Acoustic Oscillations in Solid Propellant Rocket
Chambers. Among the various kinds of periodic motions
observed in rocket combustion chambers, the most
common and simplest to analyze are those related to
classical acoustic modes. If the amplitudes are small,
the main perturbations of the familiar standing or
travelling waves in a closed chamber are proportional
to the Mach number of the mean flow. The correct
equations describing the problem are here obtained from
the general equations of motion by a limit process which
will also provide equations for studying waves of finite
amplitude. Subsequently, a single non-homogeneous
wave equation is deduced, and solved by an iteration·
perturbation procedure. The principal result is a simple
formula for the complex frequency showing explicitly
the effects of burning, suspended particles in the gases,
the exhaust nozzle, and viscous wall forces as well as
the mean flow itself. The last is particularly interesting
since, owing primarily to the flow inward from the
burning surface, the mean flow, if it is irrotational,
never acts to damp modes which do not involve axial
oscillations. As a particular application, the extensive
data taken by BROWNLEE and MARBLE are interpreted
to the extent that the linear analysis permits. A stability
boundary was obtained from 250 firings of small cylindrical
rockets, the principal variables being initial port
diameter and length. The propellant did not contain
metal particles, and it appears that the observations
cannot be explained by the supposition that viscous
damping associated with particles in the product gases
was the main source of energy loss. Apparently dissipation
at the head end, such as that associated with tangential
wall shear forces, was an important loss. On the other
hand, there is little doubt that if the combustion produces
particles, the consequent dissipation is adequate
to damp small amplitude waves.
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