TY - GEN
T1 - Adaptive Picard-Chebyshev Methods for Bang-Bang Control Dynamics
AU - Pascarella, Alex
AU - Woollands, Robyn M.
N1 - Publisher Copyright:
© 2024 by the American Institute of Aeronautics and Astronautics, Inc. All rights reserved.
PY - 2024
Y1 - 2024
N2 - Numerical integration of dynamical systems is vital to science and engineering applications as it allows solutions to be obtained numerically when analytical solutions do not exist. In this paper we present an improved methodology for propagating high-fidelity low-thrust trajectories, that exhibit a bang-bang dynamical behavior, using Picard-Chebyshev methods. The approach combines a true anomaly informed segmentation scheme as well as early anticipation and accommodation of on/off engine switches which are a challenge for implicit integrators. Adaptation of segment length and Chebyshev polynomial degree is carried out using the accuracy of the acceleration fit (force model), prior to integration with Picard iteration, as an error metric. The magnitude of the smallest Chebyshev coefficients of the acceleration is also monitored to determine if their contribution is significant to warrant inclusion. We demonstrate the utility of this novel method for solving a fuel-optimal low-thrust transfer problem from a geostationary transfer orbit to geosynchronous orbit. A radially adaptive, variable fidelity spherical harmonic gravity model is included in our simulations. We compare the performance of the algorithm to MATLAB’s ode89 and find that APC requires about 15% of the computation time, compared with ode89, when a solution with a 5 minute output timestep is required.
AB - Numerical integration of dynamical systems is vital to science and engineering applications as it allows solutions to be obtained numerically when analytical solutions do not exist. In this paper we present an improved methodology for propagating high-fidelity low-thrust trajectories, that exhibit a bang-bang dynamical behavior, using Picard-Chebyshev methods. The approach combines a true anomaly informed segmentation scheme as well as early anticipation and accommodation of on/off engine switches which are a challenge for implicit integrators. Adaptation of segment length and Chebyshev polynomial degree is carried out using the accuracy of the acceleration fit (force model), prior to integration with Picard iteration, as an error metric. The magnitude of the smallest Chebyshev coefficients of the acceleration is also monitored to determine if their contribution is significant to warrant inclusion. We demonstrate the utility of this novel method for solving a fuel-optimal low-thrust transfer problem from a geostationary transfer orbit to geosynchronous orbit. A radially adaptive, variable fidelity spherical harmonic gravity model is included in our simulations. We compare the performance of the algorithm to MATLAB’s ode89 and find that APC requires about 15% of the computation time, compared with ode89, when a solution with a 5 minute output timestep is required.
UR - http://www.scopus.com/inward/record.url?scp=85194063088&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=85194063088&partnerID=8YFLogxK
U2 - 10.2514/6.2024-1282
DO - 10.2514/6.2024-1282
M3 - Conference contribution
AN - SCOPUS:85194063088
SN - 9781624107115
T3 - AIAA SciTech Forum and Exposition, 2024
BT - AIAA SciTech Forum and Exposition, 2024
PB - American Institute of Aeronautics and Astronautics Inc, AIAA
T2 - AIAA SciTech Forum and Exposition, 2024
Y2 - 8 January 2024 through 12 January 2024
ER -