Publishing Service

Polishing & Checking

Frontiers of Information Technology & Electronic Engineering

ISSN 2095-9184 (print), ISSN 2095-9230 (online)

Multiplication extended Kalman filter-aided non-blind star image restoration algorithm based on the heterogeneous blur kernel

Abstract: Under dynamic conditions, the smearing effect of star spots on the image plane reduces centroid extraction accuracy, which has an impact on attitude estimation. To enhance the dynamic performance of the star sensor, we propose a multiplication extended Kalman filter (MEKF)-aided non-blind star image restoration algorithm based on the heterogeneous blur kernel. The proposed algorithm consists of three procedures. First, the MEKF is used to estimate the attitude and gyro drift to eliminate the measurement error of the star sensor and gyro drift. Second, the attitude predicted by MEKF is used, which provides initial conditions and accelerates the subsequent algorithm. Finally, a gyro-assisted heterogeneous blur kernel estimation algorithm is presented for restoring non-uniform and nonlinear motion-blurred star images. In contrast to existing dynamic star image deblurring algorithms, which focus mostly on image content, the proposed method emphasizes the cause of motion blur by fusing MEKF and a heterogeneous blur kernel. This leads to significantly enhanced robustness against noise and improved restoration accuracy. Simulation results demonstrate that the proposed method significantly outperforms existing techniques, improving centroid extraction accuracy by up to 59.64% and pointing accuracy across all axes by more than 78.94%.

Key words: Heterogeneous blur kernel estimation; Dynamic conditions; Regional image restoration; Multiplication extended Kalman filter; Gyro drift

Chinese Summary  <0> 基于异质模糊核的乘性扩展卡尔曼滤波辅助非盲星图像复原算法

刘洋1,2,3,邓华健1,王昊1,2,3,金仲和1,2,3
1浙江大学微小卫星研究中心,中国杭州市,310027
2浣江实验室,中国诸暨市,311899
3浙江省微纳卫星研究重点实验室,中国杭州市,310027
摘要:在动态条件下,星斑在成像平面上的模糊效应会降低质心提取精度,从而影响姿态估算。为提升星敏感器的动态性能,提出一种基于异质模糊核的乘性扩展卡尔曼滤波(MEKF)辅助非盲星图像复原算法。该算法包含3个步骤:首先,采用MEKF估计姿态和陀螺漂移,以消除星敏感器测量误差和陀螺漂移。其次,利用MEKF预测的姿态作为初始条件,加速后续算法运行。最后,提出一种陀螺辅助异质模糊核估计算法,用于恢复非均匀与非线性运动模糊的星图。与现有动态星像去模糊算法主要关注图像内容不同,本方法着眼于运动模糊的成因,融合MEKF和异质模糊核技术。这显著增强了对噪声的鲁棒性并提高了复原精度。仿真结果表明,该方法显著优于现有技术,将质心提取精度提升高达59.64%,并将各轴指向精度提高78.94%以上。

关键词组:异质模糊核估计;动态环境;局部图像复原;乘性扩展卡尔曼滤波;陀螺漂移


Share this article to: More

Go to Contents

References:

<Show All>

Open peer comments: Debate/Discuss/Question/Opinion

<1>

Please provide your name, email address and a comment





DOI:

10.1631/FITEE.2500193

CLC number:

TP391.41;V448.22

Download Full Text:

Click Here

Downloaded:

234

Clicked:

419

Cited:

0

On-line Access:

2025-11-17

Received:

2025-03-29

Revision Accepted:

2025-11-18

Crosschecked:

2025-06-10

Journal of Zhejiang University-SCIENCE, 38 Zheda Road, Hangzhou 310027, China
Tel: +86-571-87952276; Fax: +86-571-87952331; E-mail: jzus@zju.edu.cn
Copyright © 2000~ Journal of Zhejiang University-SCIENCE