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1-D Saint Venant equation : ウィキペディア英語版
One-dimensional Saint-Venant equation
In fluid dynamics, the one-dimensional (1-D) Saint-Venant equation was derived by Adhémar Jean Claude Barré de Saint-Venant, and is commonly used to model transient open-channel flow and surface runoff. It is a simplification of the two-dimensional (2-D) shallow water equations, which are also known as the two-dimensional Saint-Venant equations. The 1-D simplification is used exclusively in models including HEC-RAS, SWMM5, (InfoWorks ), ISIS, Flood Modeller, MIKE 11, and MIKE SHE because it is significantly easier to solve than the full shallow water equations. Common applications of the 1-D Saint-Venant Equation include dam break analyses, storm pulses in an open channel, as well as storm runoff in overland flow.
==Derivation from Navier–Stokes equations==
The 1-D Saint-Venant equation can be derived from the Navier–Stokes equations that describe fluid motion. The ''x''-component of the Navier–Stokes equations – when expressed in Cartesian coordinates in the ''x''-direction – can be written as:
: \frac + u \frac + v \frac+ w \frac= -\frac \frac + \nu \left(\frac + \frac + \frac\right)+ f_x,
where ''u'' is the velocity in the ''x''-direction, ''v'' is the velocity in the ''y''-direction, ''w'' is the velocity in the ''z''-direction, ''t'' is time, ''p'' is the pressure, ρ is the density of water, ν is the kinematic viscosity, and ''f''x is the body force in the ''x''-direction.
+ \frac + \frac\right)= 0.
|-
| style="vertical-align:top;" | 2. || Assuming one-dimensional flow in the ''x''-direction it follows that:
:v\frac+ w \frac = 0
|-
| style="vertical-align:top;" | 3. || Assuming also that the pressure distribution is approximately hydrostatic it follows that:
: p = \rho g h
or in differential form:
:\partial p = \rho g \left(\partial h \right).
And when these assumptions are applied to the ''x''-component of the Navier–Stokes equations:
: -\frac \frac = -\frac\frac = -g \frac.
|-
| style="vertical-align:top;" | 4. || There are 2 body forces acting on the channel fluid, gravity, and friction:
: f_x =f_ + f_
where ''f''x,g is the body force due to gravity and ''f''x,f is the body force due to friction.
|-
| style="vertical-align:top;" | 5. || ''f''x,g can be calculated using basic physics and trigonometry:
:
F_ = (\sin\theta) gM

where ''F''g is the force of gravity in the ''x''-direction, θ is the angle, and ''M'' is the mass.
The expression for sin θ can be simplified using trigonometry as:
:
\sin\theta = \frac.

For small θ (reasonable for almost all streams) it can be assumed that:
:
\sin\theta = \tan\theta = \frac = S

and given that ''f''x represents a force per unit mass, the expression becomes:
:
f_ = gS.

|-
| style="vertical-align:top;" | 6. || Assuming the energy grade line is not the same as the channel slope, and for a reach of consistent slope there is a consistent friction loss, it follows that:
:
f_ = S_f g.

|-
| style="vertical-align:top;" | 7. || All of these assumptions combined arrives at the 1-dimensional Saint-Venant equation in the ''x''-direction:
:\frac + u \frac + g \frac + g (S - S_f) = 0
:(a)\quad \ \ (b)\quad \ \ \ (c) \qquad (d) \ \ \ (e)
where (a) is the local acceleration term, (b) is the convective acceleration term, (c) is the pressure gradient term, (d) is the gravity term, and (e) is the friction term.〔Saint-Venant, A. (1871), ''Theorie du mouvement non permanent des eaux, avec application aux crues des rivieres et a l’introduction de marees dans leurs lits''. Comptes rendus des seances de l’Academie des Sciences.〕
|}

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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