NASA NTRS · 19920013251
Physical lumping methods for developing linear reduced models for high speed propulsion systems
Abstract
In gasdynamic systems, information travels in one direction for supersonic flow and in both directions for subsonic flow. A shock occurs at the transition from supersonic to subsonic flow. Thus, to simulate these systems, any simulation method implemented for the quasi-one-dimensional Euler equations must have the ability to capture the shock. In this paper, a technique combining both backward and central differencing is presented. The equations are subsequently linearized about an operating point and formulated into a linear state space model. After proper implementation of the boundary conditions, the model order is reduced from 123 to less than 10 using the Schur method of balancing. Simulations comparing frequency and step response of the reduced order model and the original system models are presented.
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Immel, S. M., Hartley, Tom T., Deabreu-Garcia, J. Alex. 1991-12-01. Physical lumping methods for developing linear reduced models for high speed propulsion systems. https://ntrs.nasa.gov/citations/19920013251
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