1 lecture 9 a whirlwind sketch of the derivation of the 1d layer-averaged equations of turbidity...
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LECTURE 9A WHIRLWIND SKETCH OF THE DERIVATION OF THE
1D LAYER-AVERAGED EQUATIONS OF TURBIDITY CURRENT FLOW DYNAMICS
The details of the derivation can be found in Parker et al. (1986).
In the earlier part of the derivation, index notation is used to reduce clutter in the analysis.
Position and instantaneous velocity vectors:
In the same way:gi = vector of gravitational accelerationvsi = vector of fall velocity of particle in still waterA this point in the analysis, the orientation of the coordinate system need not be specified. Some other parameters are:p = instantaneous pressurec = instantaneous suspended sediment concentration
i 1 2 3 i 1 2 3x (x ,x ,x ) (x,y,z) , u (u ,u ,u ) (u,v,w)
CEE 598, GEOL 593TURBIDITY CURRENTS: MORPHODYNAMICS AND DEPOSITS
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GOVERNING EQUATIONS OF THE INSTANTANEOUS FLOW
The governing equations of the instantaneous flow are:The Navier-Stokes equations for momentum balance of the flow:
the continuity equation for conservation of flow water mass:
and the equation of conservation of suspended sediment mass:
where usi denotes the velocity vector of a sediment particle, and as before
sii
cu c 0
t x
2i i i
f j f f ij i j j
u u upu g
t x x x x
i
i
u0
x
f a(1 Rc)
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GOVERNING EQUATIONS OF THE INSTANTANEOUS FLOW contd.
The Navier-Stokes equations for momentum balance can be rewritten as
where v,ij denotes the viscous stress tensor, given as
In addition, it is assumed here that the instantaneous sediment particle velocity usi is equal to the sum of the fluid velocity and the fall velocity:
so that the equation of balance of suspended sediment becomes
i sii i
c cuc v 0
t x x
v,iji if j f f i
j i j
u u pu g
t x x x
jiv,ij f
j i
uu
x x
si i siu u v
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THE AMBIENT WATER ABOVE THE CURRENT
x
zu
cq
turbid water
ambient water
The ambient water above the turbidity current is assumed to be in hydrostatic balance with density a, so that the Navier-Stokes equation reduces to
where pa denotes the ambient pressure.
aa i
i
p0 g
x
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THE BOUSSINESQ APPROXIMATION
The turbidity current can induce some deviatoric pressure pd that varies about the ambient hydrostatic value:
Now using the above relation and the relation of the previous slide to reduce the Navier-Stokes equation of two slides before, it is found that since f - a = aRc,
The heart of the Boussinesq approximation is that the effect of the density difference between the bottom underflow and the ambient water (in this care created by the presence of sediment and so = Rc) is neglected in the acceleration terms (where Rc is small compared to 1) but kept in the gravity term (where it is all that is available to drive the flow):
a dp p p
v,ijdi ia j a i
j i j
pu u(1 Rc) u Rcg
t x x x
v,ijdi ia j a i
j i j
pu u(1 Rc) u Rcg
t x x x
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THE REDUCED INSTANTANEOUS EQUATIONS
v,ijdi ij i
j a i a j
pu u 1 1u Rcg
t x x x
where
j ji iv,ij a a
j i j i
u uu u(1 Rc)
x x x x
and
i
i
u0
x
i sii i
c cuc v 0
t x x
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MEAN AND FLUCTUATING QUANTITIES FOR TURBULENT FLOW
Turbidity currents need not be turbulent. (“Turbid” comes from a Latin root meaning “muddy”.) For example, laminar turbidity currents carrying mud can travel long distances before the mud settles out. In the absence of turbulence, however, any sediment that settles cannot be re-entrained into the flow. This means that most interesting cases involve turbulent flow.
In the case of turbulent flow, the instantaneous parameters ui, c and p fluctuate about mean values. Here the mean values are denoted with an overbar, and the fluctuating values are denoted with a prime superscript:
i i iu u u , p p p , c c c
Some rules of averaging are stated below1. The average of the sum = the sum of the average.2. A quantity that is already averaged cannot be averaged more.3. Differentiation and averaging commute.4. The average of the produce does not = the product of the average.Thus if A and B are instantaneous parameters, e.g.
A A(A B) A B , (AB) AB , , AB AB A B AB
t t
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where R,ij denotes the Reynolds stress due to turbulence, and FR,i denotes the Reynolds flux of suspended sediment:
These terms quantify the tendency of turbulence to mix momentum and sediment mass, respectively, at rates that far exceed molecular processes. With this in mind, the viscous stress term in the momentum equation is neglected in subsequent slides.
R,ij a i j R,i iuu , F c u
v,ij R,ijdi ij i
j a i a j
pu u 1 1u Rcg
t x x x
i
i
ii si
i i
u0
x
Fcu v c
t x x
REYNOLDS-AVERAGED BALANCE EQUATIONS
Averaging the balance equations over turbulence results in the forms
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2D FLOW OVER A BED
x
zu
cq
turbid water
ambient water
We now use the geometry assumed earlier in the lecture. That is, x is a boundary-attached streamwise coordinate, z is a boundary-attached upward-normal coordinate, q S <<1, gi and vsi are approximated as
where vs is the scalar particle fall velocity (positive for vertical downward). In addition, the flow is assumed to be uniform in the y direction, with
i si s sg (gS, 0, g) , v (v S,0, v )
iu (u,0,w)
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GOVERNING EQUATIONS FOR 2D FLOW
u w0
x z
R,xx R,xzd
a a
pu u u 1 1u w RcgS
t x z x x z
R,xz R,zzd
a a
pw w w 1 1u w Rcg
t x z z x z
x zs s
F Fcu v S c w v c
t x z x z
where
R,xx a R,xz a R,zz au u , u w , w w
R,x R,zF c u , F c w
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SLENDER FLOW (BOUNDARY LAYER) APPROXIMATIONS
For most cases of interest it can be assumed that , so that the equation of balance of suspended sediment mass reduces to
x zs
F Fcuc w v c
t x z x z
sv S / u 1
According to the slender flow approximation, the characteristic distance Lc over which the flow changes in the streamwise (x) direction is taken to be large compared to the characteristic distance c (estimate of boundary layer thickness) over which flow changes in the upward normal (z) direction, so that
In addition, it is assumed that a characteristic time for the flow to change Tc is at least as large as Lc/Uc, where Uc is a characteristic velocity of the flow.
c
c
1L
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BALANCE EQUATIONS APPROXIMATED FOR SLENDER FLOW
The details of the application of the slender flow approximations are not shown here. They can be found in most books on turbulent flow. The reduced forms are
d
a a
pu u u 1 1u w RcgS
t x z x z
d
a
p10 Rcg
z
s
c Fuc w v c
t x z z
u w0
x z
where and F are now shorthand for R,xz and FR,z, respectively.
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THE DEVIATORIC PRESSURE TERM
d
a
p10 Rcg
z
Note that the upward normal momentum equation has reduced to a hydrostatic balance between the deviatoric pressure and the excess gravitational force due to sediment in the flow:
Now high above the flow, the pressure distribution is ambient, so that
d zp 0
Integrating the first equation using the second equation as a boundary condition, it is found that
d zp Rg cdz
The streamwise momentum equation thus reduces to
za
u u u 1u w Rg cdz RcgS
t x z x z
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LAYER INTEGRATION
The streamwise momentum equation can be further rewritten with the aid of continuity,
to the form:
This equation is now integrated from z = 0 to z = (i.e. far above the current, where the ambient water is in hydrostatic balance) under the boundary conditions
to yield
where b is the bed shear stress, given as
u w0
x z
2
za
u u uw 1Rg cdz RcgS
t x z x z
z z z 0u w 0
2b0 0 0 z 0
a
1udz u dz Rg cdz dz RgS cdz
t x x
b z 0
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LAYER INTEGRATION contd.
The equation of continuity
integrates under the boundary conditions of the previous slide and the further condition
to yield:
Note that the upward normal velocity is not taken to be zero at z = . This is a consequence of the boundary layer approximations. More specifically, we represents an entrainment velocity at which ambient flow is sucked into the flow across the interface. In the case of a steady flow, it acts to increase the forward flow discharge per unit width of the flow in the downstream direction.
u w0
x z
z 0u 0
e e z0udz w , w w
x
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LAYER INTEGRATION contd.The equation of balance of suspended sediment integrates with the aid of the previously-stated boundary conditions and the further boundary condition
to:
where
Note that Fb denotes the upward normal flux of suspended sediment at the bed, or in other words the entrainment rate of sediment from the bed. Defining a dimensionless entrainment rate Es such that
the balance equation for suspended sediment reduces to
b s b0 0cdz ucdz F v c
t x
zF 0
b bz 0 z 0F F , c c
b s sF v E
s s b0 0cdz ucdz v E c
t x
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THE TOP HAT APPROXIMATIONWe now drop the overbars in the equations, it now being understood that the quantities in question have been averaged over turbulence:
2b0 0 0 z 0
a
1udz u dz Rg cdz dz RgS cdz
t x x
e e z0udz w , w w
x
s s b0 0cdz ucdz v E c
t x
For a first look at the form of the equations, we evaluate the integrals using the top hat approximations:
clear water
u
c
U
CH
z
U , 0 z Hu
0 , z H
C , 0 z H
c0 , z H
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Performing the integrations with the top hat approximations and adding the closure relations
the resulting forms are found to be:
Relations for ew, ro and Es were presented earlier in the lecture.
EQUATIONS IN “SHALLOW WATER” FORM
2 22
f
UH U H 1 CHRg C U RgSCH
t x 2 x
w
H UHe U
t x
s s o
CH UCHv E r C
t x
2b a f b o e w
HC U , c r C , w e U
t
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REDUCTION TO “BACKWATER FORMS” FOR STEADY FLOW DEVELOPING IN THE STREAMWISE DIRECTION
2 22
f
w
s s o
UH U H 1 CHRg RgCHS C U
t x 2 xH UH
e Ut xCH UCH
v (E r C)t x
s sew f o
s
s sew f o
s
s s se so se
s s o
v q1 1S e (2 ) C r 1
2 2 U qdH
dx 1
v q1 1S e (1 ) C r 1
2 2 U qH dU
U dx 1
dq v q E HUHr 1 q
q dx U q r
Ri Ri Ri
Ri
Ri Ri Ri
Ri
For the case of steady flow, the equations to the right reduce to the forms below:
where:
2d2
s
sse
o
RgCH
Uq CUH
E UHq
r
Ri Fr
Note that qs is the volume transport rate per unit width of suspended sediment.
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CORRESPONDING “BACKWATER FORMS” FOR A RIVER
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f
s s o
UH U H 1 Hg gHS C U
t x 2 xH UH
0t xCH UCH
v (E r C)t x
For the case of steady flow, the equations to the right reduce to the forms below:
2f
2
w
s ses o
s s
S CdH
dx 1UH q const
dq qHv r 1
q dx q
Fr
Fr
where qs and qse retain their meanings from the previous slide, qw denotes the (constant) water discharge per unit width, and
3
2w
22
gH
q
gH
UFr
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CASE OF A CONSERVATIVE UNDERFLOW DRIVEN BY E.G. SALINE OR TEMPERATURE-MEDIATED BUOYANCY
EFFECTS
For a steady flow, they further reduce to the forms on the left. Note that the volume discharge qe of the fractional density excess per unit width is constant, hence the terminology “conservative”. The bulk Richardson number is now
222e
e f
w
e e
F HUH U H 1g gF HS C U
t x 2 xH UH
e Ut xHF UHF
0t x
This case is obtained in the limit as vs 0. Here RC Fe, where Fe now denotes the layer-averaged fractional buoyancy excess of the bottom flow induced by salt or cold temperature. The equations reduce to the forms to the right.
w f
w f
e e
1S e (2 ) CdH 2
dx 11
S e (1 ) CH dU 2U dx 1q F UH const
Ri Ri
Ri
Ri Ri
Ri
e e2 3
F gH gq
U U Ri
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“NORMAL” FLOW FOR A RIVER
Consider the case of flow over a constant slope S. We further assume that the bed friction coefficient Cf is constant. In the case of a river, the equations reduce to:
2 222f w
w2 3
S C qdH U, UH q const ,
dx 1 gH gH
Fr
FrFr
The equations admit a solution for a “normal” velocity Un and a “normal” depth Hn that are both constants. The governing equations for this solution are
1/ 322 f w w
f n nn
C q qS C 0 H , U
gS H
Fr
Using e.g. the Garcia-Parker sediment entrainment relation, the “normal” concentration Cn of suspended sediment is then given as
f n 0.6unun p
s
C U(Z ), Z
v Res
no
EC =
r
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“NORMAL” FLOW FOR CONSERVATIVE DENSITY UNDERFLOW
We again consider the case of a constant bed slope S and bed friction coefficient Cf. In the case of a conservative density underflow, the equation for U two slides back has a constant “normal” solution Un. This can be obtained by setting the numerator of the equation for dU/dx to 0, so that
where the subscript “n” denotes the “normal values”. Using, for example the relation below for ewn
the first equation can be solved iteratively for a constant normal Richardson number Rin. Once the (constant) transport rate per unit width of density excess qe = UHFe is specified, the normal flow velocity Un can be computed from the relation
n wn n f
1S e (1 ) C 0
2 Ri Ri
wn 2.4n
0.075e
1 718
Ri
en 3
n
gq
URi
w f
1S e (1 ) CH dU 2
U dx 1
Ri Ri
Ri
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SAMPLE SOLUTIONS FOR NORMAL FLOW OF A CONSERVATIVE DENSE UNDERFLOW
Cf 0.05
qe 0.2 m2/s
Solve by trial and error
S Rin Frdn ewn Un Flow class Rootm/s
0.2 0.314 1.78458 0.01111 1.842 supercritical -6E-050.1 0.570 1.32453 0.00548 1.510 supercritical -4E-05
0.05 1.080 0.96225 0.00255 1.220 subcritical 7.2E-050.01 5.140 0.44108 0.00039 0.725 subcritical -1E-06
0.005 10.210 0.31296 0.00017 0.577 subcritical -2E-06
n wn n f
1S e (1 ) C 0
2 Ri Ri wn 2.4
n
0.075e
1 718
Rie
n 3n
gq
URi
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“NORMAL” FLOW FOR CONSERVATIVE DENSITY UNDERFLOW contd.
The equation for dH/dx, i.e.
reduces with the relation for normal Richardson number
and the condition of constant qe = UHFe to give
Thus for the normal solution, current thickness increases linearly (as it entrains ambient water), and fractional excess density decreases hyperbolically (as the ambient water dilutes the salt or heat deficiency inthe current).
n wn n f
1S e (1 ) C 0
2 Ri Ri
w n u wn
ee n e e
n u en
dHe ( ) const H H e x
dxq
F U H q FU H e x
Ri
w f
1S e (2 ) CdH 2
dx 1
Ri Ri
Ri
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NO “NORMAL” FLOW SOLUTION EXISTS FOR A TURBIDITY CURRENT THAT FREELY EXCHANGES SEDIMENT WITH THE
BEDIf there were a corresponding “normal” solution for a turbidity current, it would take the form
where Un and qsn are constants However, if Un is given constant, then Es is also a constant Esn, where
would also be constant. The equation for conservation of suspended sediment for a steady would then take the form
n s sn w n u wn
se
n u en
dHU U , q q , e ( ) const H H e x
dxq
CRU H e x
Ri
f n 0.6un un p
s
C U(Z ) , Z
v Resn sE =E
s sns sn o
n u wn
dq qdUCHv E r const
dx dx U (H e x)
so that qs could not be constan after all. That is, dilution of the flow dueto the entrainment of ambient water acts to push the flow out of equilibrium.
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If we had some data, we might be able to determine some approximate similarity forms for u and c:
Applying the constraints
it follows that fu and fc must be such that
For example, the top hat assumptions
satisfy these constraints.
CAN WE DO BETTER THAN THE TOPHAT APPROXIMATION?
u c
u c zf ( ) f ( )
U C H
2 2
0 0 0UH udz , UCH ucdz , U H u dz
2u u u c0 0 0f ( )d 1 , f ( )d 1 , f ( )f ( )d 1
1,0
1,1)(f)(f cu
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EXAMPLE BASED ON EXPERIMENTAL DATAThe data and functions are from Parker et al. (1987). They can’t be said to be universal for any turbidity current, but they can help get a picture of the sructure of turbidity currents.
’ ’
fu fc
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SHAPE FACTORS
2b0 0 0 z 0
a
1udz u dz Rg cdz dz RgS cdz
t x x
Consider the previously-introduced layer-integrated forms:
e e z0udz w , w w
x
s s b0 0cdz ucdz v E c
t x
Now substituting the similarity forms,
and using previously-introduced closure forms for b, we and cb, we find the relations on the next slide.
u cu Uf ( ) , c Cf ( ) , dz Hd
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SHAPE FACTORS contd.
where 1, and 2 are order-one shape factors given by the relations
The data of Parker et al. (1987) suggest values of 1 and 2 close to 0.99 and 1.00, respectively.
Parker et al. (1986) called the above three conservation equations the “three-equation model”.
2 22
1 2 f
w
2 s s o
UH U H 1 CHg RCgHS C U
t x 2 xH UH
e Ut x
CH UCHv (E r C)
t x
The integral forms now reduce to
1 c 2 c0 02 f ( )d , f ( )d
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DENSITY STRATIFICATION EFFECTS
In a turbidity current, the flow higher up can be expected to have a lower concentration, and thus a lower density, than the flow lower down. Such a flow is called stably stratified. As turbulence mixes in the vertical in a stably straified flow, it must lift heavy water up and light water down. The extra work required to do this acts to damp the turbulence
z
c
z2
z1
c2
c1
2 1
f 2 a 2 f1 a 1
c c
(1 Rc ) (1 Rc )
Parker et al. (1986) developed a fairly simple layer-integrated model that accounts for density stratification. It is called the four-equation model. The additional equation governs the conservation of the kinetic energy of the turbulence.
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KINETIC ENERGY OF THE TURBULENCE
In addition to U, H and C, the four-equation model introduces a fourth variable, i.e. the layer-averaged kinetic energy of the turbulence per unit fluid mass. That is,
The balance equation for turbulent kinetic energy takes the form
where the shear velocity u is given as
The term o denotes the rate of dissipation of the energy of the turbulence per unit mass due to viscosity.
2 2 2
0
1UHK ukdz , k u v w
2
2 3w o s w s s o
KH UKH 1 1 1u U U e H Rgv CH RgCHUe RgHv (E r C)
t x 2 2 2
b
a
u
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PHYSICAL MEANING OF THE TERMS IN THE BALANCE EQUATION FOR THE KINETIC ENERGY OF THE
TURBULENCE
2 3w o s w s s o
KH UKH 1 1 1u U U e H Rgv CH RgCHUe RgHv (E r C)
t x 2 2 2
a) b) c) d) e) f) g) h)
a) time rate of change of layer-integrated turbulent kinetic energy (TKE)b) streamwise variation in the discharge per unit width of TKEc) rate of production of TKE associated with bed sheard) rate of production of TKE associated with the interfacee) rate of dissipation of TKE due to viscosityf) rate at which TKE is consumed in holding the sediment in suspensiong) rate at which TKE is consumed in lifting the suspended sediment as water
entrainment thickens the currenth) rate at which TKE is lost (gained) as new sediment is entrained upward from
(deposited downward onto) the bedTerms f), g) and (in a flow that entrains sediment in the net) h) act to damp
turbulence due to the presence of sediment.
A full derivation of the equation for K is given in Parker et al. (1987). The terms are interpreted below.
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In the four-equation model, the boundary shear stress is related to K rather than U:.
Here the coefficient is estimated as 0.1. Note that this means the sediment entrainment rate Es now also depends on K rather than U:
so that if K is damped then Es is throttled as well.
The parameter o is given as
where cD is an “equivalent” friction coefficient.
CLOSURE ASSUMPTIONS IN THE FOUR-EQUATION MODEL
2b a au K
Dw D3 / 2
0 3 / 2
D
c1e 1 2 c
K 2,
H c
Ri
0.6un un p
s
K(Z ) , Z
v
Resn sE =E
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THE FULL FOUR-EQUATION MODEL
The governing equations are
2 3w o s w s s o
KH UKH 1 1 1u U U e H Rgv CH RgCHUe RgHv (E r C)
t x 2 2 2
2 2
w
s s o
UH U H 1 CHRg RgCHS K
t x 2 xH UH
e Ut xCH UCH
v (E r C)t x
where ew is a specified function of Ri as before, Es is a function of K as outlined in the previous slide, and the form for o is specified in the previous slide.
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2 3 3 2w w s w s s 0
1 1 1u U e U e UK K RgH C v e U v E r C
2 2 2dK
dx UH
s sew o2
s
s sew o2
s
s s se so se
s s o
v q1 K 1S e 2 r 1
2 U 2 U qdH
dx 1
v q1 K 1S e 1 r 1
2 U 2 U qdU U
dx 1 H
dq v q E UHHr 1 , q
q dx U q r
Ri Ri Ri
Ri
Ri Ri Ri
Ri
“BACKWATER FORMS” FOR STEADY FLOW DEVELOPING IN THE STREAMWISE DIRECTION: THE CASE OF THE FOUR-
EQUATION MODEL
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REFERENCES
Garcia, M, and G. Parker, 1991, Entrainment of bed sediment into suspension. Journal of Hydraulic Engineering, 117(4), 414‑435.
Parker, G., 1982, Conditions for the ignition of catastrophically erosive turbidity currents. Marine Geology, 46, pp. 307‑327, 1982.
Parker, G., Y. Fukushima, and H. M. Pantin, 1986, Self‑accelerating turbidity currents. Journal of Fluid Mechanics, 171, 45‑181.
Parker, G., M. H. Garcia, Y. Fukushima, and W. Yu, 1987, Experiments on turbidity currents over an erodible bed., Journal of Hydraulic Research, 25(1), 123‑147.