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Caustics and symmetries in optical imaging. The example of convective flow visualization
A. Joets, R. Ribotta
To cite this version:
A. Joets, R. Ribotta. Caustics and symmetries in optical imaging. The example of convective flow visualization. Journal de Physique I, EDP Sciences, 1994, 4 (7), pp.1013-1026. �10.1051/jp1:1994181�.
�jpa-00246961�
J. Phys. I Fiaiic.e 4 (1994) 1013-1026 JULY 1994, PAGE 1013
Classification Fhysics AbsU.acts
42.20C 42.30V 47.80
Caustics and symmetries in optical imaging. The example of
convective flow visualization
A. Joets and R. Ribotta
Laboratoire de Physique des Solides, Bât. 510, Université de Paris Sud, 91405 Orsay Cedex, France
(Received19 Januaiy J994,
accepted
J8 Mait.h 1994)Abstract. lt is shown that
qualitative
andquantitative
information can be callected from the study of the fuit caustic formedby light
rays deflectedby
some medium. Thestudy
necessitates the calculation of the ray trajectones along with a detailed balance of thesymmetries
of the whole set- up. As an example we consider the case of the causticproduced
by parallel rays interacting with aperiodic
convective flow in aliquiô
crystal. Theamplitude
of the flow and ail its essential featurescan be deduced, indicating that a caustic carries more information than a simple image.
l. Introduction.
Light
rays deflected eitherby
a transparentinhomogeneous
medium orby
a deformed surfacecon
provide
information on theinhomogeneities
or the deformations. This is the basis of imagingtechniques
that arewidely
used in macroscopicexperiments. Usually,
transmitted rays are deviated because of indexchange
in space, while reflection images are used toanalyse
surface deformations.
Among
the most familiarexamples
is the visualization of flows(open flows,
confinedpenodic
flows,turbulence...).
Another case isprovided by
theoptical techniques developed
tostudy
the elastic deformations in aliquid crystal subjected
to someexternat
field,
withapplications
tooptical
devices. IngeneraL
thesetechniques
can givequalitative
information about the structures, but it is difficult to extract quantitativemeasurements, except may be concemmg
geometncal
characteristics(distances, angles).
And, actually,
there is a need to increase the information contained in the images and for instance, it is important to trace back to theamplitude
of the deformation.What is called an
image
is the sectionby
someplane
of thefamily
of emerging rays.Generally,
thisfamily
admits a surfaceenvelope,
the caustic, named so because at every of its points thelight
intensity issharply
increased. It is this surface whichinstead,
contains the information conceming the structure of the deformation understudy.
This surface may itselfcontain
smgulanties
of lower dimension that appearbrighter.
Now, a focussedimage
of agiven
object
is obtamed when theplane
ispositioned
in such a way that it contains thesebrightest singularities.
Anexample
isgiven by figure1.
One may presume that a betterknowledge
of the fuitcaustic, including
ail thepossible singularities,
is necessary to have amore correct
interpretation
of the images. As an illustration of thisapproach
we shall considera rather
simple
case of 2-Dperiodic
flow structuredeveloped
in aliquid crystal.
Thisstudy
wasfirst motivated
by
the interpretation of the differentlight
patterns causedby
the various flowstructures
developed
on the way to the chaos.B A
focal
plane
virtual caustic
a) b)
Fig. a) Photograph of an image of the conveciive layer. The bright thick line~ are the sections of the virtual cones
by
the focal plane of the micro~cope, locatedslightly
below the cusps. The twmning isindicated
by
the different separation distances A and B, Some fines are destabilized into some points clo~e to a defect ofpenodicity
(di;location), where the flow iscomplex
and 3-D (see text). b) Sketch of thec;tu;tic in 3-D.
2. Basic elements on caustics in
periodic
flows.An
optical
caustic is defined as theenvelope
of a givenfamily
ofnonparallel
rays[1] (Fig. 2).
If the rays are
parallel
the caustic isformally
a pointrejected
toinfinity. Any
system that has the property ofdeflecting
incidentparallel
rays for instance, willproduce
a caustic in the near field, 1-e- this caustic ispulled
back frominfinity.
The firstexample
that camesnaturally
tomina is the focal point of a converging lens. The process of ideal image formation
through
aperfect
lens associates a point caustic with every sourcepoint. However,
this caustic is unstable again~t infimtesimal deviations fromperfect
focahsation,producing
then the well- known effects ofspherical aberration,
coma, astigmatism.rays
causti
Î'
Fig. ?, A caustic is the envelope of a
famfly
ofnon-parallel
rays.N° 7 CAUSTICS, SYMMETRIES AND FLOW VISUALIZATION 1015
Other familiar
examples
of caustics are thedancing bright
[mes at the bottom of apool
due to the focalisation of Sun raysby
theirregular
surface of the water, and also thesparkling
of the reflected Sun raysby
the same surface. Less obviousexamples
in theatmosphere,
are the formation of mirages and of rainbows.From a mathematical
standpoint
caustics aresingularities
that may be either stable or unstable[2-4].
It is shown that the stablesingularities belong
to a small number of classesfolds,
cusps,swallowtails,
umbilics...However,
the focalpoint
of an idealconverging
lens does not appear in this classification because it is unstable(degenerate)
and the effect of aperturbation
is todecompose
it into a set of those stablesingularities.
An index modulation in space is
commonly
assimilated to a lens. Periodic convective flows realise aperiodical
set of such lenses. Indeed, a prototype is theRayleigh-Bénard
convection of aloyer
ofisotropic
fluid where the thermalgradients
modulate the index of refraction.Another
example
is givenby liq,Jid crystals
in which the index of refraction isspatially
modulated
by
convective rolls. These rolls areproduced
under the action of a tran~verse electric field across aloyer,
and areperiodic
in one direction of space and invariantby
translation
along
their axis[5, 6].
Theproblem
of caustic formation reduces to a 2-D onecorresponding
to the basicexperimental
situation. We shallgive
acomplete description
of the caustics formedby
the emergent rays and alsoby
their continuation the real and virtual caustics. Then we shall calculate the raytrajectories
inside the nematicloyer
and we deduce theenvelope
of the rays.By comparing
the simulation with ourexpenmental
values we are able to estimate theamplitude
of the convection. We Shall aisestudy
therelationship
between the symmetry of the caustic and the symmetry of the index modulation. As anexample,
the so- called «squint
effect » shall beremterpreted.
As the structure of the flow becomes more
complicated (at higher
values of the electric field)one observes that the caustic becomes unstable and now contains other types of
singularities
that necessitate a 3-D
analysis
which will bepresented
in anotherpublication.
3. Observation of caustics in the electroconvection of a nematic
layer.
Nematics are
composed
ofelongated
molecules, whose local orientation defines a newmacroscopic
variable,
the directorusually
denotedby
a unit vector m. It is understood thatdirectors of opposite sense are
equivalent
mm m.Optically,
the nematics are uniaxialmaterials,
theoptical
axislying along
the director. The nematic(Merck
PhaseV)
has anordinary
refractive index n~ =1.65 and an
extraordinary
refractive index n~ 94. Theliquid crystal
is sandwiched between twoconducting semi-transparent plates (plane (.r,y))
separated by
atypical
distance of d=
100 ~Lm.
By
an appropriate treatment of theplates
oneimposes a uniform molecular
alignment
in theplane
of theplates (planar anchoring) along,
say, the >.-axis. In the rest state the nematic
loyer
constitutes ahomogeneous
uniaxial medium ofoptical
axis m= x.
When an AC
voltage
v, oftypical frequency f
=
100 Hz (« conduction regime »
[5]),
isapplied
across theloyer
and fixed at some valuejust
above the thresholdv,
= 6 V, the reststate is destabilized and the convection
develops
in the form of astationary
structure ofperiodic rails,
ofperiod
A= 2 d. The axis of the rails is normal to the initial direction,; of the molecules and this is the « normal roll structure »
[6].
Because of thecoupling
between thehydrodynamic velocity
and the director, the molecularalignment
isperiodically
distortedalong
x, the maximum of the distortionbeing
at the roll centers(Fig. 4).
Alight
beam,polanzed along
x, is sentnormally
to theplates.
Inside theloyer,
the effective local index for eachincoming (extraordinary)
ray isperiodically
modulatedalong,;.
In a rather primarydescription,
theloyer
con be reduced to a set ofalternately diverging
and converging lenses[7].
After traversing the nematic the rays refract at theliquid crystal-glass
interfaceFig. 3.-Microphotograph
of the caustic. The sampie is tilted around.< by 40°. The image istopologicaliy equivalent
to a vertical section of the caustics. Note that the virtual cusps are destabilized into unfolded butterflies.= =
d
(contrary
to the incident rays which are normal bath to theglass-liquid crystal
interface= =
0 and to the
optical
axis m=
x).
Theoutgoing
rays are focalizedalong
a real caustic and theirprolongation
below the upper interface appear focalizedalong
a vii.tuai caustic. Thelight
pattern is shown usmg apolarizing
microscope, which grues the section of the caustic in its focalplane (Fig. l).
In the literature these caustics are
usually
reduced to a set of « foci », or« focal
points
»(in
the
(x, z) plane).
A more carefulstudy
of these points[8]
has shownby
a reconstructiontechnique
thatthey
are in fact thetips
of a small portion of the caustic, in the forrn of a cane. In order to obtain at once animage
of the caustic wesimply
rotate thesample
around the x-axisby
an
angle
of about 40°. Due to the mvariance of the normal rollalong
y, theresulting image
istopologically equivalent
to the section of the caustics in the verticalix, z) plane (Fig. 3).
Wesee
clearly
that the caustic iscomposed
of a sequence of canesalternately
orientedupwards
and downwards. In the
language
ofsingularities,
ail points of the caustic are « foldpoints
», except the tips of the canes which are « cusp points ». In practice, the term cusp means rathersome finite portion of the caustics around a cusp point.
According
to thetheory
ofsingulanties [9],
the two fold-curves of a cane connecttangentially
at the cusp-point, as con beseen in
figure
3. The cusps are the so-called« focal points » where the
light
intensity is muchhigher
thonanywhere
else on the fold-curve. We check that the real cusps are located above the separation fines between twoadjacent
rails(Fig. 4).
We name them up-cusps ordown-cusps
N° 7 CAUSTICS, SYMMETRIES AND FLOW VISUALIZATION loi?
real caustics
outgoing down~cusp
rays
~
up"cusp g<ass
~
,"'~"', ,"'~"i
liquid
' '
ctysta<
~
,
/ ,, /
x
', ,,' ,,_,,,'
glass
inccming
rays
virtual caustics
Fig. 4, Simulation of the ray
trajectories
(thin hnes) and of the caustic (thick fines). The model for the molecular distortion is q~= q~o sin Lt sin q= (with q~o 21,2°, A
=
2 «IL
=
393 ~Lm, d ar/q
=
308 ~m). The arrows represent the director in the midplane of the layer. The convection is indicated by
the dashed fines. The small circles indicate the expenmental points from the observed caustics. The fit is made by adjusting at once the
majonty
of theexperimental
points on the theoretical caustic curve. The typical error bar is mdicated on the lowest point on the left side of thefigure,
The mirrors M passmg through each real cusp are intercalated with the virtual cusps.depending
on whether the flow movesalong
z or z. The canes are net limitedalong
z.They
con
easily
be observed up to distances of the order of 20 d. The caustic presents remarkablegeometncal
charactenstics. For instance, the down-canes are net identical to the up-canes their cusp-points have a distinctheight.
This is netexpected
at first from arapid
consideration of the model for the flow, We aise observe that the virtual cusps are netequidistant along
x.This effect was named « squint »
il 0]
and attributed to somenonlineanty
in the electroconvec-tive mechanism,
although
it is observed even at or near the threshold. In thefollowmg
model,we shall show that this effect con be
explained differently.
It is observed that, for values of the constraint
F =
(v v, )/v~
m0.15,
each virtual cusp isreplaced by
a ensemble of three cusps(unfolded butterfly singularity) (Fig. 3).
This observation will be discussed later.4.
Equations
for the rays.We first calculate the ray
trajectories
inside the nematiclayer.
Thisproblem
can be soJvedby
severalgeneral
methodsil 1-13]. Here,
weapply
Fermat~spnnciple
which can be shown to be valid in ananisotropic
medium[12].
It states that the rays are the extremals of theoptical path
[
= n ds. where n ii the local ray index and ds is the curvilinear abscissa
along
thepath.
Here, ii is given
by iii.
n =
,/nj sin~
p+
nj cos~ p
Ilwhere p is the
angle
between the localoptical
axis m and the local tangent vectorr =
(ài/ds, dj'/ds)
to the ray.Assuming
that ail the rays passthrough
theloyer,
which is checked in the expenment, we can choose = as theindependent
variable and >. as the unknown function r =,r(=). Theoptical path
now takes the form[
=
~~
L d== ii
(=,,;(=),
~jl
+
~°~ ~
dz.
(2)
=,, =~
d= d=
It is convenient to mtroduce the
angle
q~ between the,;-axis and m, so thatp
(=, >.,il
=
q~(,;, z) + arctan Il,i. (the dot indicates the derivation with respect to =). As
usual,
we assumethat the director is
harmonically
distorted : q~= ~ao sin kx sin q=
(k
= 2 «IA, q
=
«Id).
The equation for the rays is obtainedby
writting theEuler-Lagrange equations
for the functionnal L, i.e. that the first variation of theoptical path
is zero for the actual rays. The equation for therays is then :
~2,,.
(i +.i.2) (n~ (.i~= v~,)
npp (.i.~a~ + v~=))~ ~~~
I' + nôô
where the
partial
derivatives are notedby subscripts
~a, éq~/é>., n~ = én/ép, etc. Anequivalent
form of equation(3)
wasgiven by Kosmopoulos
andZengmoglou,
whoanalyzed
the grating action of such a nematic
loyer [14].
The differential equation of second order
(3)
isintegrated
with the classicalRunge-Kutta
method of order 4. The step of
integration
d= is takenequal
to d/200. The incident rays areParametrized by
the,r-coordinate A of their entry point. The raysbeing
normal to theloyer,
the initial dataare.;(0)
= A,
,k(0)
=
0
(the loyer
is definedby
0 w = w dj. The abscissa of the entry point is taken between 0 and A.Figure
4 shows anexample
of such a simulation of the raytrajectories.
Before
Jeaving
the nematiclayer~
the rays are refracted on theliquid crystal-glass
interface= =
d. In order to test the model
quantitatively
this refraction must be included in thecalculation. The relation between the
angle
of incidence i=
arctan1.(d)
and theangle
ofN° 7 CAUSTICS, SYMMETRIES AND FLOW VISUALIZATION 1019
refraction
a con be extracted from the
general
laws ofcrystals optics Ii
n(
tan isin a
=
~
(4)
n~(ni
+n( tan~ 1)'~
where n~ is the refractive index of the
glass.
We now consider a set of incident rays
parametrized by
A. Afterpassing through
thelayer
and
refracting
at theliquid crystal-glass interface,
the rays follow again a rectilineartrajectory
characterizedby
two parameters : theabscissa,ro =.;(d)
of the exitpoint
and theangle
of refractiona. Of course,,~o and
a
depend
on A.5. Calculation of the caustic curve.
The set of the
emerging
rays constitutes a one-parameterfamily
ofstraight
fines, Its equation is>.
=,~o(Àj+ (d-z>tan a(À), (5>
The caustic is
by
definition theenvelope
of theemerging
rays, that is, the locus where« two
neighbouring
rays intersect». This is
expressed by
zeroeing thepartial
derivative of,r with respect to(see [15]
andappendix)
é>./éA
= 0
(6)
Equations (6)
and(5)
define the caustic as a curveparametrized by
A.Explicitly,
we obtain>~j(À)cos ce(À)sin
a(À)x(À
=
xo(À
~, ~
>j(À cos~
a (À
~~~
Z(À)
# d+~,~~~
where the
prime
denotes the derivation with respect to A. For each value of A, the values,ro(A )
and a (A are calculatedby
the method described in thepreceding
section. Then, thecaustic curve is deduced
by equation (7) (the
derivatives with respect to arenumerically
obtainedby
the central-differencemethod).
The result is shown infigure
4.Experimentally,
the position of points of the caustic is determinedby varying
theheight
of the localplane
of themicroscope.
These arereported
in the samefigure.
A fit is obtainedby adjusting only
one parameter theamplitude
q~o of the molecular distorsion so that themajority
of thepoints
lie onthe curves. Since the caustic is the ensemble of the cones the fit is not made for each cone
separately,
but rather for ail the cones at once. A rathergood
fit is obtained for q~o =21.2°. The asymptotic branches of the caustic
correspond
toa'(A
=
0. The real and virtual
cusp-points correspond respectively
to the local minima and to the local maxima of theheight
z.They
are then givenby
~~
=
0
(8)
(see
theappendix
for arigourous presentation).
In previous articles[7,
16,17],
in whichapproximations
were made, someanalytical
formula was given for theheight
of the cusps.Here,
on the contrary, theheight
can be deduceddirectly
from the calculation of the wholecaustic and without any approximation. However another more
powerful
method can bedenved if one is interested
only
incalculatmg
theheight
of the cusps. This method will be described in aforthcommg
paper.6. Caustics and
symmetries.
The presence of
symmetries
is, among the essentialgeometrical
characteristics of the caustics, the most noticeable feature.Here,
the caustic isperiodical along
>., with the samepenodicity
A as that of the flow pattern(Fig. 4),
measuredby
another method[6].
We notice from theexperiment
that the real cusps areequidistant
withpenod
A/2along,;,
while the virtual cuspsare twinned
(twins separated by A)
and each pairseparated by
B such that A + B=
A. The whole set of cones
(real
and virtualones)
has the mirror symmetry the mirror is vertical and passesthrough
a real cusp(a
vertical fine m theplane
of thefigure). Obviously
there is a mirror for each real cusp, and no mirror for the virtual ones. This may indicate a symmetrybreaking,
as
proposed by
Ben-Abraham[101.
One also notices that thedown-cusp
and the up-cusp are notequivalent by superposition
and are at differentheights.
In order to understand thelight
pattern, one must examine ail the
possible symmetries
of the fuit system.Owing
to Curie'sprinciple il 8]
one must indude in thisdescription,
theliquid crystal,
thelight
beam, the interactionlight-matter
and theboundary
conditions. Thisprinciple
states that« the symmetry elements of the causes must be present in the effects
produced
» In our system, it is clear that we may take thelight
pattem as the « effect », and the directorfield, conjointly
withboundary
conditions and the incident beam, as the « cause ». Now theproblem
to solve is the
relationship
between the effect and its cause. Inparticular,
is the symmetry of the tlowdirectly
reflected in the caustic ?The nematic
liquid crystal
is characterizedby
its director field which bears the localoptical
axis. A
simple
way to define a symmetry of the director field is to consider how it istransformed
by
adisplacement f (punctual
affine transformation of thei-i, z) -plane
preservingthe
distance). By
the transformationf,
apoint
P is transformed into the pointf(P)
and any vector attached to P is transformedby
the first derivativef'(P) (1.e.
the Jacobian matrix)off
into a vector attached to
f(P) (Fig. 5).
We note that the derivativef'(P)
transforms also the directions attached to P into directions attached tof(P) (this
results from thelinearity
of the operatorf'(P)).
One can say that the director fieldm(P)
is invariantby
the transformationf,
if111~f(P)
#
f'jlll(P))
119j.
Let us now assume that the director field m has a symmetry
f,
and let us compare theoptical
path along
some curve C,parametrized by
s, and theoptical path along
the transformed curvef(C), parametrized by
s'.Observing
that the local index ndepends only
on theangle p
between the director m and the local direction ds=
(dà., dz)
of the curve, and also thatf'(P)
preserves thisangle (or
at least itsmagnitude),
we can wnte1'
,ÎIÎ
~~~
~~' "~
n
lP
ds~
(9)
where
p'
=
(m(s'), ds') (Fig.
5). We have also used the fact that ds ispreserved by f.
Theoptical paths along
C andf(C
areequal.
As a consequence, the rays, which are the extremals of theoptical path,
areexchanged
into one anotherby
the transformationf.
If now theboundary
conditions and the incident beam both have the symmetry of the director field, then the ray
trajectones
form a setglobally
mvariant under the same transformation. In this case, theenvelope
of the rays, i e. the caustic, is aise invariant under the transformation. Moregenerally,
the symmetnes of the caustic reveal the symmetry elements common to the director field, the incidentlight
beam and theboundary
conditions.Let us now interpret the
geometrical
features of the caustics observed in our experiment. Thepenodicity
of the causticsalong
the ~;-axis is that of the director field. The presence of the vertical mirrors passingthrough
the real cusps indicates that the director field has this mirror symmetry. Examination offigure
3 does not reveal any other symmetry. Now [et us mtroduceN° 7 CAUSTICS, SYMMETRIES AND FLOW VISUALIZATION 1021
L
i i i i i
_ -
d~
fi fi'
~ f ~
~
Ù~~~~~~~
i
Fig. 5.
Example
of a tran~formation (symmetry with respect to L) facting on the point P and on the director m,the symmetry elements of the
boundary
conditions and of the incidentlight
beam. Theboundary
conditions concern the lower and upperseparation planes
between thehquid crystal
and the
holding plates.
There, in addition to theprevious
vertical mirrors, one has the horizontal mirror located in the middle of thelayer
andconsequently
an inversionpoint.
Theboundary
conditions are also invariantby
continuous translationsalong
x.Indeed, they
have the maximalpossible
symmetry. For a source locatedonly
on one side of thelayer,
as it is in the expenment, the incident beam issymmetrical by
ail translationsalong.~
and in everyvertical mirror,
But,
in order to becomplete,
one must aise consider an identical source locatedon the other side. There is indeed no a
priori
reason for the structure in thelayer
to have the reversaisymmetry,
forexample
the mirror symmetry about the median fine. This is achievedexperimentally, by simply
tuming thelayer upside
down. In thisoperation,
the new caustic isclearly
deduced from the previous oneby
an inversion relative to a point located in the centre of the rolls. At some abscissa x, a up-cusp of the former caustic isreplaced
on the other side of thelayer by
adown-cusp (Fig. 6).
The up-cusp is recoveredby translating
the causticby
,
~. _" ..
_"
L,1: ~,
: j[ ;(
Î
," ~. ;~ ~.
; source is below
~, 'l ~ :
i
._ / i
"_ i source <sabove
O
,
.- -'
> J fl '
]r l'
.lÎ ,[
." '.
' Î
.'. f
l Il ÎÎ Î
1 Z ~ Î
'fl
Fig. 6. The fui] caustic produced by the incident beam coming from below (resp. above) is indicated
by the thick
(resp.
dotted) fines, The director fieldcorresponds
to the standard model. lt shows the symmetry 5, generated by a mirror (the dashed vertical fine), and an inversion around the center of the point located in themid-plane
of the layer. The nematiclayer
is confined between the two horizontal fines, The fui] caustic does have the same symmetnes.,4/2. Moreover the
twinning
effect is still present andundergoes
the same transformation. In conclusion, theknowledge
of the fuit caustic(the effect),
and that of the two components of thecause, enables us to deduce the symmetry elements of the last component of the cause, i-e- the
structure.
This
study
can besupplemented,
in this case, where we know some of the features of the flow structure,by using
the classification of the symmetry groups for a 2-Dlayer.
Here, thereis a
periodicity along
an axis,~, and then, the classificationgives
seven symmetry groups[20].
These are the groups of the patterns obtained
by repeating
some motifs on a fine. Here we choose to represent the motifsby appropriate alphabet
characters. Thus the seven patterns are1)
...LLLL..2)
...rLrL...3)
VVVV...4)
...NNNN...5)
AVAV..6)...DDDD...
7)
HHHH... We notice that the symmetry groups 6 and 7 are notcompatible
with a non-zero molecular distortion at the roll centers and that the symmetry groups 1, 2 and 4 do net contain the mirror symmetry. The choice is between the symmetry group 3,generated by
two verticalparallel
mirrors, and the symmetry group5, generated by
one vertical mirror and one inversion(Fig. 6).
In order to reveal apossible
inversionpoint,
one must insure that the two componentsof the cause under control have this inversion
point.
This is what has been madeby reversing
the
sample.
One is left withgroups.
This is the maximal symmetrycorresponding
to aconvective flow in form of rolls
filling
the whole thickness of thesample.
Let us now examine the
particular
distribution of the virtual cusps.First,
one notices that the real cusps possess the symmetry with respect to the vertical mirror passingthrough
them. Thisis associated with their
equidistance along.i (periodicity A/2).
On the contrary, there is no mirrorpassing through
the virtual cusps, but rather there is a mirrorpassing
inbetween with thesame
periodicity
A/2. This does notimpose
anequidistance
between the virtual cusps, inwhich case the
periodicity
of the cusps is A. Thisparticular
distribution of the virtual cusps isdue to the convective flow cell characterized
by
an inversionpoint,
the centre, and the absenceof any vertical mirror. It
might
appear inexperiments
that the virtual cusps are very close toequidistant,
but this would be rather due to someparticular
values of the parameters. Thegenerality
is that those cusps are netequidistant
but are rather twinned.Then,
there is no need to invoke the effect of the nonlinearities, contrary to what is assumedm reference
[2 Ii
in order tointerpret
this result. In the paper citedhere,
thenon-equidistance
was ascribed to some
particular
flow structure(squint)
that wouldimply
the absence of any inversion point. On the contrary, theexperiment clearly
shows the presence of such symmetry.Moreover, it can
hardly
be the result of nonlinear effects, smce the twinnmg is observed even within fl above threshold.The same reason, i-e- the absence of any vertical mirror
passing through
the centre of theroll, implies
that the up anddown-cusps
are notnecessarily
identical. Indeed the experiment indicates thatthey
appear at differentheight (Fig. 3).
7. Discussion.
Let us
point
out that these results can begeneralised.
We first consider the effects of ananharmonicity
of the molecular distortionalong,;.
As
already
mentioned, far above the convection threshold nonlinearities come intoplay
and the virtual cusps evolve towards morecomplex shapes (Fig. 3).
This effect can beexpected
from the presence of
higher
harmonies in the molecular distortion. The numerical simulation ofthe caustic is now made after
mtroducing
two harmonies in the previous model for themolecular distortion ~
= (q~o sm k,; + a sin ? k,; + b sin 3 k>. sm qz. The result shown in
figure
7 agrees quite well with theexperimental
observation. Then theanharmonicity
can be reflectedby changes (instabilities)
in thetopology
of the caustic. The symmetry is conserved,N° 7 CAUSTICS, SYMMETRIES AND FLOW VISUALIZATION 1023
Fig.
7, -Simulation of the caustics for a molecular distortsion q~containing
3 harmonics : q~=
(q~o sin k~r + a sin 2 kV + b sin 3 k> sin q= with q~o 0.377, a
=
0.005, h 0.0285. The virtual cusps
are replaced
by
« butterflies» (3 connected cusps). Compare with
figure
3.because of the symmetry of the chosen harmonies. In the
general
case, it islikely
that another type of harmonic with a differentsymmetry
would induce a symmetrybreaking
of the caustic,We have studied the case where ail the rays are
parallel
to the(,;,
=-plane
and theproblem
is
essentially
2-D. The basicequations
for the caustic(6)
and(8)
have there asimple interpretation
and do notjustify
a mathematical demonstration.However,
for other convectivestructures that break the continuous translational invanance
along
thej,-axis,
for instance thevancose structure
[6],
theproblem
becomes 3-D, It needs a mathematical formulation based onthe
theory
of thesingularities.
Such ananalysis
is sketched in theappendix
for the 2-Dlight
patterns, and will bedeveloped
in detail for 3-Dlight
patterns in aforthcoming
paper.However,
our statement that the fuit caustic has thesymmetries
common to the director field, theboundary
conditions and the incidentlight
beam, ismdependent
of the dimension of thephysical
space.Consequently,
it remains valid in the much moregeneral
case of the3-D-light
patterns. It is also vahd for other types of materais,provided
that the refractive indexdepends only
onangles,
so that equation(9)
holds. Inparticular,
our resultsapply
to the case of biaxialliquid crystals.
The symmetnes considered in the
previous
section aregenerated by punctual
transforma- tions,namely displacements. They
act on thepoints,
the vectors and the directors. We may also define local transformations whichkeep
thepoints
invanant and which actonly
on thevectors or on the directors. For
example
[et us consider the standard model for the director fieldq~ = q~o sm k.r sin qz and the local mirror symmetry t around the >.-axis
(Fig. 8).
This director field is not invariantby
t.Composing
t with the mirror f in themid-plane
of thelayer,
wedefine the transformation
f
*= t o
f.
The director field is invariantby
Î * while theoptical path
is net conserved
by f* Then,
the reasoning that we have usedthroughout
this article is nolonger
valid, and the symmetry f * cannot be evidenced in the caustic.Generally,
the caustic will notnecessarily
contain these local symmetries. Thisimplies
that the causticmight
notreveal the fine structure, for instance of the flow or of the index
distribution,
thusrestrictmg
theamount of information that one can extract from a caustic.
A wider class of
symmetries
isprovided by diffeomorphisms,
i e.bijective
and differentiable point transformations. It is obvious that here too, our conclusions on thesymmetries
of thecaustic are identical,
provided
that equation(9)
holds. Thisproblem
would deserve adeeper
G ~Î----x
~ ai@--u--x
~
~~p~=p t(m>
i(P)
nô)
~~
--/-~
x
~
Fig.
8. -a) Definition of the local mirror symmetry t around the ~< axis, and of the global mirrorsymmetry Î around the,t axis. b)The director field in the convection flow does not possess both symmetnes t and
Î,
but the symmetry Î*= ta Î.
study.
We noteonly
that it can be formalized in terms of isometries of the metric space, whose fine element is definedby
theoptical path
element nds(cf. [13]).
For the state of comparison with our
example,
[et usfinally
consider the muchsimpler
caseof thermal convection in
isotropic
fluids(Rayleigh-Bénard convection)
close to the threshold.There,
the index is a function of thetemperature
distribution. Itsperiod along
x is thepenod
A of the flow. The real caustics nowcorrespond
toonly
one direction of the vertical flow(downwards)
while the virtual onecorresponds
to theupwards
motion. There are no other cusps. With each cusp is associated a vertical mirror. Thus ail cusps areequidistant.
8. Conclusion.
We have
analysed
in detail theg~umetry
of thehght
pattemproduced by
apenodic
flow in alayer.
We have taken as anexample
the convection in a nematiclayer mainly
because it alsoincludes an
anisotropy,
thusmaking
theexample
richer and of a wider interest than theisotropic case. The
light
pattern is the section of a surface, the caustic which issingular
and which containssingularities
of lower dimension. Theequations
for the rays have been derived,and the fuit caustic has been calculated. It is found to be in
good
agreement with theexperimental
observations. Theamplitude
of the molecular distortion has beendirectly
deduced
by fitting
with theexpenment.
The inverseproblem
ofinterpretation
of the director fieldstarting
from thelight
pattern necessitates a detailed account of the symmetries which arepresent in the whole set-up : the
light
pattern, thelight
source and theboundary
conditions.This gives a
powerful
method and the symmetry of the director field has been identified.Moreover,
we have given asatisfactory interpretation
of the pairing of the virtual cusps. Thisapproach
is rathergeneral
and may be valid also to caustics formed after reflections ondeformed surfaces.
However,
in most cases it has to besupplemented by
other methods inorder to grue a
fully
detaileddescription
of the deformations thatproduce
thelight
pattern.Inversely,
since a caustic carnes more information, itmight
bemisleading
to restrict thestudy
to the image which is a mere section of it. Dur purpose is now to extend this
study
ta the more realistic 3-D case.Acknowledgments.
This work was
supported by
the Direction des Recherches et EtudesTechniques
under thecontract DRET/ERS/901616.
N° 7 CAUSTICS, SYMMETRIES AND FLOW VISUALIZATION 1025
Appendix.
Here,
thegeneral
formalism of thetheory
ofsingularities [22, 9]
is used to write theequations
of the fold andcusp-points.
We start from theequation
for the rays :4~
(x,
z, Àf
x xo
(À
+(z
à) tan a(À
=
0
(10)
given in section 5. This
equation
defines a 2-D surface M in the 3-D spaceix,
z, A).
The surface M isglobally parametrized by
z and A, equation(10) giving
the coordinate,r as afunction of
z and :
x(z,
A=
xo(A
+(d
z tan a(A
). The causticpoints correspond
to thesingularities
of theprojection
wfrom M onto thephysical
2-D spaceix,
=),
that is to say to the points where the Jacobian matrix w * of gris not of maximum rank(here 2).
Moreprecisely,
thefold-points
are definedby
the condition : corankw*(z, )
=1, where the corank (at thesource)
of w * is defined as the difference between the dimension of M and its rank. The matrixw * reads
~
jéx/éz
é>./ôAjé,r/éz
éx/éA ~~ ~~"
éz/éz éz/éA 0
so that the condition for the corank of w * to be
equal
to 1, is written é,;/éA=
0,
and we recoverformula
(6).
It defines the curvelS'
of thefold-points.
In order to find the cusp-points, we repeat the same reasomng, the
only
differencebeing
that M isreplaced
hereby 3'.
Thecurve
3'
is
parametrized by
A, and the restriction of gr to3~
lSWI
~i1 À-
(X(Z(À)j, Z(À )).
The condition
giving
the cusp-points is that the corank of the Jacobian matrix(w [~,)*
should be
equal
to 1, or in orderwords,
that its rank should beequal
to 0. On the other hand we have~~
jéx/éz.
dz/dA + éx/éA dzjôx/ôzj
~~~~~ ~~ dz/dÀ dÀ
(using
the fact that ôx/ôA=
0 on
lS').
Then the equation that gives the set lS~. ' of the cusp- points is dz/dA=
0,
and we recover formula(8).
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