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A Semi-Implicit, Three-Dimensional Model for Estuarine ... - USGS

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Appendix A - Coriolis Acceleration 163<br />

where the advective acceleration (u • ∇)u is introduced by the Eulerian specification of the flow. Equation A.9 states that the<br />

equation of motion in the rotating frame is equivalent to that in an absolute frame so long as it is assumed that a pseudo body <strong>for</strong>ce<br />

per unit mass represented by (–2Ω × u) 54 acts upon the fluid. This pseudo body <strong>for</strong>ce is known as the Coriolis acceleration<br />

(<strong>for</strong>ce/unit mass) and is often significant in estuarine modeling.<br />

In Cartesian coordinates using u = ui + vj + wk and Ω = Ω x i + Ω y j + Ω z k, the acceleration terms are<br />

-----<br />

∂u<br />

u<br />

∂t<br />

∂u<br />

----- v<br />

∂x<br />

∂u<br />

----- w<br />

∂y<br />

∂u<br />

+ + + ----- – 2Ω<br />

∂z zv + 2Ωyw , (A.10)<br />

∂v<br />

----- u<br />

∂t<br />

∂v<br />

----- v<br />

∂x<br />

∂v<br />

----- w<br />

∂y<br />

∂v<br />

+ + + ----- + 2Ω<br />

∂z zu – 2Ωxw , and (A.11)<br />

∂w<br />

------ u<br />

∂t<br />

∂w<br />

------ v<br />

∂x<br />

∂w<br />

------ w<br />

∂y<br />

∂w<br />

+ + + ------ + 2Ω<br />

∂z xv – 2Ωyu .<br />

(A.12)<br />

For a reference frame chosen using the z-axis vertically-upward, but using the horizontal axes rotated by an angle θ, the components<br />

of Ω are dependent on both the latitude φ and the rotation θ by<br />

Ωx = Ω cosφsinθ,<br />

Ωy = Ω cosφcosθ<br />

, and (A.13)<br />

Ωz = Ω sinφ.<br />

When the x-axis is toward the east and the y-axis is toward the north (θ = 0°), these reduce to<br />

Ω x<br />

= 0 ,<br />

Ωy = Ω cosφ,<br />

and (A.14)<br />

Ωz = Ω sinφ<br />

.<br />

In a shallow estuary, the vertical velocity component w is typically very small, and there<strong>for</strong>e the two Coriolis terms involving w in<br />

the horizontal momentum equations (A.10 and A.11) are usually neglected. Frequently the term (Ω xv – Ω yu) in the z-momentum<br />

equation is also neglected because it is considered to be small in comparison with g. Pond and Pickard (1986, p. 40) point out,<br />

however, that, although (Ω xv – Ω yu) may be small compared with g, it may not always be small compared with the difference<br />

between the pressure term in the z-momentum equation and g. Evces and Raney (1990) <strong>for</strong>mulated a 2-D vertically-averaged<br />

hydrodynamic model that included the z-component Coriolis term and estimated it may correct the total Coriolis term <strong>for</strong> a high<br />

tidal range estuary near latitude φ = 45° by10 percent. The correction will be most pronounced at high latitudes (φ > 45°) and in<br />

some instances may warrant inclusion in a model applied at lower latitudes. For the model discussed herein, however, the term is<br />

neglected, as is customary. In this case, the <strong>for</strong>m of the acceleration terms in the rotating reference frame are most commonly<br />

expressed as<br />

∂u<br />

----- u<br />

∂t<br />

∂u<br />

----- v<br />

∂x<br />

∂u<br />

----- w<br />

∂y<br />

∂u<br />

+ + + ----- – fv<br />

(A.15)<br />

∂z<br />

54 Using the subscript notation from Chapter 2 of this report, the Coriolis acceleration 2Ω × u is written as 2εijkΩ ju k.

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