Atmospheric Density Uncertainty Quantification for Satellite Conjunction Assessment
David J. Gondelach, Richard Linares

TL;DR
This paper introduces a novel method for quantifying atmospheric density uncertainties and incorporating them into satellite conjunction assessments, improving collision risk estimates by accounting for density error correlations.
Contribution
It presents a dynamic reduced-order density model that efficiently estimates density uncertainties and propagates them for collision probability calculations, including cross-correlation effects.
Findings
Density uncertainties significantly impact collision probability estimates.
Ignoring cross-correlation can lead to severe underestimation of collision risk.
The method improves the accuracy of conjunction assessments by incorporating density error dependencies.
Abstract
Conjunction assessment requires knowledge of the uncertainty in the predicted orbit. Errors in the atmospheric density are a major source of error in the prediction of low Earth orbits. Therefore, accurate estimation of the density and quantification of the uncertainty in the density is required. Most atmospheric density models, however, do not provide an estimate of the uncertainty in the density. In this work, we present a new approach to quantify uncertainties in the density and to include these for calculating the probability of collision Pc. For this, we employ a recently developed dynamic reduced-order density model that enables efficient prediction of the thermospheric density. First, the model is used to obtain accurate estimates of the density and of the uncertainty in the estimates. Second, the density uncertainties are propagated forward simultaneously with orbit propagation…
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Taxonomy
TopicsIonosphere and magnetosphere dynamics · GNSS positioning and interference · Monetary Policy and Economic Impact
