浅海声源深度判决的正交子空间方法
Source depth discrimination based on the orthogonal subspace in shallow water
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摘要: 针对浅水环境中的水面水下目标分辨问题, 提出一种基于正交子空间的深度判决方法。通过凸优化方法对陷波子空间进行预处理, 以去除干扰项提高子空间能量的估计精度。使用Schimidt正交构建正交的陷波分量和自由分量子空间, 保留了完整的模态空间以增加参与判决的模态信息。通过仿真分析了信噪比和垂直孔径对各方法性能的影响, 结果表明所提方法在阵列垂直孔径较小时的深度判决性能优于作为对比方法的匹配子空间判决器和基于正则最小二乘的模态滤波器。最后, 利用浅海实验获得的数据对该方法进行了验证。数据结果表明, 信噪比为7~16 dB时, 在阵列孔径为0.16倍环境水深的情况下, 所提方法仍可实现对水面和水下目标的分辨, 正确分辨率高于对比方法。Abstract: A solution based on the orthogonal subspace to the problem of source depth discrimination in a downward refracting shallow water waveguide is presented for the case of a limited vertical line array. The trapped subspace is preprocessed by convex optimization to remove the interference terms and improve the estimation accuracy of the subspace energy. The Schmidt orthogonalization is applied to construct orthogonal subspaces of the trapped and free components, preserving the complete mode space to increase the mode information involved in the source depth discrimination. The performance is predicted with simulations, allowing one to compare the proposed and reference methods. The effects of signal-to-noise ratio and the vertical aperture on the performance are numerically investigated, and the results show that the proposed method is more robust than the matched subspace discriminator and the regular least squares-based mode filter, which are used as reference methods, for a limited-vertical aperture case. Finally, the approach is validated on experimental data collected with a vertical line array deployed in a shallow sea experiment. The results show that with signal-to-noise ratio ranging from 7 dB to 16 dB, the proposed method can still discriminate the surface and submerged sources at an array aperture of 0.16 times the water depth with higher correct discrimination rates than the reference methods.
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