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  • Viscous Flows A.H. Shapiro and A.A. Sonin 6.16

    Problem 6.16This problem is from Advanced Fluid Mechanics Problems by A.H. Shapiro and A.A. Sonin

    viscous liquid

    g

    y

    x

    h(x, t)

    air, pa

    A rigid plane surface is inclined at an angle relative to the horizontal and wetted by a thin layer of highlyviscous liquid which begins to flow down the incline.

    (a) Show that if the flow is two-dimensional and in the inertia-free limit, and if the angle of the inclinationis not too small, the local thickness h(x, t) of the liquid layer obeys the equation

    h

    t+ c

    h

    x= 0

    where

    c =gh2

    sin

    (b) Demonstrate that the result of (a) implies that in a region where h decreases in the flow direction,the angle of the free surface relative to the inclined plane will steepen as the fluid flows down theincline, while in a region where h increases in the flow direction, the reverse is true. Does this explainsomething about what happens to slow-drying paint when it is applied to an inclined surface?

    (c) Considering the result of (b) above, do you think that the steady-state solutions of the previousproblems would ever apply in practice? Discuss.

    Solution:

    (a) Assumptions:

    ReH HL 1 two dimensional flow THIN layer HL = characteristic heightcharacteristic length 1

    Unknown: h(x, t)?

    For the sake of completeness, this solution provides detailed nondimensionalization of full 2D Navier-Stokes as well as continuity equations. So please bear with me!!

    (1) Choose relevant scales: (* denotes dimensionless variables)

    x =x

    Lvx =

    vxU

    t =tU

    L

    y =y

    Hvy =

    vyV

    p =p

    Pwhere P is an unknown pressure scale.

    2.25 Advanced Fluid Mechanics 5 Copyright c 2006, MIT

  • Viscous Flows A.H. Shapiro and A.A. Sonin 6.16

    (2) Non-dimensionalize continuity:

    vxx

    +vyy

    = 0

    U

    L

    vxx

    +V

    L

    vyy

    = 0

    Since dimensionless variables are assumed to be of the same order (O(1)),U

    L V

    H

    V = HLU where

    H

    L 1

    (3) Non-dimensionalize Navier-Stokes:x-direction:

    U2

    L

    (vxt

    + vxvxx

    + vyvxy

    )= P

    L

    p

    x+ g sin +

    (U

    L22vxx2

    +U

    H22vxy2

    )Divide through by UH2 :

    UH2

    L ReH

    HL=small

    (vx

    t+ vx

    vxx

    + vyvxy

    )= PH

    2

    UL

    p

    x+gH2 sin

    U+(H

    L

    )2 small

    2vx

    x2+2vxy2

    y-direction:

    U2

    L

    H

    L

    (vyt

    + vxvyx

    + vyvyy

    )= P

    H

    p

    y g cos + H

    L

    (U

    L22vyx2

    +U

    H22vyy2

    )Divide through by UH2 :

    UH2

    L ReH(HL )

    2=small

    (vy

    t+ vx

    vyx

    + vyvyy

    )= PH

    U

    p

    y gH

    2 cos U

    +(H

    L

    )3 small

    2vyx2

    +H

    Lsmall

    2vy

    y2

    Now assume that PHU O(1):1

    P = UH viscous pressure scale for low Re

    Substitute this expression for P in x-direction equation:

    0 = UH

    H2

    UL

    p

    x+gH2 sin

    U+2vxy2

    0 = HL

    small

    p

    x+gH2 sin

    U+2vxy2

    0 = gH2 sin U

    +2vxy2

    xmomentum

    and 0 =p

    y+gH2 cos

    U ymomentum

    Going back to the dimensional form,

    0 = g sin + 2vxy2

    (6.16a)

    1Notice we now only have a hydrostatic relation in y-direction

    2.25 Advanced Fluid Mechanics 6 Copyright c 2006, MIT

  • Viscous Flows A.H. Shapiro and A.A. Sonin 6.16

    (4) Solve for vx by integrating both sides of Eq. (6.16a):2vxy2

    dy =

    g sin

    dy

    2vxy2

    = g sin

    y + C1

    Using B.C. that vxy = 0 at y = h (free surface),

    C1 =gh sin

    2vxy2

    = g sin

    (y h)

    Integrating again and using no-slip B.C. (vx = 0 at y = 0):

    vx =g sin

    (hy 1

    2y2) (6.16b)

    (5) Use mass conservation to obtain a single evolution equation for h(x, t).Consider the following control volume in the limit of x 0:

    d

    dt

    CV

    dV + CS

    (v vc) ndA = 0

    limx0

    ddt

    (hx) + h0vxdy

    x= 0

    ht

    +

    x

    ( h0

    vxdy

    )=

    h

    t+Q

    x= 0 (6.16c)

    The above equation can also be derived by combining the kinematic boundary condition, ht +vx

    hx = vy|y=h(x), with conservation of mass.

    (6) Combine Eq. (6.16b) with Eq. (6.16c):

    h

    t+

    x

    h0

    g sin

    (hy 12y2)dy = 0

    h

    t+g sin

    x

    (h3

    3

    )= 0

    h

    t+(g sin

    h2)

    c

    h

    x= 0 (6.16d)

    Eq. (6.16d) is a nonlinear wave equation with a solution of the form h = f(x ct), where c is thewave speed.

    (b) Since g sin h2 0, ht and hx have opposite signs to satisfy Eq. (6.16d).

    Thus, where h is decreasing locally (hx < 0), h increases in time (ht > 0).

    Angle of free surface steepens because points oflarger h increase more rapidly (c h2) thanpoints of lower h:

    2.25 Advanced Fluid Mechanics 7 Copyright c 2006, MIT

  • Viscous Flows A.H. Shapiro and A.A. Sonin 6.16

    Where h is increasing locally (hx > 0), h decreases in time (ht < 0),

    Angle of free surface flattens because points oflarger h decrease more rapidly (c h2) thanpoints of lower h:

    In the case of slow-drying paint, when thereis a bump, Eq. (6.16d) dictates that the bumpgrows! However it never forms a shock becausein reality, one has to consider effects of surfacetension.

    In practice, the solution to Eq. (6.16d) fails (or goes unstable) in the case of a symmetric perturbation,as explained in (b). Thus, it is not very applicable unless one accounts or effects of surface tension andsuch.

    However, when h is monotonically increasing (hx > 0 everywhere) the solution to Eq. (6.16d) is indeedstable since it predicts that h flattens in time.

    Problem Solution by Sungyon Lee, Fall 2005

    2.25 Advanced Fluid Mechanics 8 Copyright c 2006, MIT

  • Problem 6.21 (a) In terms of flow geometry, this problem is similar to 6.3; the difference here being that the flow is unsteady! Writing the Navier-Stokes equation in the cylindrical gap between the bearing pad and ground:

    N N N2 2 2

    2 2 2 2 2

    1 1 2r r r r r r r rr z

    VII VII III IV

    u uu u u u u u u upu u rt r r z r r r r r r z r r

    u + + + = + + +

    Lets perform an order-of-magnitude analysis. Note that 0 = .

    2

    2~ 1IV hV D

  • Since it is given that S is very small and also h is small, we can safely assume that I can be neglected compared to V. Hence we have the N-S eqn as:

    2

    2 0rup

    r z + =

    Integrating, we get u as: ( )r z

    ( )212r pu zr = h z 3 3

    0

    ( ) 2 ( )6 6

    h

    rh r p h r dpQ r r u z dz

    r d

    = = = r (3) Note that Q is a function of r, since the settling down of the pad drives greater and greater flow rates as r increases! This can be verified by applying mass conservation in a cylindrical CV, as shown. The height of this CV changes as h(t).

    Deforming CV: Radius r, Height h(t)

    W

    r = 0

    ur urh(t)

    S

    0 ( CSCV CS

    d dV V V ndAdt

    = + G G G). ( )2 22 0 2r rd dhr h rhu r rhu Q rdt dt + = = = ( )

    Since, dh Sdt

    = , we have: 2( )Q r r S=

    Plugging Q(r) into (3), we have:

    32

    3

    66

    h r dp Srr S dp drdr h

    = =

    2.25 Advanced Fluid Mechanics Copyright 2007, MIT

  • 22

    3

    3( )4

    S Dp r rh =

    where the BC used is 02Dp = (gauge pressure!)

    Now, we can perform a vertical force-balance on the pad:

    2 42

    23 3

    0

    3 324 3

    D

    S D SDrdrh h = = 2

    W r

    3

    4

    323

    WhSD = (4)

    (b) Plugging in the numbers, we obtain

    159

    4

    32 100 27 10 1.2 10 /3 0.93 81 10

    S m

    = = s (very small!) (c) From (4), we have:

    0

    3

    4 30

    32 323 3

    h t

    h

    dh Wh dh WSdt D h D = = = 4 dt (5)

    1/ 22

    02 2 4 4

    0 0

    641 1 64 13 3

    WhWt h th h D h D

    = = +

    (d) 2 . Plugging in the values, we get the time required as 10.4 hours. 0h h=

    (e) Referring to relation (5), dhSdt

    = instead of dhdt

    and consequently, we have:

    2 20

    1 1 643

    Fth h D = 4 As the disk is pulled away, and we have th as:

    4

    20

    364

    Dth F

    =

    Solution by Mayank Kumar, Fall 2007

    2.25 Advanced Fluid Mechanics Copyright 2007, MIT

  • Problem 6.216.21.pdfProblem 6.21