Multi-Fidelity Monte-Carlo Estimation of Satellite Drag in Very-Low-Earth Orbit
Jovan Boskovic, Marcel Pfeifer, Andrea Beck

TL;DR
This paper introduces a multi-fidelity Monte Carlo method to efficiently estimate satellite drag uncertainty in very-low-Earth orbit by combining high-fidelity DSMC simulations with low-fidelity panel models.
Contribution
It develops a novel MFMC estimator that leverages panel models as control variates to reduce computational cost in drag uncertainty quantification.
Findings
MFMC reduces RMSE of drag coefficient estimates when low-fidelity models are highly correlated.
The method is validated on CubeSat and satellite configurations with thermospheric variability.
Practical factors like correlation and cost ratios influence the effectiveness of control variates.
Abstract
Very-low-Earth orbit drag uncertainty quantification in the rarefied/transitional Knudsen-number regime requires estimating not only the mean drag coefficient but also higher-order moments under atmospheric variability, which becomes prohibitively expensive when high-fidelity kinetic solvers are required. This work develops a multi-fidelity Monte Carlo (MFMC) estimator for the drag coefficient using a DSMC solver (PICLas) as the high-fidelity model and two free-molecular panel-method variants (ADBSat with Sentman and Cercignani-Lampis-Lord (CLL) gas-surface interaction models) as low-fidelity control variates. We treat E[C_D] and E[C_D^2] as the primary estimation targets and form the physically induced variance only afterwards via Var(C_D)=E[C_D^2]-(E[C_D])^2. High-fidelity reference moments are obtained from long DSMC sequences using objective convergence criteria based on…
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