers

Re → ∞

Page 31: What happens when Ra grows large: Turbulent convection Statistical approach

Far from boundary layers:

inertial range(Kolmogorov 1941,

or K41)

ετ

=u3

l= constant → u ≈ l1/ 3

E(k)dk ≈ u2 ≈ l2 / 3

k ≈1/ l

E(k) ≈ k−5 / 3

log k

log E(k)

k-5/3

E

Direct energy cascadefrom large

to small scales