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Chapter 8 IDEAL-FLUID FLOW

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Title: Chapter 8 IDEAL-FLUID FLOW


1
Chapter 8IDEAL-FLUID FLOW
2
  • In the preceding chapters most of the relations
    have been developed for one-dimensional flow,
    i.e., flow in which the average velocity at each
    cross section is used and variations across the
    section are neglected.
  • Many design problems in fluid flow, however,
    require more exact knowledge of velocity and
    pressure distributions, such as in flow over
    curved boundaries along an airplane wing, through
    the passages of a pump or compressor, or over the
    crest of a dam.
  • An understanding of two- and three-dimensional
    flow of a nonviscous, incompressible fluid
    provides the student with a much broader approach
    to many real fluid-flow situations. There are
    also analogies that permit the same methods to
    apply to flow through porous media.
  • In this chapter the principles of irrotational
    flow of an ideal fluid are developed and applied
    to elementary flow cases. After the flow
    requirements are established, Euler's equation is
    derived and the velocity potential is defined.

3
8.1 REQUIREMENTS FOR IDEAL-FLUID FLOW
  • The Prandtl hypothesis states that for fluids of
    low viscosity the effects of viscosity are
    appreciable only in a narrow region surrounding
    the fluid boundaries.
  • For incompressible flow situations in which the
    boundary layer remains thin, ideal-fluid results
    may be applied to flow of a real fluid to a
    satisfactory degree of approximation.
  •  An ideal fluid must satisfy the following
    requirements
  • 1. The continuity equation div q 0, or
  •                 
  • 2. Newton's second law of motion at every point
    at every instant
  • 3. Neither penetration of fluid into, nor gaps
    between, fluid and boundary at any solid 
    boundary

4
  • If, in addition to requirements 1, 2, and 3, the
    assumption of irrotational flow is made, the
    resulting fluid motion closely resembles
    real-fluid motion for fluids of low viscosity,
    outside boundary layers.
  • Using the above conditions, the application of
    Newton's second law to a fluid particle leads to
    the Euler equation, which, together with the
    assumption of irrotational flow, can be
    integrated to obtain the Bernoulli equation. The
    unknowns in a fluid-flow situation with given
    boundaries are velocity and pressure at every
    point.
  • Unfortunately, in most cases it is impossible to
    proceed directly to equations for velocity and
    pressure distribution from the boundary
    conditions.

5
8.2 EULER'S EQUATION OF MOTION
  • Euler's equation of motion along a streamline
    (one-dimensional) was developed in Sec. 3.5 by
    use of the momentum and continuity equations and
    Eq. (2.2.5).
  • In this section it is developed from Eq. (2.2.5)
    for the xyz-coordinate system in any orientation,
    with the assumption that gravity is the only body
    force acting. Since Euler's equation is based on
    a frictionless fluid, the vector equation (2.2.5)
  •               
  • (2.2.5)
  • may be reorganized into the proper form. The unit
    vector j' is directed vertically upward in the
    coordinate direction h.
  • These are the direction cosines of h with respect
    to the xyz system of coordinates, and they may be
    written

6
Figure 8.1 Arbitrary orientation of xyz
coordinate system
7
  • For example, ?h/?x is the change in h for unit
    change in x when y, z, and t are constant. In
    equation form,
  •               
  • The operation applied to the scalar h
    yields the gradient of h, as in Eq. (2.2.2).
  • Eq. (2.2.5) now becomes
  • (8.2.1)
  • The component equations of Eq.(8.2.1) are
  • (8.2.2)

8
  • u, v, w are velocity components in the x, y, z
    directions, respectively, at any point du/dt is
    the x component of acceleration of the fluid
    particle at (x, y, z).
  • Since u is a function of x, y, z, and t and x, y,
    and z are coordinates of the moving fluid
    particle, they become functions of t hence,
  •                 
  • However, dx/dt, dy/dt, and dz/dt are the velocity
    components of the particle, so that ax, the x
    component of the particle acceleration, is

9
  • By treating dv/dt and dw/dt in a similar manner,
    the Euler equations in three dimensions for a
    frictionless fluid are
  •                                    
  • (8.2.3)
  • (8.2.4)
  • (8.2.5)
  • The first three terms on the right-hand sides of
    the equations are convective-acceleration terms,
    depending upon changes of velocity with space.
  • The last term is local acceleration, depending
    upon velocity change with time at a point.

10
Natural Coordinates in Two-Dimensional Flow
  • Euler's equations in two dimensions are obtained
    from the general-component equations by setting w
    0 and ?/?z0 thus
  •                                            
  • (8.2.6)
  • (8.2.7)
  • By taking particular directions for the x and y
    axes, they can be reduced to a form that makes
    them easier to understand.
  • The velocity component u is vs, and the component
    v is vn. As vn is zero at the point, Eq. (8.2.6)
    becomes
  • (8.2.8)
  •                                              
  • Although vn is zero at the point (s, n), its
    rates of change with respect to s and t are not
    necessarily zero. Equation (8.2.7) becomes
  • (8.2.9)

11
Figure 8.2 Notation for natural coordinates
12
  • With r the radius of curvature of the streamline
    at s, from similar triangles (Fig. 8.2),
  •          
  •        
  • Substituting into Eq. (8.2.9) gives
  • (8.2.10)
  •                                                
  • For steady flow of an incompressible fluid Eqs.
    (8.2.6) and (8.2.10) can be written
  •          


  • (8.2.11)
  • and 
  • (8.2.12)
  •                                               
  • Equation (8.2.11) can be integrated with respect
    to s to produce Eq. (3.6.1), with the constant of
    integration varying with n, that is, from one
    streamline to another.
  • Equation (8.2.12) shows how pressure head varies
    across streamlines. With vs and r known functions
    of n, Eq. (8.2.12) can be integrated.

13
  • Example 8.1
  • A container of liquid is rotated with angular
    velocity ? about a vertical axis as a solid.
    Determine the variation of pressure in the
    liquid.
  • Solution
  • n is the radial distance, measured inwardly, dn
    -dr, and vs ?r . Integrating Eq. (8.2.12) gives
  •        
  • or             
  • To evaluate the constant, if p p0 when r 0
    and h 0,
  •                 
  • which shows that the pressure is hydrostatic
    along a vertical line and increases as the square
    of the radius.
  • Integration of Eq. (8.2.11) shows that the
    pressure is constant for a given h and vs, that
    is, along a streamline.

14
8.3 IRROTATIONAL FLOW VELOCITY POTENTIAL
  • In this section it is shown that the assumption
    of irrotational flow leads to the existence of a
    velocity potential. By use of these relations and
    the assumption of a conservative body force, the
    Euler equations can be integrated.
  • The individual particles of a frictionless
    incompressible fluid initially at rest cannot be
    caused to rotate. This can be visualized by
    considering a small free body of fluid in the
    shape of a sphere. Surface forces act normal to
    its surface, since the fluid is frictionless, and
    therefore act through the center of the sphere.
  • Similarly, the body force acts at the mass
    center. Hence, no torque can be exerted on the
    sphere, and it remains without rotation.
    Likewise, once an ideal fluid has rotation, there
    is no way of altering it, as no torque can be
    exerted on an elementary sphere of the fluid.

15
  • An analytical expression for fluid rotation of a
    particle about an axis parallel to the z axis is
    developed. The rotation component may be defined
    as the average angular velocity of two
    infinitesimal linear elements that are mutually
    perpendicular to each other and to the axis of
    rotation.
  • The two line elements may conveniently be taken
    as x and y in Fig. 8.3, although any other two
    perpendicular elements in the plane through the
    point would yield the same result. The particle
    is at P(x, y), and it has velocity components u,
    v in the xy plane. The angular velocities of dx
    and dy are sought.
  • The angular velocity of dx is
  • and the angular velocity of dy is
  •             
  •     
  • if counterclockwise is positive. Hence, by
    definition, the rotation component ?z of a fluid
    particle at (x,y) is
  • (8.3.1)

16
Figure 8.3 Rotation in a fluid
17
  • Similarly, the two other rotation components, ?x
    and ?y, about axes parallel to x and to y are
  • (8.3.2)
  •                                     
  • The rotation vector ? is
  •               
  •                                      (8.3.3)
  • The vorticity vector, curl q q, is
    defined as twice the rotation vector. It is given
    by 2?.
  • By assuming that the fluid has no rotation, i.e.,
    it is irrotational, curl q 0, or from Eqs.
    (8.3.1) and (8.3.2)
  • (8.3.4)
  • These restrictions on the velocity must hold at
    every point (except special singular points or
    lines).

18
  • The first equation is the irrotational condition
    for two dimensional flow. It is the condition
    that the differential expression
  •            
  •     
  • is exact, say
  • (8.3.5)
  • The minus sign is arbitrary it is a convention
    that causes the value of f to decrease in the
    direction of the velocity. By comparing terms in
    Eq. (8.3.5),
  • In vector form,
  •  (8.3.6)
  • is equivalent to
  • (8.3.7)

19
  • The assumption of a velocity potential is
    equivalent to the assumption of irrotational
    flow, as
  •            
  • (8.3.8)
  •                               
  • because . This is shown from Eq.
    (8.3.7) by cross-differentiation
  •                            
  • proving etc.
  • Substitution of Eqs. (8.3.7) into the continuity
    equation
  •                 
  • yields
  • (8.3.9)

20
  • In vector form this is
  •                                            
  • (8.3.10)
  • and is written
  • Equation (8.3.9) or (8.3.10) is the Laplace
    equation. Any function that satisfies the Laplace
    equation is a possible irrotational fluid-flow
    case. As there are an infinite number of
    solutions to the Laplace equation, each of which
    satisfies certain flow boundaries, the main
    problem is the selection of the proper function
    for the particular flow case.
  • Because appears to the first power in each term,
    Eq. (8.3.9), is a linear equation, and the sum of
    two solutions also is a solution e.g., if f1 and
    f2 are solutions of Eq. (8.3.9), then f1 f2 is
    a solution thus
  •                       
  • then  
  •          
  • Similarly, if f1 is a solution, Cf1 is a solution
    if C is constant.

21
8.4 INTEGRATION OF EULERS EQUATIONS BERNOULLI
EQUATION
  • Equation (8.2.3) can be rearranged so that every
    term contains a partial derivative with respect
    to x. From Eq. (8.3.4)
  •                 
  •            
  • and from Eg. (8.3.7)
  •                 
  • Making these substitution into Eq. (8.2.3) and
    rearranging give
  •                 
  • As the square of the speed,
  • (8.4.1)

22
  • Similarly, for the y and z direction,
  •        
  •                                            (8.4.2)
  • (8.4.3)
  • The quantities within the parentheses are the
    same in Eqs. (8.4.1) to (8.4.3). Equation (8.4.1)
    states that the quantity is not a function of x,
    since the derivative with respect to x is zero.
  • Similarly, the other equations show that the
    quantity is not a function of y or z. Therefore,
    it can be a function of t only, say F(t)
  •            
  •                       (8.4.4)
  •              
  • In steady flow ?f/?t0 and F(t) becomes a
    constant E
  • (8.4.5)
  •                                                   
           
  • The available energy is everywhere constant
    throughout the fluid. This is Bernoulli's
    equation for an irrotational fluid.

23
  • The pressure term can be separated into two
    parts, the hydrostatic pressure ps, and the
    dynamic pressure pd, so that ps pd. Inserting
    in Eq. (8.4.5) gives
  •                
  • The first two terms can be written
  •                 
  • with h measured vertically upward. The expression
    is a constant, since it expresses the hydrostatic
    law of variation of pressure. These two terms may
    be included in the constant E. After dropping the
    subscript on the dynamic pressure, there remains
  •         (8.4.6)
  •                                                   
        
  • This simple equation permits the variation in
    pressure to be determined if the speed is known
    or vice versa. Assuming both the speed q0 and the
    dynamic pressure p0 to be known at one point,
  • (8.4.7)

24
  • Example 8.2
  • A submarine moves through water at a speed of 10
    m/s. At a point A on the submarine 1.5 m above
    the nose, the velocity of the submarine relative
    to the water is 15 m/s. Determine the dynamic
    pressure difference between this point and the
    nose, and determine the difference in total
    pressure between the two points.
  • Solution
  • If the submarine is stationary and the water is
    moving past it, the velocity at the nose is zero
    and the velocity at A is 15 m/s. By selecting the
    dynamic pressure at infinity as zero, from Eq.
    (8.4.6)
  •              
  •    
  • For the nose
  •      
  •             
  •                    
  • For point A

25
  • Therefore, the difference in dynamic pressure is
  •        
  •            
  • The difference in total pressure can be obtained
    by applying Eq. (8.4.5) to point A and to the
    nose n,
  •        
  •          
  • Hence      
  •    
  • It can also be reasoned that the actual pressure
    difference varies by 1.5? from the dynamic
    pressure difference since A is 1.5 m above the
    nose, or

26
8.5 STREAM FUNCTIONS BOUNDARY CONDITIONS
  • Two-Dimensional Stream Function
  • If A, P represent two points in one of the flow
    planes, e.g., the xy plane (Fig. 8.4), and if the
    plane has unit thickness, the rate of flow across
    any two lines ACP, ABP must be the same if the
    density is constant and no fluid is created or
    destroyed within the region, as a consequence of
    continuity.
  • If A is a fixed point and P a movable point, the
    flow rate across any line connecting the two
    points is a function of the position of P.
  • If this function is ?, and if it is taken as a
    sign convention that it denotes the flow rate
    from right to left as the observer views the line
    from A looking toward P, then is defined as the
    stream function.

27
Figure 8.4 Fluid region showing the positive flow
direction used in the definition of a stream
function
Figure 8.5 Flow between two points in a fluid
region
28
  • If ?1 and ?2 represent the values of stream
    function at points Pl and P2 (Fig. 8.5),
    respectively, then ?2 - ?1 is the flow across
    PlP2 and is independent of the location of A.
  • Taking another point 0 in the place of A changes
    the values of ?1 and ?2 by the same amount,
    namely, the flow across OA. Then ? is
    indeterminate to the extent of an arbitrary
    constant.
  • The velocity components u, v in the x, y
    directions can be obtained from the stream
    function. In Fig. 8.6a, the flow d? across APdy,
    from right to left, is -udy, or
  • (8.5.1)
  • (8.5.2)

29
  • In plane polar coordinates from Fig. 8.6b.
  • Comparing Egs. (8.3.3) with Eqs. (8.5.1) and
    (8.5.2) leads to
  • (8.5.3)
  • These are the Cauchy-Riemann equations.
  •  
  • By Eqs. (8.5.3), a stream function can be found
    for each velocity potential. If the velocity
    potential satisfies the Laplace equation, the
    stream function also satisfies it. Hence, the
    stream function may be considered as velocity
    potential for another flow case.

30
Figure 8.6 Selection of path to show relation of
velocity components to stream function
31
  • Stokes's Stream Function for Axially Symmetric
    Flow
  • In any one of the planes through the axis of
    symmetry select two points A, P such that A is
    fixed and P is variable. Draw a line connecting
    AP.
  • The flow through the surface generated by
    rotating AP about the axis of symmetry is a
    function of the position of P. Let his function
    be 2P?, and let the x axis of symmetry be the
    axis of a cartesian system of reference. Then ?
    is a function of x and ?, where
  • is the distance from P to the x axis. The
    surfaces ? const are stream surfaces.
  • The resulting relations between stream function
    and velocity are given by

32
  • Solving for u and v gives
  • (8.5.4)
  • The same sign convention is used as in the
    two-dimensional case.
  • The relations between stream function and
    potential function are
  • (8.5.5)
  • The stream function is used for flow about bodies
    of revolution that are frequently expressed most
    readily in spherical polar coordinates. From Fig.
    8.7a and b,

33
  • from which              
  •                                 
                   (8.5.6)
  • and                                         
  • (8.5.7)
  • These expressions are useful in dealing with flow
    about spheres, ellipsoids, and disks and through
    apertures.

34
Figure 8.7 Displacement of to show the relation
between velocity components and Stokes' stream
function.
35
  • Boundary Conditions
  • At a fixed boundary the velocity component normal
    to the boundary must be zero at every point on
    the boundary (Fig. 8.8)
  •                                                   
                     (8.5.8)
  • n1  is a unit vector normal to the boundary. In
    scalar notation this is easily expressed in terms
    of the velocity potential
  •                                                   
                      (8.5.9)
  • at all points on the boundary. For a moving
    boundary (Fig. 8.9), where the boundary point has
    the velocity V, the fluid velocity component
    normal to the boundary must equal the velocity of
    the boundary normal to boundary thus
  •                                                   
                  (8.5.10)
  • or                                                
              
  • (8.5.11)

36
Figure 8.8 Notation for boundary condition at a
fixed boundary
Figure 8.9 Notation for boundary condition at a
moving boundary
37
8.6 THE FLOW NET
  • In two-dimensional flow the flow net is of great
    benefit it is taken up in this section.
  • The line given by f(x, y)const is called an
    equipotential line. It is a line along which the
    value of f (the velocity potential) does not
    change. Since velocity vs in any direction s is
    given by
  • The line f(x, y)const is a streamline and is
    everywhere tangent to the velocity vector.
    Streamlines and equipotential lines are therefore
    orthogonal i.e., they intersect at right angles,
    except at singular points.
  • In Fig. 8.10, if the distance between streamlines
    is ?n and the distance between equipotential
    lines is ?s at some small region in the flow net,
    the approximate velocity vs is the given in terms
    of the spacing of the equipotential lines Eq.
    (8.3.7),
  • or in terms of the spacing of streamlines Eqs.
    (8.5.1) and (8.5.2).

38
Figure 8.10 Elements of a flow net
39
  • In steady flow when the boundaries are
    stationary, the boundaries themselves become part
    of the flow net, as they are streamlines. The
    problem of finding the flow net to satisfy given
    fixed boundaries may be considered purely as a
    graphical exercise
  • This is one of the practical methods employed in
    two-dimensional-flow analysis, although it
    usually requires many attempts and much erasing.
  •  Another practical method of obtaining a flow net
    for a particular set of fixed boundaries is the
    electrical analogy. The boundaries in a model are
    formed out of strips of nonconducting material
    mounted on a flat nonconducting surface, and the
    end equipotential lines are formed out of a
    conducting strip, e.g., brass or copper.
  • The relaxation method numerically determines the
    value of potential function at points throughout
    the flow, usually located at the intersections of
    a square grid. The laplace equation is written as
    a difference equation, and it is shown that the
    value of the potential function at a grid point
    is the average of the four values at the
    neighboring grid points.

40
  • Use of the Flow Net
  • After a flow net for a given boundary
    configuration has been obtained, it may be used
    for all irrotational flows with geometrically
    similar boundaries.
  • Application of the Bernoulli equation Eq.
    (8.4.7) produces the dynamic pressure. If the
    velocity is known, e.g., at A (Fig. 8.10).
  • With the constant ?c determined for the whole
    grid in this manner, measurement of ?s or ?n at
    any other point permits the velocity to be
    computed there,
  •                
  • The concepts underlying the flow net have been
    developed for irrotational flow of an ideal
    fluid.

41
8.7 TWO-DIMENSIONAL FLOW
  • Flow around a Corner
  • The potential function
  •             
  •     
  • has as its stream function
  •                 
  • in which r and ? are polar coordinates. It is
    plotted for equal-increment changes in f and ? in
    Fig. 8.11. Conditions at the origin are not
    defined, as it is a stagnation point.
  • The streamlines are rectangular hyperbolas having
    yx as axes and the coordinate axes as
    asymptotes. From the polar form of the stream
    function it is noted that the two lines ?0 and
    ?p/2 are the streamline ?0.

42
Figure 8.11 Flow net for flow around a 90o
 bend
Figure 8.12 Flow net for flow along two inclined
surfaces
43
  • Source
  • A line normal to the xy plane, from which fluid
    is imagined to flow uniformly in all directions
    at right angles to it, is a source. It appears as
    a point in the customary two-dimensional flow
    diagram. The total flow per unit time per unit
    length of line is called the strength of the
    source.
  • Since by Eq. (8.3.7) the velocity in any
    direction is given by the negative derivative of
    the velocity potential with respect to the
    direction,
  • is the velocity potential, in which r is the
    distance from the source. This value of f
    satisfies the Laplace equation in two dimensions.

44
  • The streamlines are radial lines from the source,
    i.e.,
  •                
  • From the second equation
  •                
  • Lines of constant f (equipotential lines) and
    constant ? are shown in Fig. 8.13. A sink is a
    negative source, a line into which fluid is
    flowing.

Figure 8.13 Flow net for source or vortex
45
  • Vortex
  • In examining the flow case given by selecting the
    stream function for the source as a velocity
    potential,
  •                              
  • which also satisfies the Laplace equation, it is
    seen that the equipotential lines are radial
    lines and the streamlines are circles.
  • The velocity is in a tangential direction only,
    since ?f/?r0 . It is
  •                 
  • since r ?f is the length element in the
    tangential direction.
  • In referring to Fig. 8.14, the flow along a
    closed curve is called the circulation. The
    circulation G around a closed path C is

46
  • The value of the circulation is the strength of
    the vortex. By selecting any circular path of
    radius r to determine the circulation,
    hence,

Figure 8.14 Notation for definition of
circulation
47
  • Doublet
  • The two-dimensional doublet is defined as the
    limiting case as a source and sink of equal
    strength approach each other so that the product
    of their strength and the distance between them
    remains a constant 2pµ. µ is called the strength
    of the doublet.
  • In Fig. 8.15 a source is located at (a, 0) and a
    sink of equal strength at (-a, 0). The velocity
    potential for both, at some point P, is
  • with r1, r2 measured from source and sink,
    respectively, to the point P.

48
Figure 8.15 Notation for derivation of a
two-dimensional doublet
49
  • The terms r1, and r2 may be expressed in terms of
    the polar coordinates r, ? by the cosine law, as
    follows
  • Rewriting the expression for f with these
    relations gives

50
  • The series expression
  • leads to
  •              
  •                 
  •                 
  • After simplifying,

51
  • If 2amµ, and if the limit is taken as a
    approaches zero,
  •                 
  • which is the velocity potential for a
    two-dimensional doublet at the origin, with axis
    in the x direction.
  • Using the relations
  •                
  •              
  • gives for the doublet
  •            
  •                      
  • After integrating,

52
  • The equations in cartesian coordinates are
  •                           
  • Rearranging gives
  •                           
  • The lines of constant f are circles through the
    origin with centers on the x axis, and the
    streamlines are circles through the origin with
    centers on the y axis, as shown in Fig. 8.16.
  • The origin is a singular point where the velocity
    goes to infinity.

53
Figure 8.16 Equipotantial lines and streamlines
for the two-dimensional doublet
54
  • Uniform Flow
  • Uniform flow in the -x direction, u -U, is
    expressed by
  •                                   
  • In polar coordinates,

55
  • Flow around a Circular Cylinder
  • The addition of the flow due to a doublet and a
    uniform flow results in flow around a circular
    cylinder thus
  •                           
  • As a streamline in steady flow is a possible
    boundary, the streamline ?0 is given by
  •                 
  • which is satisfied by ?0, p, or by the value of
    r that makes
  •                 
  • If this value is ra, which is a circular
    cylinder, then

56
  • The potential and stream functions for uniform
    flow around a circular cylinder of radius a are,
    by substitution of the value of µ
  •          
  •                  
  • for the uniform flow in the -x direction. The
    equipotential lines and streamlines for this case
    are shown in Fig. 8.17
  • On the surface of the cylinder the velocity is
    necessarily tangential and is expressed by
    ??/?r0 for ra thus
  • For the dynamic pressure zero at infinity, with
    Eq. (8.4.7)

57
Figure 8.17 Equipotential lines and streamlines
for flow around a circular cylinder
58
  • For points on the cylinder,
  • A cylindrical pilot-static tube is made by
    providing three openings in a cylinder, at 0 and
    30, as the difference in pressure between 0
    and 30 is the dynamic pressure ?U2/2.
  • The drag on the cylinder is shown to be zero by
    integration of the x component of the pressure
    force over the cylinder thus
  • Similarly, the lift force on the cylinder is
    zero.

59
  • Flow around a Circular Cylinder with Circulation
  • The addition of a vortex to the doublet and the
    uniform flow results in flow around a circular
    cylinder with circulation,
  •                 
  •                 
  • The streamline is the circular cylinder r
    a. At great distances from the origin, the
    velocity remains u - U, showing that flow
    around a circular cylinder is maintained with
    addition of the vortex. Some of the streamlines
    are shown in Fig. 8.18.

60
Figure 8.18 Streamlines for flow around a
circular cylinder with circulation
61
  • The velocity at the surface of the cylinder,
    necessarily tangent to the cylinder, is
  •                 
  • Stagnation points occur when q0 that is,
  • The pressure at the surface of the cylinder is
  •               
  • The drag again is zero. The lift, however,
    becomes

62
  • The theoretical flow around a circular cylinder
    with circulation can be transformed  into flow
    around an airfoil with the same circulation and
    the same lift.
  • The airfoil develops its lift by producing
    circulation around it due to its shape. It can be
    shown that the lift is for any cylinder in
    two-dimensional flow. The angle or inclination of
    the airfoil relative to the approach velocity
    (angle of attack) greatly affects the
    circulation. For large angels or attack, the flow
    does not follow the wing profile, and the theory
    breaks down.
  • It should be mentioned that all two-dimensional
    ideal-fluid-flow cases may be conveniently
    handled by complex-variable theory and by a
    system of conformal mapping, which transforms a
    flow net from one configuration to another by a
    suitable complex-variable mapping function.

63
  • Example 8.3
  • A source with strength 0.2 m3/sm and a vortex
    with strength 1 m2/s are located at the origin.
    Determine the equations for velocity potential
    and stream function. What are the velocity
    components at x 1 m, y 0.5 m?
  • Solution
  • The velocity potential for the source is
  •                      
  • and the corresponding stream function is

64
  • The velocity potential for the vortex is
  •                                                   
       
  • and the corresponding stream function is
  •         
  •         
  • Adding the respective functions gives
  •              
  •        
  • The radial and tangential velocity components are
  •                          
  •               
  • At (1, 0.5), , vr 0.0285 m/s, v?
    0.143 m/s

65
  • Example 8.4
  • A circular cylinder 2 m in diameter and 20 m long
    is rotating at 120 rpm in the positive direction
    (counterclockwise) about its axis. Its center is
    at the origin of a cartesian coordinate system.
    Wind at 10 m/s blows over the cylinder in the
    positive x direction t200C and p100 kPa abs.
    Determine the lift on the cylinder and the
    location in the fourth quadrant of the streamline
    through the stagnation point.
  • Solution
  • The stagnation point has ?0 . By selecting
    increments of R, ? can be determined from
  •                
  • The lift is given by ?UGL.
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