| タイトル | Nonlinear Longitudinal Mode Instability in Liquid Propellant Rocket Engine Preburners |
| 本文（外部サイト） | http://hdl.handle.net/2060/20040085982 |
| 著者（英） | Flandro, Gary A.; Sims, J. D.; Majdalani, Joseph; Sims, Joseph D. |
| 著者所属（英） | NASA Marshall Space Flight Center |
| 発行日 | 2004-07-11 |
| 言語 | eng |
| 内容記述 | Nonlinear pressure oscillations have been observed in liquid propellant rocket instability preburner devices. Unlike the familiar transverse mode instabilities that characterize primary combustion chambers, these oscillations appear as longitudinal gas motions with frequencies that are typical of the chamber axial acoustic modes. In several respects, the phenomenon is similar to longitudinal mode combustion instability appearing in low-smoke solid propellant motors. An important feature is evidence of steep-fronted wave motions with very high amplitude. Clearly, gas motions of this type threaten the mechanical integrity of associated engine components and create unacceptably high vibration levels. This paper focuses on development of the analytical tools needed to predict, diagnose, and correct instabilities of this type. For this purpose, mechanisms that lead to steep-fronted, high-amplitude pressure waves are described in detail. It is shown that such gas motions are the outcome of the natural steepening process in which initially low amplitude standing acoustic waves grow into shock-like disturbances. The energy source that promotes this behavior is a combination of unsteady combustion energy release and interactions with the quasi-steady mean chamber flow. Since shock waves characterize the gas motions, detonation-like mechanisms may well control the unsteady combustion processes. When the energy gains exceed the losses (represented mainly by nozzle and viscous damping), the waves can rapidly grow to a finite amplitude limit cycle. Analytical tools are described that allow the prediction of the limit cycle amplitude and show the dependence of this wave amplitude on the system geometry and other design parameters. This information can be used to guide corrective procedures that mitigate or eliminate the oscillations. |
| NASA分類 | Spacecraft Propulsion and Power |
| レポートNO | AIAA Paper 2004-4162 |
| 権利 | Copyright, Distribution under U.S. Government purpose rights |
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