| Literature DB >> 27657069 |
Xi Liu1, Hua Qu2,3, Jihong Zhao4, Pengcheng Yue5, Meng Wang6.
Abstract
A new algorithm called maximum correntropy unscented Kalman filter (MCUKF) is proposed and applied to relative state estimation in space communication networks. As is well known, the unscented Kalman filter (UKF) provides an efficient tool to solve the non-linear state estimate problem. However, the UKF usually plays well in Gaussian noises. Its performance may deteriorate substantially in the presence of non-Gaussian noises, especially when the measurements are disturbed by some heavy-tailed impulsive noises. By making use of the maximum correntropy criterion (MCC), the proposed algorithm can enhance the robustness of UKF against impulsive noises. In the MCUKF, the unscented transformation (UT) is applied to obtain a predicted state estimation and covariance matrix, and a nonlinear regression method with the MCC cost is then used to reformulate the measurement information. Finally, the UT is adopted to the measurement equation to obtain the filter state and covariance matrix. Illustrative examples demonstrate the superior performance of the new algorithm.Entities:
Keywords: maximum correntropy criterion (MCC); unscented Kalman filter (UKF); unscented transformation (UT)
Year: 2016 PMID: 27657069 PMCID: PMC5038803 DOI: 10.3390/s16091530
Source DB: PubMed Journal: Sensors (Basel) ISSN: 1424-8220 Impact factor: 3.576
s of x in Gaussian noises.
| Filter | MSE of |
|---|---|
| UKF | 67.6974 |
| MCUKF | 87.6836 |
| MCUKF | 80.8406 |
| MCUKF | 74.0286 |
| MCUKF | 72.3362 |
| MCUKF | 68.6795 |
s of x in non-Gaussian measurement noise.
| Filter | MSE of |
|---|---|
| UKF | 85.8439 |
| MCUKF | 84.1944 |
| MCUKF | 82.6933 |
| MCUKF | 83.1098 |
| MCUKF | 84.7173 |
| MCUKF | 85.4411 |
Figure 1Illustration of example 2.
Figure 2Measurement coordinate system.
Initial orbital elements of chief spacecraft.
| Orbital Elements | Chief Spacecraft |
|---|---|
| Semi-major axis | 8000 km |
| Eccentricity | 0.150 |
| Orbit inclination | |
| Argument of perigee | |
| Right ascension of the ascending node | |
| True anomaly | 0 rad |
Figure 3Relative motion of the deputy spacecraft in the Hill frame.
Figure 4with different filters in Gaussian noises.
Figure 5with different filters in Gaussian noises.
and in Gaussian noises.
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| EKF |
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| HEKF |
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| UKF |
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| NRUKF |
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| MCUKF |
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| MCUKF |
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| MCUKF |
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Figure 6with different filters in non-Gaussian noises.
Figure 7with different filters in non-Gaussian noises.
and in non-Gaussian noises.
| Filter |
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| EKF |
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| HEKF |
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| UKF |
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| NRUKF |
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| MCUKF |
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| MCUKF |
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| MCUKF |
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Computation time comparison.
| Filter | Computation Ratio |
|---|---|
| UKF | 1 |
| HEKF |
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| NRUKF |
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| MCUKF |
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