As an object moves through a gas, the gas molecules are deflected
around the object. If the speed of the object is much less than the
speed of sound
of the gas, the density of the gas remains constant and the flow of
gas can be described by conserving
momentum, and
energy.
As the
speed of the object approaches the speed of sound, we
must consider
compressibility effects
on the gas. The density of the gas varies locally as the gas is
compressed by the object.

For compressible flows with little or small
flow turning, the flow process is reversible and the
entropy
is constant.
The change in flow properties are then given by the
isentropic relations
(isentropic means "constant entropy").
But when an object moves faster than the speed of sound,
and there is an abrupt decrease in the flow area,
shock waves are generated in the flow.
Shock waves are very small regions in the gas where the
gas properties
change by a large amount.
Across a shock wave, the static
pressure,
temperature,
and gas
density
increases almost instantaneously.
The changes in the flow
properties are irreversible and the
entropy
of the entire system increases.
Because a shock wave does no work, and there is no heat addition, the
total
enthalpy
and the total temperature are constant.
But because the flow is non-isentropic, the
total pressure downstream of the shock is always less than the total pressure
upstream of the shock. There is a loss of total pressure associated with
a shock wave.

On this page, we consider the supersonic flow of air past a two-dimensional wedge.
If the Mach number is high enough and the wedge angle is small enough, an
oblique shock wave
is generated by the wedge, with the origin of the shock attached to the sharp leading
edge of the wedge. If we think of the oblique shock as a
normal shock
inclined to the flow at some shock angle s, then the normal shock relations can
be applied across the shock in a direction perpendicular to the shock, and the flow component
parallel to the shock remains unchanged. The resulting
Mach number
and speed of the flow decrease across the shock wave.
For the Mach number change across an oblique shock there are
two possible solutions; one supersonic and one subsonic. In nature, the
supersonic ("weak shock") solution occurs most often. However, under some
conditions the "strong shock", subsonic solution is possible.
For a given upstream Mach number, there is a maximum wedge angle for which the
shock remains attached to the leading edge. For wedge angles greater than the maximum, a
detached normal shock
occurs. The conditions for an attached shock is shown on the slide.

where M is the free stream Mach number, a is the wedge angle measured in radians,
and gamma is the ratio of specific heats for the gas (=1.4 for air at sea -level
standard temperature and pressure).

On the slide we have listed the equations which describe the change
in flow variables for flow past a two dimensional shock generated by a wedge
of angle a.
The equations presented here were derived by considering the conservation of
mass,
momentum, and energy
for a compressible gas while ignoring viscous effects.
The equations have been further specialized for a two-dimensional flow
(not three dimensional axisymmetric) without heat addition.
The equations only apply for
those combinations of free stream Mach number and wedge angle for which
an attached oblique shock occurs. If the Mach number is too low, or the
wedge angle too high, the
normal shock
equations should be used.

For the problem given on the slide, a supersonic flow at Mach number M
approaches a wedge of angle a. A shock wave is generated which is
inclined at angle s. Then:

The right hand side of all these equations depend only on the free stream
Mach number and the shock angle. The shock angle depends in a complex way on
the free stream Mach number and the wedge angle. So knowing the Mach number
and the wedge angle, we can determine all the conditions associated with
the oblique shock.
The equations describing oblique shocks
were published in NACA report
(NACA-1135)
in 1951.

Here's a Java program based on the oblique shock equations.
You can use this simulator to study the flow past a wedge.

Due to IT
security concerns, many users are currently experiencing problems running NASA Glenn
educational applets. The applets are slowly being updated, but it is a lengthy process.
If you are familiar with Java Runtime Environments (JRE), you may want to try downloading
the applet and running it on an Integrated Development Environment (IDE) such as Netbeans or Eclipse.
The following are tutorials for running Java applets on either IDE:
Netbeans Eclipse

Input to the program can be made
using the sliders, or input boxes at the upper right. To
change the value of an input variable, simply move the slider. Or
click on the input box, select and replace the old value, and
hit Enter to send the new value to the program.
Output from the program is displayed
in output boxes at the lower right. The flow variables are presented as ratios
to free stream values. The graphic at the left shows the wedge (in red)
and the shock wave generated by the wedge as a line. The line is colored
blue for an oblique shock and magenta when the shock is a normal shock. The black
lines show the streamlines of the flow past the wedge. Notice that downstream
(to the right) of the shock wave, the lines are closer together than upstream.
This indicates an increase in the density of the flow.

There is more complete
shock simulation program
that is also avaliable at this web site. It solves for both flow past a wedge
and flow past a
cone.
If you are an experienced user of the simulator, you can use a
sleek version
of the program which loads faster on your computer and does not include the
user's manual. The
ShockModeler
program models the intersection and reflection of multiple oblique shock waves
generated by multiple wedges.
You can also download your own copy of the program to run off-line by clicking on this button: