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Geometrical Analysis of Avalanches in a 2D Drum
Florence Cantelaube, Yann Limon-Duparcmeur, Daniel Bideau, G.H. Ristow
To cite this version:
Florence Cantelaube, Yann Limon-Duparcmeur, Daniel Bideau, G.H. Ristow. Geometrical Analy- sis of Avalanches in a 2D Drum. Journal de Physique I, EDP Sciences, 1995, 5 (5), pp.581-596.
�10.1051/jp1:1995107�. �jpa-00247084�
Classification Physics Abstracts
46.10 05.40 64.60C
Geometrical Analysis of Avalanches in
a2D Drum
Florence Cantelaube
(~),
YannLimon-Duparcmeur (1),
Daniel Bideau(1)
andG-H Ristow (~)
(~) Groupe Matière Condensée et Matériaux
(*),
Université de Rennes I,Campus
de Beaulieu,35042 Rennes Cedex, France
(~) Fachbereich Physik, Philipps Universitàt Marburg, Renthof 6, 35032 Marburg, Germany
(Received
28 July 1994, revised 15 December 1994, accepted 2February1995)
fibstract.
We present an experimental and numerical analysis of intermittent flow at the surface of a 2-dimensional granular medium. Two types of devices are used: a 2-dimensional drum and a long rectangular box. Two types of grains are used(disks
andpentagons),
andcomparison is made between the dilferent cases. The experimental data are compared with the results obtained from molecular dynamics simulations, usmg roughly trie same number of
partiales. Dynamical conditions of stability are determined from the angle of repose 6r and trie angle of maximum stability 6m. Intermittent flow at the "surface" appears ta be of two types, as
in 3-dimension: small avalanches whose time fluctuations are characterised by
a power spectrum obeying a power law, and large events with well-defined average size and duration time.
l. Introduction
Granular media are not
only
one of the most often used mater1als in industrial processes but are alsomassively
present in our environment. Tueir flowproperties
have been [1] andare still now tue
subject
of many studies mpuysics,
mecuanics and soitmechanics,
civil and chemicalengineering.
Someexciting puenomena
areinvestigated,
sucu as the formation ofconvection
cells,
spontaneousheap
formation, surfacefluidization, avalanches, density
waves,or size
segregation [2,3].
For a review, see forexample
the paperby Jaeger
andNagel
[4].Avalanches have
recently
received a great attention, asbeing
aparadigm
for SelfOrganized Criticality (SOC
[SI. Asandpile
wouldby
itselfadjust
itsslope
to a criticalvalue, supposed
to be the
"angle
ofrepose"
@r, defined as theangle
between the horizontal and the free surface of thesandpile.
This selfadjustment
issuggested
to beanalog
toSOC,
and then characterizedby long-range spatial
andtemporal correlations,
with atypical 1If
power spectrum of thefluctuations. Some cellular automaton models have confirmed this
assumption [6-9]. Except
in small-size systems,
experimental
results[10-13]
are m contradiction with theprediction
of SOC model:peak
distributions of avalanche sizes on intervals areobserved,
insteadof1If
(*) URA CNRS N° 804
@
Les Editions de Physique 1995582 JOURNAL DE PHYSIQUE I N°5
noise. Tue essent1al reason of tuis
discrepancy
comes from tue fact tuat tuestability
of tuesandpile
cannot be describedby
aunique angle
of repose @r, butby
twoangles (and
ahysteresis
is
observed):
the maximumangle
ofstability
@m measuredjust
when an avalanche starts and theangle
of repose measuredjust
after the avalanche. The average dilference between these twoangles
@m @r is of the order of 2° for sand in 3D.Although
SOC is anexciting problem,
numerical andexperimentalstudies
of avalanches are interesting becausethey
areessent1ally
linked to two not well-understoodproblems concerning granular
materials: friction anddilatancy.
The
dilatancy
was first introducedby Reynolds
[14] and it is of greatimportance
in the deformation of densegranular
media: due to thegeometricalinterlocking
ofgrains,
a shear-ing
deformation cannot beimposed
to a non-cohesivegranular
mater1al withoutdilating
it.Starting
from thisanalysis,
a model forsandpile
avalanches has beenproposed,
which takesdilatancy
and frictionexplicitly
into account[11,15,16].
A macroscopic friction coefficient was introduced
by
Coulomb [17] asequalto
~t=
tan@r.
This mean value of friction does trot
explain
the two values of obtainedabove,
and their relation to the geometry of the system, theshape
of thegrain,
and themicroscopic
friction is not clear.Because of its
cyclic
character, arotating
drum allows forexperiments
withlong-time
ob- servations in processes characterizedby
short-time scales(e.g., avalanches),
and it has servedas a
good experimental
toolrecently [18,19].
This geometry is alsocurrently
used in industrial systems, such ascylindrical
ovens.In this paper we
explore experimentally
andnumerically
the rote of the friction coefficient and thepartiale shape
inequilibrium
of theheap,
and tue detail of the statistics of avalanches.We restrict ourselves to two
spatial
dimensions in order to be able to observe the geomet- rical modifications in the system. Someexperiments
havepreviously
beenperformed using
pentagons,
showing clearly
the main importance of face to face contacts,compared
to tuat of tue usualpunctual
contacts ofspueres
or disks [20]. Infact,
in tue case of pentagons, tue number ofpossible
stableconfigurations
islarger,
and somelarge
dilferences areexpected
in tue definition of tue surfaceequilibrium
of apile,
from botu the statics anddynarnics.
Wuile it is
perfect
forgeometrical properties,
tuis2-dimensionalexperimental
and numerical system posesproblems
m tue context of SOC: the 2D version of tue modelproposed by Bak, Tang
and Wiesenfeld(BTW)
[Si for avalanches is not critical atail,
unlike some otuer cellularautomaton models [21]. A numencal simulation
by
moleculardynamics
of a 2Dsandpile
does notgive
clear resultsconcerning
tuis cntical cuaracter [22].Tuis paper is divided into turee parts: in tue first part, we present our
experimental
set-up and numericaltechniques.
Tue second part is devoted to tuedynamicalequilibrium
conditions of apile,
and tue tuird part gives ourexperimental
and numerical results on statistics ofavalanches.
2.
Description
of OurSystem
2.1. EXPERIMENTAL SET-UP. Tue watts of the drum are two
parallel glass
disks with adiameter of 60 cm. The width between these two disks is
(1+ e)
mm(e
«1)
and we have usedparticles (disks
orpentagons)
which are 1 mm thick. Thus theoverlap
ofpartiales
isimpossible,
and our system isactually
2-dimensional. The ensemble is driver in rotationby
amotor and a v-belt. Avalanches are studied
by filling
half of the drum with 1400 pentagonswith a side
length
of 6 mm, or with 1400 disks with a diameter of 8 mm. Thepacking
fraction(surface
of thegrain
over totalsurface)
of thepile
is found to beequal
to o.77 + o.03, a valueOE~«-UloewoE~-UloeoE~-UloeoE~
-oeOE«Ulw~moe-oeoEUlwmoeooeoE ---oeoeoe number of pentagons
Fig. 1. Distribution of the mass of avalanches observed in the drum for pentagons.
comparable
to that obtained on densepackings
of pentagons [20]. Fordisks,
thispacking
fraction is 0.82 + o.02.
As stated
above,
the surface of thepacking
within the drum is characterizedby
twoangles:
tue
angle
of repose @r and tue maximumangle
ofstability
@m. Tue dilferenceA@(=
@m @r)between tue two is
generally
of a fewdegrees.
For small systems, tuere is a criticallengtu
1,defined as the
length
from which onegrain
is seenby
anangle
A@. If the size of the system is smaller than 1,hysteresis
cannot beobserved,
and the nature of avalanches ischanged:
forexample,
some power law for the avalanche size distribution is observed [12]. In our case, thislength
1is 3 cm, which is smallcompared
to tue diarneter of tue drum.Tue rotation speed (uJ) is about o.25 rpm, wuicu is
sufficiently
slow to ensure tuat tue statistics of avalanches isspeed-independent.
A video film of tue drum in rotation isanalyzed by
animage processing
program(visilog 4.1.3)
on a work station. Fromtuat,
we obtain the statistics of tueweigut,
duration andseparation
time ofavalanches,
and we are able to measure theangle
at tuebeginning
and at tue end of an avalanche. Tue results obtained on pentagonsby
tuis metuod arecompared
to tue results tuat we havepreviously
obtained ondisks,
andby
numerical simulations.
For eacu avalanche event, we record grey scale
images rigut
before andrigut
after tue avalanche anddigitize
tuem using tueimage processing
prograrn. Tuesepictures
are bina- rized witu a thresuold in order to represent pentagonsby
values of1 and thebackground by
o.On the
picture
taken after anavalanche,
weimpose
anegative
rotationby #
= uJtd, where id is the duration of tuisavalanche,
to correct tue drum rotation in our calculation of the mass of the avalanche. If one tilts tue voles m the picturesby
ageometrical
operation(dilation)
andtuen subtracts
tuem,
theresulting
picture shows tue surface of tueavalanche,
wuicu we will coltweigut.
In order to separate
large
events from small events, we have carried out two types ofanalysis
of these statistics. Asimple
observation of ourexperiments,
or of avalanches at tue surface of an mclined box filledby sand, clearly
shows that these two dilferent types of avalanchescoexist:
they
will be described later.Figure gives
the mass distribution of avalanches. It is important to note tuat in tuisfigure,
tueprobability
to observe verybig
avalanches is cut off due to finite size elfects in the drum which prevent the system fromreaching
ashigu
a valueas m the static case. For the
analysis
oflarge
events, we suppress events with a surface smaller584 JOURNAL DE PHYSIQUE I N°5
o
@ C
©
2ce
OE
, o
~ o
O
~ ~ ~
@ ~
£l
E io0
o ~ o
° cxpcnmcnul
~ C
~ .
~cantcd
o
0
0 5 10 15 20 25 30
deltatheta
Fig. 2. Experimental
(0)
and tueoretical(-)
relationships between the angle dilference and the avalanche mass, expressed in number of grains.tuan 25 pentagons.
In order to
study
tuespatial
distribution of avalanches moreprecisely,
we bave built anexperimental
device very similar to tuat used in Drake'sexperiment
[23]. It is a 2-dimensionalbox, consisting
of tworectangular glass planes,
200 cmlong
and 30 cmuigh.
Tue widtubetween tue two
planes
is about 1.2 mm. Tue inclinationangle
of tuis box witu respect to tue horizontal cari be controlledby
a system ofpulleys.
As in thedrum,
we tilt tuis cell witu styrene disks witu a diameter of 8 mm, or witu pentagons whosesidelengtu
is 6 mm. It is necessary to use 2400particles
to obtainsize-independent results,
witu apile
about terparticles uigu.
Actually
tuere are never more tuan rivelayers
ofgrains
whicu fait when an avalanche settles.Thus tue surface on whicu the
partiales
flow isreally
constituted of otuer mobileparticles
likem the drum.
2.2. EXPERIMENTAL VALIDATION.
Using
pentagons allows us to have anamorphous
systemwithout
crystalline
zones, which con induce some non trivial correlations in collective rotations.Crystalline
structuresclearly modify
the conditions of the static anddynamic equilibrium.
We have also studiedamorphous
systems ofequal
disks in thedrum,
and in the 2Dbox, by gluing
a
rough layer
of disks of dilferent sizes at the externatwatt,
orby mixing particles
of dilferent sizes.Figure
2 shows the avalanche mass versus A@, the dilference of theangle
before and alteran avalanche. The
points
have been obtainedby
the imageprocessing
program where we took tue rotation of the drumdunng
tue avalanche into account. Thestraight
fine is the theoreticalcurve calculated via the relation
~
~
Î
~~where L is the
length
of thepile,
C thepacking fraction,
andSp
the surface of one pentagon.It is obtained
directly by writing
the surfaceoccupied by
pentagons in an arch of radiusL/2
and of
angle
@.The
experimental points
are the result ofaveraging
the masses obtained in each interval of onedegree. Except
for small events(which
are,by
nature, dilferent irom thelarge
events descnbedby
thisformula),
a reasonable agreement is obtained(the
fluctuations observed areessent1ally experimental),
and we conclude that theexperimental weight
isroughly proportional
to the
angle
dilference of thelarge
avalanches.2.3. NUMERICAL MODEL. In
1979,
Cundall and Strackproposed
a model to describe the forcesacting
at themicroscopic
level ongrains
in anassembly
ofspheres
whichthey
called the distinct element method [24]. Since then this method has been extended andslightly
modified todescribe,
among otherthings,
the mechanicalsorting
ofgrains
[25], the shear-inducedphase
boundaries
[26],
theorigin
of convection cells[27-29],
and the outflow from ahopper [30-32].
For the sake of
simplicity,
we will considerspherical particles,
but if one includes a static friction mechanism(thereby neglecting
the rotation of the individualsphere),
we can wellreproduce
theexperimental
results obtained with pentagons, which we will discuss below.Whenever two
partiales
are doser thon the sum of theirradii,
1-e-, whenthey
have beendeformed, they
interact via normal and shear forces. The force onpartiale1,
causedby partiale j
isgiven by:
F~j
=Fnii
+Fsé (1)
Fn
=-kn(r~
+ rj(ri rj)ii)" ~inme~(f~ fj)11 (2)
Fs
=-sign(ôs) min(ks jôsj,/J jfnj) (3)
where
m~mj
~~~
mi + mj
and
ôs =
Î
(é~éj )é
dlHere ri denotes tue
position
vector of tue i~~partiale,
ù is tue unit vectorpointing
from thepartiale
toj
and § is a unit vectorperpendicular
to iirotating
clockwise. Tue constant kn stands for tue"Young modulus",
ks for tuespring
constant in the suear direction to mimic static friction[32],
and ôs for tue total sheardisplacement during
the contact of the twopartiales.
me~ is the effective mass. Tue shear force Fs bas two
regimes
where tue transition isgiven by
the friction coefficient ~t due to the Coulomb
Fs
critenon. For a= 1, we are left with Hooke's law and for a =
3/2,
weinvestigate
the Hertzian contact force forslightly
deformable disks.Our units are chosen in such a way that the average
partiale
diameter is unity with a massof
unity.
Thepseudo "Young
modulus"kn
isequal
to 10~N/m~/~,
and we used a time step of Ai = 2 x 10~~ s which assured numericalstability.
The
relationship
between ourdamping
parameter ~in and theexperimentally
morecommonly
used restitution coefficient e con be derivedexactly
for a = 1 from equations(1)
and(2)
and is of tue formIn(e)
'/n C~
~
For a = 1.5, one
gets
a very weakvelocity dependence
but the aboveequation
can still be usedover a wide range. Tuis has been verified for our model
by
one of us [30].To avoid tue ordered
triangular lattice,
we use a distribution ofpartiale
sizes wuere tue size of tuebiggest particle
is four times tue size of tue smallestpartiale.
The drum is ualf filled withpartiales
and containsrouguly
1450 of tuem. We bave tested our simulation for dilferent rotationspeeds
and have found the threeexperimentally
well-knownregimes
of distinctavalanches,
continuous flow andcentrifugated regime
[18]. The rotationspeed
has been chosenas uJ = 0.25 rpm in order to be in the distinct avalanche
regime
which is thatexperimentally
used,
as discussed in thepreceding
section.586 JOURNAL DE PHYSIQUE I N°5
0.2 0.2
P(8M)
(a)P(8R)
(b)0.ifi 0.ifi
0.12 0.12
0.08 0.08
0.04 0.04
0 0
30 40 60 60 30 40 60 60
BM
8R
Fig. 3. Probability distribution of the maximum angle of stability 6m
(a)
and of the angle of repose 6r(b)
of an avalanche. These distributions are obtained experimentally with pentagons.As it has been
argued
in Section 2.2, the mass of an avalanche isproportional
to theangle
dilference A@
= @m-@r. Since the latter is measured more
easily
in oursimulations,
we will now describe theprocedure.
At each iteration, therotating
drum is divided into 100 verticalstrips
and the position of the
highest partiale
in each strip is searched. From these 100partiales,
we obtain theangle
of the surfaceby
aleast-squares
fit. Theangle
isaveraged
over 1000 iterations and we check our automatedalgorithm by comparing
the results with a visual manual fit fordilferent times.
3.
Dynamic Equilibrium
of trie Pile andGeometry
We have seen that in the intermittent
regime (avalanches),
aheap
of sand is cuaracterizedby
two
angles:
tue maximumangle
ofstability
@m and tueangle
of repose @r. Tueseangles
arenon-trivial functions of tue coefficient of friction between
grains,
tue geometry of tue systemat tue individual scale
(shape
of tue grains, etc. and at tueglobal
scale.3.1. EXPERIMENTAL ANALYSIS. Each
experimental angle
is determined as trie result ofan
averaging
process(least-squares metuod)
over tue drumdiameter,
in order to smooth theroughness
of the surface.Experimentally,
it is clear that there is a more or less broad dis- tribution of the measuredangle
of repose @r and of the maximumangle
ofstability
@m. The distributions for pentagons obtainedby measuring
260 avalanches aregiven
mFigure
3: themean value of
@r is 37° and that of @m is 45°.
Experimentally
too, foramorphous (1.e.,
with disk sizedistribution) packings
ofdisks,
we have obtained @r= 24° and @m
= 33°. Two reasons
con
explam
this dilference:first,
because of face-to-face contacts, each pentagon is more stable thon thecorresponding
disk. But there are also strong correlations in the relative rotations of pentagons [33], and tuebeginning
of an avalanche and its motion are more difficult in thiscase: a
pile
of pentagons is more stable tuan apile
of disks.As suown in
Figure
4, tueexperimental angle
dilference A@, wuicu measures tue range of avalanchesizes,
is very wide: it ranges fromnearly
zero tonearly
20degrees,
witu a mean value of 9°. One notes tuat tueangles
between 2 and 14degrees
are almostequally probable.
o.io
P(A8)
0.08
o-où
0.04
0.02
0
0 10 20
A8
Fig. 4. Probability distribution
P(A6)
of the dilference A6 between the starting and stopping angleof an avalanche, obtained experimentally with pentagons.
Tuis
large
range is due to tue facttuat,
for pentagons, tuepossibility
to find anequilibrium (individual
orcollective)
is greatercompared
to tuat for disks3.2. NUMERICAL APPROACH. It is difficult to make a
quantitative expenmental analysis
of tue influence of tue friction coefficient betweengrains
on theangles
@r and @m. In return,using
our numericalsimulations,
since the introducedspring
constant ks is ratuerartific1al,
we may obtain a reasonable value of tue
angles defining
tueequilibrium
of theheap
fromsome test runs. We fill the drum
halfway
withpartiales
of dilferent diameters(which
is theway of
introducing
disorder in the numencalsimulations)
and start to rotate it. After some thousands ofiterations,
we stop the drum rotation and watt for the system to relax: we control the relaxationby monitoring
the kinetic energy. We measure the obtainedangle
of repose @r for dilferent values of k~ and of tue Coulomb turesuold ~t. Tue results arepresented
inFigure
5, in whicu the continuous litrecorresponds
to the Coulomb relation @r=
tan~~
~t [32].A linear
relationship
is obtained for @r as a function of ks for small values of p. Forlarger
values of ~t, a saturation elfect is observed. In order to obtain
equilibrium
conditions in nu- merica1 simulations and inexperiments
on pentagons, we haveadjusted
our simulationsby choosing
~t= o-G for a value of ks
= 1000 N.m~~
Doing this,
we obtain à numerica1value of@m near the
expenmental
one.Figure
6 shows the distribution ofangles
obtainednumerically
for
non-rotating
disksaveraged
over 112 avalanches: we obtain @m= 45° and @r
= 40°.
Therefore one has to
keep
in mind that, in spite of an apparentquantitative
agreement, there are stronggeometrical
dilferences between tue two systems(disks
andpentagons),
asdiscussed above: tue numerical value of @r is dilferent from tue
experimental
one. Here too tueexperimental packings
of pentagonscomparatively
olfer alarger
number ofequilibrium
states than in
numericalsystems
ofdisks,
even with a strong friction: tuisexplains
tuat tue distributions ofangles
arelarger
forexperimental
pentagons(see Fig. 3)
than for numerical disks. These distributions are trotsymmetrical,
and we believe that this is due for alarge
partto limite size elfects
(see below).
4. Avalanches
4.1. DEFINITIONS. An avalanche is here defined as the motion of at least one
particle
down tue inclined surface.
Starting
from tuisdefinition,
we mustdistinguisu
between two590 JOURNAL DE PHYSIQUE I N°5
(a) (b)
20000 ioooo
p J~
ioooo ioooo
0 0
0 20 40 fi0 80 100 0 20 40 60
t Îs) t (s)
a) b)
Fig. 8.
(a)
Fluctuations m pixel of two successive pictures obtained experimentally in the 2D drum filled with pentagons. Measurements are taken every 1° of rotation;(b)
same result obtainednumerically. Measurements are taken every o.15° of rotation.
Tuis initiates a collective
back-avalanche,
wuicu is aglobal
loss ofequilibrium involving
ailpartiales
of tuepile leading
to a total reconstruction of tuesurface,
wuicu isfinally
inclined from tue horizontalby
@r.Small events
only
involve one or fewgrains
m metastableequilibrium
on the surface of tuepile.
Tuis loss ofequilibrium
isindividual,
and is of the type observed if oneplaces
onegrain
on arougu
inclined surface builtby gluing glass spueres
on it [36,37].
Wuen it loses itsequilibrium,
tuegrain
fallsdown,
andduring
itsmotion,
it bas some collisions witu otuergrains,
and stops or may create a collective motion.
Orly
a weak andgenerally
local modification in tue surfacemorpuology
is observedalong
alengtu
1,being
tue freepatu
of tuis event,generally
smaller tuan tue
lengtu
of tue free "surface". Tue occurrence of tuese eventsdepends
on tuemorpuology
of thepile surface,
on the inclinationangle
and on its fluctuations.In the
following
part, we will descnbe tue statistics of tuese two dilferent events.4.2. SMALL EVENTS
4.2.1.
Experimental A~ialysis.
Bretz et ai. [34] bave suown tuat tue surface of asandpile
issubject
to small fluctuations wuen oneslowly
increases theangle
of repose. Tuese small eventsoccur between
large
avalanches: this is what we observe in bothexperiments
in the 2D drumand in a 2D inclined chute.
They
evolve less than 30particules (disks
orpentagons).
Figure
8a illustrates the relative importance of each type of events, and howthey
are time- distributed: itgives
the mass fluctuation at tue surface of tue 2Dpile
ofpentagons
m tue drum.To obtain this
(small)
massvariation,
weanalyse
the pictures, butonly
between identifiedlarge
events. We
plot
the dilference inpixels
between two successivepictures
taken with an interval of timeequal
to 0.67 simposed by
the resolution of theimage processing
program andexactly
the sonne
procedure
as descnbed in Section 2.1 isapplied
to measure the fluctuation ofweight.
The area obtained
by
tue subtraction of the two pictures results from thereorganization
of theÎ t~
= z
~ n
m
~ n
fl o
u
20 40 60 80 100 120 140 160 180 200 20 40 60 80 100 120 140 160 180 200
a)
startIng position (cm)b)
~~~~~'~~ P°~'~'°~ l~~lFig. 9. Probability for
a disk to be the seed of a small event at distance L from the top of the pile,
in the inchned chute:
(a)
pentagons;(b)
disks.heap
surfaceduring
tue rotation of1°(rotàtion angle
of tue drumduring
tue interval of time of 0.67s).
Weapply
tue sameprocedure
at eacu rotationby
onedegree
until the nextlarge
event. The statistics obtained are the sum of these
analyses.
Even if the
experimental
spectrum obtained from the square of theamplitude
of these mass fluctuations could be fittedby
astraight
litre with aslope
of the orderof1.5,
the statisticsare not sufficient to be affirmative
jbout
any power law behaviour. The numerica1simulationscan
explore
the fluctuations of thepile
surfaceduring
an interval of time reduced to 0.1 s.Tuus we suall use tuese numerical simulations to describe a better
analysis
of tuese small mass fluctuations in tuefollowing
section.According
to results obtained on tue inclinedplane [36, 37],
it is reasonable to expect auomogeneous
distribution of tuestarting positions along
tue line for tuese small events: onecon believe tuat at tue surface of a
packing,
tueprobability
to findpartiales
in metastableequilibrium
is tue sameeverywuere
on tue surface.We
plotted
onuistograms presented
inFigures
9a and 9b tueprobability
for a small eventto occur at a distance L from the top for pentagons
(a)
and disks(b),
obtained in the indinedchute. This
probability
is not constantalong
thesurface,
neither fordisks,
nor forpentagons.
On the contrary, we observe that the
probability
of thestarting position
decreasesnearly linearly
with L. This evolution is smoother for disks thon for pentagons. Nevertheless small events are intercalated betweenlarge
events, wuich lead to acomplete reorganization
of the tue surface. After the reconstruction of thepile,
the successive small events willdestroy
the metastable states below itsstarting
position up to its captureby
the bulk: the surface isprogressively
washed. Tuisexplains
trie results suownFigure
9.4.2.2. Numencal
Analysis.
In tue case of numerical studies of small events, we map every o.1 s ourgrain configuration
to a soc x 500binary grid
wuere a 1 in tue cell indicated thatmore tuan 501~ of the cell area is covered
by
apartiale.
Two successive grids are subtracted from another and the dilference is measured in cells. This dilference is our measurement for the small surface fluctuations.A
typical
time trace of our numerical system is shown inFigure
10. In part(a)
we show theangle
of the surfaceaveraged
over looo iterations(which
has been obtainedby dividing
thedrum in loo vertical
regions, looking
for the coordinate of thehighest partiale
andmaking
aleast-squares fit).
In part(b)
we show the total kinetic energy of thepartides.
One sees how eacupeak
in the energycorresponds
to a drasticchange
in tue surfaceangle corresponding
to aiouxNAL DB pHYsioçB i T.s,w s,MAy 199s n
592 JOURNAL DE PHYSIQUE I N°5
2000
e 1',1
Il
,ji
'
jçoo
~~
.,~
~(
~Î. Ji'
~
~~ 1,~
,
' J 1200
v
j
Si t 'j
) ' soc
~~ 400
, ,
~
6o go 100 120
j~ ,~ fi0 80 100 120 2° 4°
1trie (si tinte (si
a) b)
Fig. 10.
(a)
Surface angle fluctuation obtained numerically;(b)
corresponding total kinetic energy fluctuations.cuaracteristic avalanche. Also notable are tue small fluctuations
(small events)
in botugrapus (anotuer
source for fluctuations are tue statistical errors of our measurementtechnique).
From these numerical results, we con draw
Figure
8b. The noise(at
afrequency roughly equal
to làHz)
observed in thisfigure,
thenconcerning
numericalsimulations,
isessentially
due to the numerical method. Between
large
events, we observe a succession of very small events(one
has tokeep
in mind that thelarge
event distribution is cut offby
the finite size ofour
system).
As before we
plotted
the power spectrum of the square of theamplitude
of the mass fluc- tuations. The dataonly ranged
over one order ofmagnitude
with an error ofroughly
o-à- The numericalresults,
shown inFigure
ii are fittedby
astraight
line with aslope of1.8,
notalfected
by
the "numerica1noise" which appears atfrequency
15 Hz.4.2.3. Conclusion. These numerical and
experimental results,
whichgive
tue power laws for tuese small events, arequalitatively
similar to tuose obtained in 3 dimensions[12, 34]. However,
because of the small size of our systems, no definitive conclusion cari be drawn.
4.3. LARGE EVENTS.
Large
events involve trie wholepile.
As it is aglobal
process, which is trot modifiedby
small events, theprobability P(L)
to observe an avalanchestarting
at adistance L from the top of the
pile
isexpected
to be constant.P(L),
determmed in our inclinedchute,
isgiven
inFigure
12a for pentagons and inFigure
12b for disks.Except
for small orlarge
values ofL, P(L)
isroughly
constant in both cases. Near thebottom,
the slide of arow of
partiales
is blockedby
the wall and near the top, the pressure on agrain
is screenednear the wall: this
explains why P(L)
is smaller at the two ends of the distribution. These two screeninglengths
are a littlelarger
for pentagons than fordisks,
as thestability
of thesegrains
islarger. They
are of about 40particle
diameters.Accordingly,
finite size effects areexpected
to besignificant
in our experiments in a drum: for disks in adrum,
thehistogram
iscomparable
to that ofFigure
12a.Figure
13 shows thatP(Ù)
is not a constant of the starting position for pentagons in the drum: tue firstpartiale
wuicu flows down tuepile
is locatedmostly
at tue top of tue surface.Thjs dilference in
P(L')
between disks and pentagons con be correlated to tuegeometrical
le-05
~p
ie-06
ie-llî
le-os
Ie-09
le-10
o-1 10 10']
f[H2]
Fig. Il. Power spectrum relative to surface fluctuations obtained numerically.
£~ ~
é ~
W £
n @
o n
ÉO
20 40 60 80 100 120 140160 180 200 20 40 60 80 100120 140 160180 200
startIng position (cm) startIng position (cm)
a) b)
Fig. 12.
P(L),
probability for an avalanche to start at a distance L from the bottom of the pile mtue box, uprsus L:
(a)
pentagons;(b)
disks.configuration
of tue top of tuepile just
before tue avalanche(see Fig. 14):
fordisks,
tue surface of tuepile
in tue drum isregular (Fig. 14a),
wuereas for pentagons, tuesuape
is very dilferent near trie top(Fig. 14b). Figure
14a shows tueconfiguration
of tue top of tue surface for a mixture of small andlarge disks;
but tuere is nochange
in tuispile geometry
wuen builtonly
witularge partiales.
Because tueslope
is steeper in tuis part, tue top of tue pentagonpile
becomes very instable wuen becomes of tue order of @m. Therefore tue avalanches startpreferentially
at tue top.Figure
15a shows the distribution of tue duration time of an avalanche andFigure 15b,
tueseparation
time between two running avalanches. Theuistograrn
of the duration looksquite
suarp, and tue mean duration time is 2.7 seconds. Tueseparation
distribution is broader thon tue duration one and gives a mean separation time of 8-9 seconds.594 JOURNAL DE PHYSIQUE I N°5
ce + W W O ce + W w O ce + W w
ce ce ce ce ce
Starting length (cm)
Fig. 13. Probability for an avalanche to start at a distance L' from the top of trie pile in the drum, for pentagons.
i
b) a)
Fig. 14. Photographs
showmg
the geometry of the surface of the pile m trie drum:(a)
disks;(b)
pentagons.5. Conclusion
While made m
relatively
small systems, ourstudy
in 2 dimensions has confirmed the bimodal character of avalanches at the surface of apile:
small events, wuose size ditribution is describedby
a powerlaw,
and cuaracteristic(large)
events wuose size and time duration arewell-averaged.
Tuese results are
qualitatively
tue same wuetuer oneuses
disks,
orpentagons
in expenments.Tue numerical simulations are
essentially
used as acomplementary
tool tostudy
in more detail tue influence of somepuysical
parameters wuich cannot be reachedexperimentally (friction,
energy, etc. ).
0.4
~~~~ l~) Plt) jb)
0.3 0.12
0.2 0.08
o-1 0.04
0 0
0 2 4 fi 0 4 8 12
t [s] t [s]
Fig. 15.
(a)
Distribution of avalanche duration;(b)
distribution of time separation between two successive avalanches, obtained experimentally with pentagons.Beyond
tuese results, we bave outlined tue strong influence of tuepartiale shape
and friction coefficient on tueangle
of repose or of maximumstability. Finally,
because of tue extremesensitivity
of tue avalanche to tue local andglobal equilibrium,
we bave suown thatgeometrical
limite size elfects are important in these systems.
Acknowledgments
This work has benefited from useful discussions with J-P-
Troadec,
A. Hansen and S. Roux. It has beenpartly supported by
the GdR CNRS"Physique
des MilieuxHétérogènes Complexes".
References
[1] Faraday M., Phil. Trans. Roy. Soc. London 52
(1831)
299.[2] Bideau D. and Hansen A., Disorder and Granular Media
(North
Holland,1993).
[3] Mehta A., Granular Matter
(Spnnger,
1994).[4] Jaeger H-M- and Nagel S-R-, Science 255
(1992)
1523.[Si Bak P., Tang C. and Wiesenfeld K., Phys. Reu. Lent. 59
(1987)
381.[6] Tang C. and Bak P., Phys. Reu. Lent. 60
(1988)
2347.[7] Dhar D., Phys. Reu. Lent. 62
(1989)
1813.[8] Gutfram R., Private Communication.
[9] Puhl H., Physica A 197
(1993)
14.[10] Jaeger H-M-, Liu Ch. and Nagel S-R-, Phys. Reu. Lent. 62
(1989)
40.[Il]
Evesque P., Phys. Reu. A 43(1991)
270.[12] Held G-A-, Solina D.A. Il, Keane D.T., Haag W-J-, Horn P-M- and Grinstein G., Phys. Reu. Lent.
65
(1990)
l120.[13] Rosendahl J., Vekic M. and Kelley J., Phys. Reu. E 47
(1993)
1401.596 JOURNAL DE PHYSIQUE I N°5
[14] Reynolds O., Phd. Mag. 20 (1885) 469.
[15] Evesque P., Fargeix D., Habib P., Luong M.P. and Porion P., Phys. Reu. E 47
(1993)
2326.[16] Porion P., Thèse, Université des Sciences et Technologie de Lille
(1994).
[17] de Coulomb C.A., "Mémoires de Mathématiques et de Physique présentés à l'Académie Royale des Sciences" 7
(1773)
343.[18] Rajchenbach J., Phys. Reu. Lent. 65
(1990)
2221.[19] Caponeri M., Douady S., Fauve S. and Laroche C., prepnnt.
[20] Ammi M., Bideau D. and Troadec J-P-, J. Phys. D 20
(1987)
424.[21] Kadanolf L.P., Nagel S-R-, Wu L., Zhou S., Phys. Reu. A 39
(1989]
6524.[22] Lee J., J. Phys. I France 3
(1993)
2017.[23] Drake T.G., J. Geophys. Res. 95
(1990)
8681.[24] Cundall P. and Strack O.D.L., Geotechniq. 29
(1979)
47.[25] Half P.'K. and Werner B-T-, Powder Technol. 48
(1986)
239.[26] Thompson P-A- and Grest G-S-, Phys. Reu. Lent. 67
(1991)
1751.[27] Ristow G-H-, J. Phys. I France 2
(1992)
649.[28] Taguchi Y.H., Phys. Reu. Lent. 69
(1992)
1367.[29] Gallas J-A-C-, Herrmann H-J- and Sokolowski S., Phys. Reu. Lent. 69
(1992)
1371.[30] Ristow G-H-, Int. J. Mod. Phys. C 3
(1992)1281.
[31] Ristow G-H- and Herrmann H-J-, Phys. Reu. E, in press.
[32] Lee J. and Herrmann H.J., J. Phys. A 26
(1993)
373.[33] Limon-Duparcmeur Y., pnvate communication.
[34] Bretz M., Cunningham J-B-, Kurczynski P-L- and Non F., Phys. Reu. Lent. 69
(1992)
2431.[35] Carlson J-M-, J. Geophys. Res. 96
(1991)
4255.[36] Riguidel F-X-, Jullien R., Ristow G-H-, Hansen A. and Bideau D., J. Phys. I France 4
(1994)
261.[37] Riguidel F-X-, Hansen A. and Bideau D., Europhys. Lent., submitted.