AE1303 AERODYNAMICS II - PowerPoint PPT Presentation

1 / 30
About This Presentation
Title:

AE1303 AERODYNAMICS II

Description:

Prandtl-Glauert Rule for Linearized Subsonic Flow (2-D Over Thin Airfoils) ... For supersonic flow over any 2-D slender airfoil, ... – PowerPoint PPT presentation

Number of Views:971
Avg rating:3.0/5.0
Slides: 31
Provided by: rajala
Category:

less

Transcript and Presenter's Notes

Title: AE1303 AERODYNAMICS II


1
AE1303 AERODYNAMICS -II
2
ONE DIMENSIONAL COMPRESSIBLE FLOW
  • Continuity Equation
  • for steady flow

3
ONE DIMENSIONAL COMPRESSIBLE FLOW
  • EULER EQUATION

For steady flow
4
ONE DIMENSIONAL COMPRESSIBLE FLOW
Momentum Equation
Energy Equation
5
Oblique Shock Waves
  • The oblique shock waves typically occurs when a
    supersonic flow is turned to itself by a wall or
    its equivalent boundary condition.
  • All the streamlines have the same deflection
    angle q at the shock wave, parallel to the
    surface downstream.
  • Across the oblique shock, M decreases but p, T
    and r increase.

6
Expansion Waves
  • The expansion waves typically occur when a
    supersonic flow is turned away from itself by a
    wall or its equivalent boundary condition.
  • The streamlines are smoothly curved through the
    expansion fan until they are all parallel to the
    wall behind the corner point.
  • All flow properties through an expansion wave
    change smoothly and continuously. Across the
    expansion wave, M increases while p, T, and r
    decreases.

7
Source of Oblique Waves
  • For an object moving at a supersonic speed, the
    object is always ahead of the sound wave fronts
    generated by the object. This cause the sound
    wave fronts to coalesce into a line disturbance,
    called Mach wave, at the Mack angle m relative to
    the direction of the beeper.
  • The physical mechanism to form the oblique shock
    wave is essentially the same as the Mach wave.
    The Mach wave is actually an infinitely weak
    shock wave.

8
Oblique Shock Relations
  • The oblique shock tilts at a wave angle b with
    respect to V1, the upstream velocity. Behind the
    shock, the flow is deflected toward the shock by
    the flow deflection angle q.
  • Let u and w denote the normal and parallel flow
    velocity components relative to the oblique shock
    and Mn and Mt the corresponding Mach numbers, we
    have for a steady adiabatic flow with no body
    forces the following relations

9
Oblique Shock Relations (contd.)
  • So and Mn1 and Mn2 all satisfy
    the corresponding normal shock relations, which
    are all functions of M1 and b, because

10
Oblique Shock Relations (contd.)?-ß-M relation
  • For any given free stream Mach number M1, there
    is
  • a maximum q beyond which the shock will be
    detached.
  • For any given M1 and q lt qmax, there are two bs.
    The
  • larger b is called the strong shock
    solution, where M2 is
  • subsonic. The lower b is called the weak
    shock solution,
  • where M2 is supersonic except for a small
    region near
  • qmax.
  • 3. If q 0, then b p/2 (normal shock) or b m
    (Mach wave).

11
Straight Oblique Shock Relations (contd.)
  • For a calorically perfect gas,

12
Supersonic Flow Over Cones
  • The flow over a cone is inherently
    three-dimensional. The three-dimensionality has
    the relieving effect to result in a weaker shock
    wave as compared to a wedge of the same half
    angle.
  • The flow between the shock and the cone is no
    longer uniform the streamlines there are curved
    and the surface pressure are not constant.

13
Shock Wave Reflection
  • Consider an incident oblique shock on a lower
    wall that is reflected by the upper wall at
    point. The reflection angle of the shock at the
    upper wall is determined by two conditions
  • (a) M2 lt M1
  • (b) The flow downstream of the reflected shock
  • wave must be parallel to the upper
    wall. That is, the flow is deflected downward by
    q.

14
Pressure-Deflection Diagram
  • The pressure-deflection diagram is a plot of the
    static pressure behind an oblique shock versus
    the flow deflection angle for a given upstream
    condition.
  • For left-running waves, the flow deflection angle
    is upward it is considered as positive. For
    right-running waves, the flow deflection angle is
    downward it is considered as negative.

15
Intersection of Shock Waves of Opposite Families
  • Consider the intersection of left- and
    right-running shocks (A and B). The two shocks
    intersect at E and result in two refracted shocks
    C and D. Since the shock wave strengths of A and
    B in general are different, there is a slip line
    in the region between the two refracted waves
    where
  • (a) the pressure is continuous but the entropy
    is
  • discontinuous at the slip line
    (b) the velocities
    on two sides of the slip line are in the
  • same direction but of different
    magnitudes

16
Intersection of Shock Waves of the Same Family
  • As two left running oblique shock waves A and B
    intersect at C , they will form a single shock
    wave CD and a reflected shock wave CE such that
    there is slip line in the region between CD and
    CE.

17
Prandtl-Meyer Expansion Waves
  • M2 gt M1. An expansion corner is a means to
    increase the flow mach number.
  • P2/p1 lt1, r2/r1 lt1, T2/T1 lt 1. The pressure,
    density, and temperature decrease through an
    expansion wave.
  • The expansion fan is a continuous expansion
    region, composed of of an infinite number of Mach
    waves, bounded upstream by m1 and downstream by
    m2.

18
Prandtl-Meyer Expansion Waves (contd.)
  • Centered expansion fan is also called
    Prandtl-Meyer expansion wave.
  • where m1 sin-1(1/M1) and m2 sin-1(1/M2).
  • Streamlines through an expansion wave are smooth
    curved lines.
  • Since the expansion takes place through a
    continuous succession of Mach waves, and ds 0
    for each wave, the expansion is isentropic.

19
Prandtl-Meyer Expansion Waves (contd.)
  • For perfect gas, the Prandtl-Meyer expansion
    waves are governed by
  • Knowing M1 and q2, we can find
  • M2

20
Prandtl-Meyer Expansion Waves (contd.)
  • Since the expansion is isentropic, and hence To
    and Po are constant, we have

21
Shock-Expansion Method-Flow Conditions
Downstream of the Trailing Edge
  • In supersonic flow, the conditions at the
    trailing edge cannot affect the flow upstream.
    Therefore, unlike the subsonic flow, there is no
    need to impose a Kutta condition at the trailing
    edge in order to determine the airfoil lift.
  • However, if there is an interest to know the flow
    conditions downstream of the T.E., they can be
    determined by requiring the pressures downstream
    of the top- and bottom-surface flows to be equal.

22
Conditions Downstream of the T.E.-An Example
  • For the case shown, the angle of attack is less
    than the wedges half angle so we expect two
    oblique shocks at the trailing edge.
  • In order to know the flow conditions downstream
    of the airfoil, we start a guess value of the
    deflection angle g of the downstream flow
    relative of the free stream.
  • Knowing the Mach number and static pressure
    immediately upstream of each shock leads to the
    prediction of the static pressures downstream of
    each shock.
  • Then through the iteration process, g is changed
    until the pressures downstream of the top- and
    bottom-surface flow become equal.

23
Total and Perturbation Velocity Potentials
  • Consider a slender body immersed in an inviscid,
    irrotational flow where
  • We can define the (total) velocity potential F
    and the perturbation velocity potential f as
    follows

24
Velocity Potential Equation
  • For a steady, irrotational flow, starting from
    the differential continuity equation
  • we have
  • In terms of the velocity potential F(x,y,z), the
    above continuity equation becomes

25
Linearized Velocity Potential Equation
  • By assuming small velocity perturbations such
    that
  • we can prove that for the Mach number ranges
    excluding

the transonic range
the hypersonic range
26
Linearized Pressure Coefficient
  • For calorically perfect gas, the pressure
    coefficient Cp can be reduce to
  • For small velocity perturbations, we can prove
    that
  • Note that the linearized Cp only depends on u.

27
Prandtl-Glauert Rule for Linearized Subsonic Flow
(2-D Over Thin Airfoils)
28
Cp of 2-D Supersonic Flows Around Thin Wings
  • For supersonic flow over any 2-D slender airfoil,
  • where q is the local surface inclination with
    respect to the free stream

29
Cl of 2-D Supersonic Flow Over Thin Wings
  • For supersonic flow over any 2-D slender airfoil,

30
Cm of 2-D Supersonic Flow Over Thin Wings
  • For supersonic flow over any 2-D slender airfoil,
    the pitching moment coefficient with respect to
    an arbitrary point xo is
  • The center of pressure for a symmetrical airfoil
    in supersonic flow is predicted at the mid-chord
    point.
Write a Comment
User Comments (0)
About PowerShow.com