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Errachidia 2011 Errachidia 2011

Errachidia 2011 - PowerPoint Presentation

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Errachidia 2011 - PPT Presentation

Lecture 2 nonlinear equations from symmetry and conservation application to sand ripples Chaouqi MISBAH LIPhy Laboartoire Interdisciplinaire de Physique Univ J Fourier Grenoble and CNRS ID: 564886

errachidia 2011 anisotropy conservation 2011 errachidia conservation anisotropy derived sand ripples nonlinear mass modified dunes model eqs 1998 valance

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Slide1

Errachidia 2011

Lecture 2: nonlinear equationsfrom symmetry and conservation: application to sand ripples

Chaouqi

MISBAH

LIPhy

(

Laboartoire

Interdisciplinaire de Physique)

Univ

. J. Fourier Grenoble and CNRS

FranceSlide2

Errachidia 2011

normal

velocity

Remark

: in 3D

add

Gauss

curvature

and use surface

operator

Geometrical

formulationSlide3

Errachidia 2011Conservation constraints

Csahok, C.M., Valance Physica D 128 (1999) 87–1001) No conservation

1) Mass conservation

If

anisotropy

: Slide4

Errachidia 2011

Snowflacke

Dense pattern

Star

fishSlide5

Errachidia 2011« Weakly

 » nonlinear equations1) No conservation

x

z

h(x)

Kuramoto

-

SivashinskySlide6

Errachidia 2011

Spatiotemporal chaosSlide7

Errachidia 2011

KS

equation

and

this one can be made

free of parameterSlide8

Errachidia 2011

2) Mass conservationCase C=0 or small

Similar

to situation

encountered

in

crystal growth; O. Pierre-Louis, Phys.

Rev. Lett. 1998

Recent analysis by

Guedda and BenlahsenSlide9

Errachidia 2011

Indefinite increase of the amplitude Slide10

Errachidia 2011

3) No conservation with anisotropy

Benney

equation

(KS+KDV)Slide11

Errachidia 2011

Benney

eq

. derived

for step bunching

by C.M. and O. Pierre-Louis (PRE, 1998); see also

C.M. et al. Review of Modern

Physics 2010.And for

sand ripples

under erosion using a modified model of

Bouchaud et el. 1994.Valanace

and C.M., (PRE 2003)Slide12

Errachidia 2011

4) Mass conservation with anisotropy (case of sand ripples, dunes)

Modified

BCRE model (

Csahok

, C.M.,

Rioual, Valance, EPJE 2000) Slide13

Errachidia 2011

Spatio-temporal portaitSlide14

Errachidia 2011

No

consevation

C=0

consevation

anisotropy

anisotropySlide15

Errachidia 2011Conclusion

Classes of equations derived from symmetries and conservations Eqs can be weakly or highly nonlinear; identification by

scaling

This

provides

a powerfull basis to guide the analysis

Eqs. are consistent with those

derived from « microscopic

 » models

Application to dunes would be interesting

Next lecture: when is coarsening expected

?