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Transition from Pervasive to Segregated Fluid Flow in Ductile Rocks James Connolly and Yuri Podladchikov, ETH Zurich A transition between “Darcy” and Stokes regimes Geological scenario Review of steady flow instabilities => porosity waves Analysis of conditions for disaggregation

A transition between “Darcy” and Stokes regimes Geological scenario

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Transition from Pervasive to Segregated Fluid Flow in Ductile Rocks James Connolly and Yuri Podladchikov, ETH Zurich. A transition between “Darcy” and Stokes regimes Geological scenario Review of steady flow instabilities => porosity waves Analysis of conditions for disaggregation. - PowerPoint PPT Presentation

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Page 1: A transition between “Darcy” and Stokes regimes Geological scenario

Transition from Pervasive to Segregated Fluid Flow in Ductile Rocks

James Connolly and Yuri Podladchikov, ETH Zurich

A transition between “Darcy” and Stokes regimes

• Geological scenario• Review of steady flow instabilities => porosity waves

• Analysis of conditions for disaggregation

Page 2: A transition between “Darcy” and Stokes regimes Geological scenario

Lithosphere

Partia lly (3 vol % ) m oltenasthenosphere

Basalt d ikes

Basalt s ills

M assive D unites

Replacive Dunites

Replacive Dunites = reactive transport channeling instab ility?Basa lt d ikes = self propagating cracks?

Basalt s ills = segregation caused by m agica l perm eability barriers?M assive Dunites = rem obilized replacive dunite?

M id-O cean R idge

lithosphere

Page 3: A transition between “Darcy” and Stokes regimes Geological scenario

1D Flow Instability, Small (<<1) Formulation, Initial Conditions

-250 -200 -150 -100 -50 0

2

4

6

8t = 0

z

-250 -200 -150 -100 -50 0-1

-0.5

0

0.5

1

z

p

1 1.5 2 2.5 3 3.5 4 4.5 5-1

-0.5

0

0.5

1

p = d, disaggregation condition

1D Movie? (b1d)

Page 4: A transition between “Darcy” and Stokes regimes Geological scenario

1D Final

-350 -300 -250 -200 -150 -100 -50 0

1

2

3

4

5t = 70

z

-350 -300 -250 -200 -150 -100 -50 0-1

-0.5

0

0.5

1

z

p

1 1.5 2 2.5 3 3.5 4 4.5 5-1

-0.5

0

0.5

1

p

• Solitary vs periodic solutions

• Solitary wave amplitude close to source amplitude

• Transient effects lead to mass loss

Page 5: A transition between “Darcy” and Stokes regimes Geological scenario

2D Instability

Page 6: A transition between “Darcy” and Stokes regimes Geological scenario

Birth of the Blob

• Stringent nucleation conditions• Small amplification, low velocities

• Dissipative transient effects

Bad news for Blob fans:

Page 7: A transition between “Darcy” and Stokes regimes Geological scenario

Is the blob model stupid?

A differential compaction model

Dike Movie? (z2d)

Page 8: A transition between “Darcy” and Stokes regimes Geological scenario

The details of dike-like waves

Comparison movie (y2d2)

Page 9: A transition between “Darcy” and Stokes regimes Geological scenario

Final comparison

• Dike-like waves nucleate from essentially nothing

• They suck melt out of the matrix

• They are bigger and faster

• Spacing c, width d

But are they solitary waves?

Page 10: A transition between “Darcy” and Stokes regimes Geological scenario

Velocity and Amplitude

0 5 10 15 20 25 30 353.4

3.6

3.8

4

4.2

4.4

4.6

4.8

5

5.2

time /

Blob model

amplitudevelocity

0 0.5 1 1.5 2 2.5 3 3.50

5

10

15

20

25

30

35

40

time /

Dike model

amplitudevelocity

Page 11: A transition between “Darcy” and Stokes regimes Geological scenario

1D Quasi-Stationary State

4.5 5 5.5-10

-5

0

5

10

15

20

25

30

35

x/

Horizontal Section

-60 -40 -20 0-10

-5

0

5

10

15

20

25

30

35

y/

Vertical Section

0 10 20 30 40

-6

-4

-2

0

2

4

6

p

Phase Portrait

Pressure,Porosity

Pressure,Porosity

• Essentially 1D lateral pressure profile• Waves grow by sucking melt from the matrix

•The waves establish a new “background”” porosity• Not a true stationary state

1

1

Page 12: A transition between “Darcy” and Stokes regimes Geological scenario

So dike-like waves are the ultimate in porosity-wave fashion:

They nucleate out of essentially nothing They suck melt out of the matrix

They seem to grow inexorably toward disaggregation

But

Do they really grow inexorably, what about 1?Can we predict the conditions (fluxes) for disaggregation?

Simple 1D analysis

Page 13: A transition between “Darcy” and Stokes regimes Geological scenario

Mathematical Formulation

• Incompressible viscous fluid and solid components

• Darcy’s law with k = f(), Eirik’s talk

• Viscous bulk rheology with

• 1D stationary states traveling with phase velocity

es

s

2 2q

11

d

1

q

mq

pv

f

f

es

s

pv

(geological formulations ala McKenzie have )

Page 14: A transition between “Darcy” and Stokes regimes Geological scenario

Balancing ball

gv ht x

v pxt z

0 ,p fz

x vt

1( )s

pfz

v g hx v x

sp Hp

0 hvdv g dxx

0 s

Hpdp d

2

2vE hg

2

2 spU H sg

Porosity WaveBalancing Ball

Page 15: A transition between “Darcy” and Stokes regimes Geological scenario

H(omega)

Page 16: A transition between “Darcy” and Stokes regimes Geological scenario

Phase diagram

Page 17: A transition between “Darcy” and Stokes regimes Geological scenario

Sensitivity to Constituitive Relationships