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Physical Modelling in Fluvial Geomorphology

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PHYSICAL MODELLING IN FLUVIAL GEOMORPHOLOGY 227<br />

In the case of the Froude number, s<strong>in</strong>ce acceleration due to gravity, g, rema<strong>in</strong>s constant for<br />

both model and prototype, then<br />

and therefore<br />

2<br />

U m Rm<br />

=<br />

2<br />

U R p p<br />

0.<br />

5<br />

m m<br />

u ( 8)<br />

⎟<br />

p p<br />

Equations (6) and (8) can only be resolved if Rm is equal to Rp. Thus, the flow Reynolds<br />

number is commonly relaxed, with the proviso that <strong>in</strong> the case of open channel flows it<br />

rema<strong>in</strong>s with<strong>in</strong> the fully turbulent flow regime (Re > 500). As noted previously, this form<br />

of modell<strong>in</strong>g is referred to as Froude scale modell<strong>in</strong>g (FSM).<br />

⎟<br />

U ⎛ ⎞<br />

⎜<br />

R<br />

λ = =<br />

U ⎜<br />

⎝<br />

R<br />

⎠<br />

Movable-bed modell<strong>in</strong>g (case with mobile sediment)<br />

If a movable rather than fixed bed is considered, the flow can be considered as a<br />

two-phase flow with both fluid and particles. The follow<strong>in</strong>g set of parameters is used to<br />

describe these flows: µ, ρ, S, R, g and two parameters which describe the sediment, ρs (the<br />

sediment density) and D (the characteristic gra<strong>in</strong> size of the sediment). Some of these<br />

variables can be replaced by other dependent parameters. For example, the shear velocity<br />

U* = (gRS) 0.5 can replace S and the immersed specific weight of gra<strong>in</strong>s <strong>in</strong> the fluid γs =<br />

g(ρs -ρ) can replace g giv<strong>in</strong>g µ, ρ, R, D, ρs, U* and γs, These variables also produce n - 3 or<br />

4Π terms<br />

The Π1and Π2 terms represent relative roughness of the sediment and relative density<br />

respectively, while the term Π3 is the gra<strong>in</strong> Reynolds number (Re*), which is a measure of<br />

the roughness of the bed relative to the thickness of the viscous sub-layer. Equation (12)<br />

expresses the Shields relationship which is normally rearranged as<br />

τ =<br />

*<br />

∏<br />

∏<br />

∏<br />

∏<br />

where τ is the bed shear stress responsible for <strong>in</strong>itiat<strong>in</strong>g sediment transport for a particular<br />

gra<strong>in</strong> size, D, and τ* is the dimensionless shear stress. Together, τ* and Re* form the axes<br />

of the Shields entra<strong>in</strong>ment diagram (Figure 9.2). The scatter of po<strong>in</strong>ts on the Shields<br />

1<br />

2<br />

3<br />

4<br />

R<br />

=<br />

D<br />

ρs<br />

=<br />

ρ<br />

ρU*<br />

D<br />

= = Re<br />

µ<br />

s<br />

2<br />

*<br />

ρU<br />

=<br />

γ D<br />

( ρ − ρ )<br />

s<br />

τ<br />

gD<br />

*<br />

( 7)<br />

( 9)<br />

( 10)<br />

( 11)<br />

( 12)<br />

( 13)

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