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Sivasankar, Pugazhenthi, Lewis, Bennie G., Probe, Austin B., and Elgohary, Tarek A., 2025. A validation framework for orbit uncertainty propagation using real satellite data applied to orthogonal probability approximation. Acta Astronautica, 232:453–478, doi:10.1016/j.actaastro.2025.02.034.
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@ARTICLE{2025AcAau.232..453S,
author = {{Sivasankar}, Pugazhenthi and {Lewis}, Bennie G. and {Probe}, Austin B. and {Elgohary}, Tarek A.},
title = "{A validation framework for orbit uncertainty propagation using real satellite data applied to orthogonal probability approximation}",
journal = {Acta Astronautica},
keywords = {Space situational awareness, Uncertainty propagation, GRACE data, Chebyshev approximation, FireOPAL data},
year = 2025,
month = jul,
volume = {232},
pages = {453-478},
abstract = "{This paper presents a validation framework using data for uncertainty
propagation techniques for space situational awareness (SSA)
applications. In particular, we validate a novel technique for
uncertainty propagation, dubbed here as Orthogonal Probability
Approximation (OPA) This technique describes the evolution of
state/parameter uncertainties, e.g. initial condition and/or
drag coefficient, of nonlinear dynamical systems at a future
time. This new uncertainty quantification method employs
Liouville's theorem and Chebyshev polynomial approximation to
create a functional representation of the probability density
function (PDF) at the future time of interest at a fraction of
the computational cost of classical high-fidelity uncertainty
propagation methods. OPA is first compared against Polynomial
Chaos Expansions and Monte-Carlo simulations to numerically
demonstrate the accuracy of the method. For the real data
validation, two sources of satellite data are used: GRACE
navigation data from the Jet Propulsion Laboratory (JPL)
database, and FireOPAL ground-based observer provided by
Lockheed Martin. In the presented validation framework, the
state/parameter uncertainties of resident space objects (RSOs)
are propagated by OPA without using any measurements. The
maximum likelihood estimate and the uncertainty bounds of the
RSO state from OPA are compared with documented estimates and
uncertainty bounds obtained from real satellite/object tracking
data as well as other uncertainty propagation methods Results
indicate successful validation using GRACE navigation data
(precise orbit determination in LEO), and FireOPAL sensor
tracking data for Yamal 202 (GEO case) and a rocket body of
Block-DM satellite with highly elliptical orbit (HEO). The
results show the capability of OPA to accurately estimate the
states of RSOs in the absence of continuous measurements, and,
in addition, the presented framework can be used to validate any
uncertainty propagation technique.}",
doi = {10.1016/j.actaastro.2025.02.034},
adsurl = {https://ui.adsabs.harvard.edu/abs/2025AcAau.232..453S},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
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