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一种无需任何先验知识的多光谱温度场超稀疏层析成像重建方法。

An Extremely Sparse Tomography Reconstruction of a Multispectral Temperature Field without Any a Priori Knowledge.

作者信息

Zhang Xuan, Han Yan

机构信息

School of Information and Communication Engineering, North University of China, Taiyuan 030051, China.

Shanxi Key Laboratory of Signal Capturing & Processing, North University of China, Taiyuan 030051, China.

出版信息

Sensors (Basel). 2024 Aug 14;24(16):5264. doi: 10.3390/s24165264.

DOI:10.3390/s24165264
PMID:39204959
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC11360723/
Abstract

When undertaking optical sparse projection reconstruction, the reconstruction of the tested field often requires the utilization of a priori knowledge to compensate for the lack of information due to the sparse projection angle. In order to reconstruct the radiation field of unknown materials or in situations where a priori knowledge cannot be obtained, this paper proposes an extremely sparse tomography multispectral temperature field reconstruction algorithm that analyzes the similarity (the similarity here compares and calculates the Euclidean distance of the spectral emissivity values at various wavelengths between different spectral curves) of radiation characteristics of materials under the same pressure and concentration but different temperature, describes the similarity between the radiation information of the tested field using the dynamic time warping (DTW) algorithm, and uses the similarity sum of the radiation information among the subregions of the temperature field as the optimization objective. This is combined with the equation-constrained optimization algorithm and multispectral thermometry to establish the statistical law between the missing information and finally realize the reconstruction of the temperature field. Simulation experiments show that, without any a priori knowledge, the method in this paper can realize reconstruction of the temperature field with an accuracy of 1.53-12.05% under two projection angles and has fewer projection angles and stronger robustness than other methods.

摘要

在进行光学稀疏投影重建时,被测场的重建通常需要利用先验知识来弥补由于稀疏投影角度导致的信息不足。为了重建未知材料的辐射场或在无法获取先验知识的情况下,本文提出了一种极稀疏层析多光谱温度场重建算法,该算法分析了相同压力、浓度但不同温度下材料辐射特性的相似性(这里的相似性是比较并计算不同光谱曲线在各波长处的光谱发射率值的欧几里得距离),利用动态时间规整(DTW)算法描述被测场辐射信息之间的相似性,并将温度场子区域间辐射信息的相似性总和作为优化目标。将其与方程约束优化算法和多光谱测温法相结合,建立缺失信息之间的统计规律,最终实现温度场的重建。仿真实验表明,在没有任何先验知识的情况下,本文方法在两个投影角度下能够以1.53 - 12.05%的精度实现温度场重建,且与其他方法相比,所需投影角度更少,鲁棒性更强。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/7900/11360723/303427103e7a/sensors-24-05264-g012.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/7900/11360723/99d24438c467/sensors-24-05264-g001.jpg
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https://cdn.ncbi.nlm.nih.gov/pmc/blobs/7900/11360723/29612a0c9923/sensors-24-05264-g003a.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/7900/11360723/3731fa247a29/sensors-24-05264-g004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/7900/11360723/8b46b05b05df/sensors-24-05264-g005.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/7900/11360723/d9ec80c248ec/sensors-24-05264-g006.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/7900/11360723/5a7d16a78d0b/sensors-24-05264-g007.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/7900/11360723/4e6a61c8d9df/sensors-24-05264-g008.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/7900/11360723/d7f9097d181c/sensors-24-05264-g009.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/7900/11360723/d81766446237/sensors-24-05264-g010.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/7900/11360723/2c1e58f82197/sensors-24-05264-g011.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/7900/11360723/303427103e7a/sensors-24-05264-g012.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/7900/11360723/99d24438c467/sensors-24-05264-g001.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/7900/11360723/f079f3cfdf40/sensors-24-05264-g002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/7900/11360723/29612a0c9923/sensors-24-05264-g003a.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/7900/11360723/3731fa247a29/sensors-24-05264-g004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/7900/11360723/8b46b05b05df/sensors-24-05264-g005.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/7900/11360723/d9ec80c248ec/sensors-24-05264-g006.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/7900/11360723/5a7d16a78d0b/sensors-24-05264-g007.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/7900/11360723/4e6a61c8d9df/sensors-24-05264-g008.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/7900/11360723/d7f9097d181c/sensors-24-05264-g009.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/7900/11360723/d81766446237/sensors-24-05264-g010.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/7900/11360723/2c1e58f82197/sensors-24-05264-g011.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/7900/11360723/303427103e7a/sensors-24-05264-g012.jpg

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