To describe the acoustic instabilities in the combustion chambers of laterally burning solid propellant rockets the interaction of the mean flow with the acoustic waves is analysed, using multiple scale techniques, for realistic cases in which the combustion chamber is slender and the nozzle area is small compared with the cross-sectional area of the chamber. Associated with the longitudinal acoustic oscillations we find vorticity and entropy waves, with a wavelength typically small compared with the radius of the chamber, penetrating deeply into the chamber. We obtain a set of differential equations to calculate the radial and axial dependence of the amplitude of these waves. The boundary conditions are provided by the acoustic admittance of the propellant surface, given by an existing analysis of the thin gas-phase reaction layer adjacent to the solid-gas interface, and of the nozzle, accounting here for the possible effect of the vorticity and entropy waves. The equations are integrated in closed form and the results provide the growth rate of the disturbances, which we use to determine the conditions for instability of the longitudinal oscillations.
IntroductionThe purpose of this paper is to clarify the role of the vorticity and entropy waves that accompany acoustic oscillations in solid rocket motors in their acoustic instabilities. With this aim, we shall consider the simple case of an axis-symmetric configuration, in which the solid propellant is of cylindrical shape, bounded externally by an enclosure and with a cylindrical gaseous cavity of circular shape inside. The cavity is closed at one end by an endwall and the other end is attached to a nozzle, where the gases generated by the combustion process in the internal surface of the propellant are accelerated to supersonic speeds.If the Mach number in the nozzle throat is close to unity, the ratio of its area, A t , to the internal surface area, A s , of the propellant bounding the cavity must be, as derived from mass conservation considerations, of the order of the Mach number M b = V b /c b of the gaseous combustion products leaving, with velocity V b , the thin reaction layer adjacent to the surface of the propellant. M b 1, because V b is typically of the order of 1 m s −1 , very small compared with the sound velocity c b of the burned gases. Due to the small value of A t /A s , the attenuation of any acoustic oscillations that may be excited in the nearly closed gaseous cavity is very weak, and this may contribute to the existence of combustion instabilities in the chamber. The analysis of the acoustic instabilities has received considerable attention in the literature; see, for example, the