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Session B.pdf - Clarkson University

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heat exchange simulation on the boundary of the water surface with the atmosphere taking<br />

into account the possibility of ice formation and melting. At that this task has to be<br />

solved namely at unsteady setting taking into account the dynamics of weather factors<br />

changing: air temperature, wind velocity and direction, air humidity, precipitation intensity,<br />

cloudiness and so on. Unsteadiness imposes strict demands on the efficiency of the<br />

used numerical method especially if the task is solved in three-dimensional (3D) setting.<br />

There is a number of different approaches to solve the task with the majority of which<br />

are based on one-dimensional [1] or plane (2D) [2-4] setting.<br />

2D and 3D algorithms given in this work are made up on the method of the finite volume<br />

that allows to create numerical diagrams conservative by mass and pulse [5-7]. For<br />

the tasks connected with unsteady heat transmission the conservatism of the numerical<br />

diagram is an obligatory condition.<br />

Plane (2D) Model of Hydro-Dynamics and Heat Transmission<br />

The divergent form of the 2-D system of the shallow water equations for viscous liquid and<br />

for heat transmission in Cartesian coordinate system (x,y) is the following [8]:<br />

where the vector of variables, fluxes and sources is written as<br />

∂Q<br />

∂E<br />

∂G<br />

+ + = S , (1)<br />

∂t<br />

∂x<br />

∂y<br />

⎡h<br />

⎤ ⎡hu<br />

⎤ ⎡hv<br />

⎢ ⎢ 2 2 ⎥ ⎢<br />

hu<br />

⎥<br />

⎢ ⎥<br />

2<br />

; ⎢<br />

hu + gh<br />

huv<br />

Q = E =<br />

⎥ ; G = ⎢<br />

2 2<br />

⎢hv<br />

⎥ ⎢huv<br />

⎥ ⎢hu<br />

+ gh 2<br />

⎢ ⎥ ⎢<br />

⎥ ⎢<br />

⎣hT<br />

⎦ ⎣huT<br />

+ hγ T<br />

∂T<br />

∂x⎦<br />

⎣hvT<br />

+ hγ T<br />

∂T<br />

⎡ Φ<br />

⎤<br />

⎢<br />

2<br />

⎢<br />

ghS0x<br />

− S<br />

fx<br />

+ hfv + τ<br />

x<br />

ρ + hγ∇<br />

u<br />

S =<br />

.<br />

⎢<br />

2<br />

ghS0<br />

y<br />

− S<br />

fy<br />

− hfu + τ<br />

y<br />

ρ + hγ∇<br />

v<br />

⎢<br />

⎢⎣<br />

ρc<br />

( ) ⎥ ⎥⎥⎥⎥ ΘΦ<br />

+ Θbot<br />

+ ΘS<br />

⎦<br />

⎤<br />

⎥<br />

⎥<br />

⎥<br />

⎥<br />

∂y⎦<br />

Here: g – free fall acceleration; h – water depth; u and v – components of the vector U<br />

averaged by the velocity depth in Cartesian coordinate system; S – components of<br />

S0 x,<br />

0 y<br />

−4<br />

the bottom slope; f = 1,458 × 10 sin( ϕ)<br />

– Coriolis parameter, ϕ – geographical latitude;<br />

τ<br />

x<br />

, τ<br />

y<br />

– components of the wind tangential stress on the free surface; ρ – water<br />

2<br />

density, c – its specific heat; ∇ – Laplace operator; Φ – mass source; T – water temperature<br />

average by depth; γ<br />

T<br />

– coefficient of temperature conductivity in the horizontal<br />

direction including turbulent and disperse components. The components of the friction<br />

force vector on the bottom can be determined by Manning formulae:<br />

S<br />

2<br />

2 2<br />

gn<br />

= C<br />

f<br />

( h) hu U ; S<br />

fy<br />

= C<br />

f<br />

( h) hv U ; U = u + v ; C<br />

f<br />

( h) . (2)<br />

4 3<br />

h<br />

fx<br />

=<br />

If there is ice cover the roughness coefficient n is calculated by the formula [9]:<br />

;<br />

160

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