fluid_mechanics
284 Chapter 6 ■ Differential Analysis of Fluid Flow where f is called the velocity potential. Direct substitution of these expressions for the velocity components into Eqs. 6.59, 6.60, and 6.61 will verify that a velocity field defined by Eqs. 6.64 is indeed irrotational. In vector form, Eqs. 6.64 can be written as V f (6.65) Inviscid, incompressible, irrotational flow fields are governed by Laplace’s equation and are called potential flows. Streamlines 2 0 2 0 Vorticity contours so that for an irrotational flow the velocity is expressible as the gradient of a scalar function f. The velocity potential is a consequence of the irrotationality of the flow field, whereas the stream function is a consequence of conservation of mass (see Section 6.2.3). It is to be noted, however, that the velocity potential can be defined for a general three-dimensional flow, whereas the stream function is restricted to two-dimensional flows. For an incompressible fluid we know from conservation of mass that and therefore for incompressible, irrotational flow 1with V f2 it follows that where 2 1 2 1 2 is the Laplacian operator. In Cartesian coordinates (6.66) This differential equation arises in many different areas of engineering and physics and is called Laplace’s equation. Thus, inviscid, incompressible, irrotational flow fields are governed by Laplace’s equation. This type of flow is commonly called a potential flow. To complete the mathematical formulation of a given problem, boundary conditions have to be specified. These are usually velocities specified on the boundaries of the flow field of interest. It follows that if the potential function can be determined, then the velocity at all points in the flow field can be determined from Eq. 6.64, and the pressure at all points can be determined from the Bernoulli equation 1Eq. 6.632. Although the concept of the velocity potential is applicable to both steady and unsteady flow, we will confine our attention to steady flow. Potential flows, governed by Eqs. 6.64 and 6.66, are irrotational flows. That is, the vorticity is zero throughout. If vorticity is present (e.g., boundary layer, wake), then the flow cannot be described by Laplace’s equation. The figure in the margin illustrates a flow in which the vorticity is not zero in two regions—the separated region behind the bump and the boundary layer next to the solid surface. This is discussed in detail in Chapter 9. For some problems it will be convenient to use cylindrical coordinates, r, u, and z. In this coordinate system the gradient operator is so that where f f1r, u, z2. Since V 0 2 f 0 0 2 f 0x 2 02 f 0y 2 02 f 0z 2 0 1 2 01 2 0r ê r 1 r f 0f 0r ê r 1 r V v r ê r v u ê u v z ê z it follows for an irrotational flow 1with V f2 01 2 0u ê u 01 2 0z ê z 0f 0u ê u 0f 0z ê z (6.67) (6.68) (6.69) v r 0f 0r v u 1 0f r 0u v z 0f 0z (6.70) Also, Laplace’s equation in cylindrical coordinates is 1 r 0 0f ar 0r 0r b 1 02 f r 2 0u 02 f 2 0z 0 2 (6.71)
6.4 Inviscid Flow 285 E XAMPLE 6.4 Velocity Potential and Inviscid Flow Pressure GIVEN The two-dimensional flow of a nonviscous, incompressible fluid in the vicinity of the 90° corner of Fig. E6.4a is described by the stream function c 2r 2 sin 2u where c has units of m 2 s when r is in meters. Assume the fluid density is 10 3 kgm 3 and the x–y plane is horizontal— that is, there is no difference in elevation between points 112 and 122. FIND (a) Determine, if possible, the corresponding velocity potential. (b) If the pressure at point 112 on the wall is 30 kPa, what is the pressure at point 122? y y Streamline ( ψ = constant) 0.5 m (2) r Equipotential line ( φ = constant) θ (1) x 1 m (a) (b) x α α (c) F I G U R E E6.4 SOLUTION (a) The radial and tangential velocity components can be obtained from the stream function as 1see Eq. 6.422 and Since it follows that v r 1 0c 4r cos 2u r 0u v u 0c 4r sin 2u 0r v r 0f 0r 0f 4r cos 2u 0r and therefore by integration f 2r 2 cos 2u f 1 1u2 (1) where f 1 1u2 is an arbitrary function of u. Similarly v u 1 0f 4r sin 2u r 0u and integration yields f 2r 2 cos 2u f 2 1r2 (2) where f 2 1r2 is an arbitrary function of r. To satisfy both Eqs. 1 and 2, the velocity potential must have the form f 2r 2 cos 2u C (Ans) where C is an arbitrary constant. As is the case for stream functions, the specific value of C is not important, and it is customary to let C 0 so that the velocity potential for this corner flow is f 2r 2 cos 2u (Ans)
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284 Chapter 6 ■ Differential Analysis of Fluid Flow<br />
where f is called the velocity potential. Direct substitution of these expressions for the velocity<br />
components into Eqs. 6.59, 6.60, and 6.61 will verify that a velocity field defined by Eqs. 6.64 is<br />
indeed irrotational. In vector form, Eqs. 6.64 can be written as<br />
V f<br />
(6.65)<br />
Inviscid, incompressible,<br />
irrotational<br />
flow fields<br />
are governed by<br />
Laplace’s equation<br />
and are called<br />
potential flows.<br />
Streamlines<br />
2 0<br />
2 0<br />
Vorticity contours<br />
so that for an irrotational flow the velocity is expressible as the gradient of a scalar function f.<br />
The velocity potential is a consequence of the irrotationality of the flow field, whereas the<br />
stream function is a consequence of conservation of mass (see Section 6.2.3). It is to be noted,<br />
however, that the velocity potential can be defined for a general three-dimensional flow, whereas<br />
the stream function is restricted to two-dimensional flows.<br />
For an incompressible <strong>fluid</strong> we know from conservation of mass that<br />
and therefore for incompressible, irrotational flow 1with V f2 it follows that<br />
where 2 1 2 1 2 is the Laplacian operator. In Cartesian coordinates<br />
(6.66)<br />
This differential equation arises in many different areas of engineering and physics and is called<br />
Laplace’s equation. Thus, inviscid, incompressible, irrotational flow fields are governed by<br />
Laplace’s equation. This type of flow is commonly called a potential flow. To complete the<br />
mathematical formulation of a given problem, boundary conditions have to be specified. These are<br />
usually velocities specified on the boundaries of the flow field of interest. It follows that if<br />
the potential function can be determined, then the velocity at all points in the flow field can be<br />
determined from Eq. 6.64, and the pressure at all points can be determined from the Bernoulli<br />
equation 1Eq. 6.632. Although the concept of the velocity potential is applicable to both steady and<br />
unsteady flow, we will confine our attention to steady flow.<br />
Potential flows, governed by Eqs. 6.64 and 6.66, are irrotational flows. That is, the vorticity<br />
is zero throughout. If vorticity is present (e.g., boundary layer, wake), then the flow cannot be<br />
described by Laplace’s equation. The figure in the margin illustrates a flow in which the vorticity<br />
is not zero in two regions—the separated region behind the bump and the boundary layer next to<br />
the solid surface. This is discussed in detail in Chapter 9.<br />
For some problems it will be convenient to use cylindrical coordinates, r, u, and z. In this<br />
coordinate system the gradient operator is<br />
so that<br />
where f f1r, u, z2. Since<br />
V 0<br />
2 f 0<br />
0 2 f<br />
0x 2 02 f<br />
0y 2 02 f<br />
0z 2 0<br />
1 2 01 2<br />
0r ê r 1 r<br />
f 0f<br />
0r ê r 1 r<br />
V v r ê r v u ê u v z ê z<br />
it follows for an irrotational flow 1with V f2<br />
01 2<br />
0u ê u 01 2<br />
0z ê z<br />
0f<br />
0u ê u 0f<br />
0z ê z<br />
(6.67)<br />
(6.68)<br />
(6.69)<br />
v r 0f<br />
0r<br />
v u 1 0f<br />
r 0u<br />
v z 0f<br />
0z<br />
(6.70)<br />
Also, Laplace’s equation in cylindrical coordinates is<br />
1<br />
r<br />
0 0f<br />
ar<br />
0r 0r b 1 02 f<br />
r 2 0u 02 f<br />
2 0z 0 2<br />
(6.71)