基于深度学习的新型 ASO-S/HXI 太阳硬 X 射线图像重建算法

IF 2.7 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Yuehan Xia, Yang Su, Hui Liu, Wenhui Yu, Zhentong Li, Wei Chen, Yu Huang, Weiqun Gan
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引用次数: 0

摘要

在过去和现在的太阳飞行任务中,大多数太阳硬 X 射线(HXR)成像仪都是通过傅立叶变换成像技术获得 X 射线图像的,这就需要采用适当的成像算法,从空间调制或时间调制信号中重建图像。在过去的 50 年中,针对不同仪器的特点开发了多种算法。在这项工作中,我们介绍了一种基于深度学习为先进天基太阳观测站(ASO-S)上的硬 X 射线成像仪(HXI)开发的新成像算法,以及该算法在模拟数据和观测数据方面的初步测试结果。我们首先创建了一个训练数据集,分别从模拟的单源、双源和环形源的 HXR 图像中获取调制数据,以及 HXI 子准直器的模式。然后,我们引入机器学习算法,建立了基于模式的深度学习网络模型:HXI_DLA,它可以直接从调制计数生成图像。用简单光源训练模型后,我们测试了简单光源、扩展光源和双光源成像动态范围的 DLA。最后,我们比较了从三个耀斑的 HXI 观测中重建的 CLEAN 和 DLA 图像。总之,这些成像测试表明,目前的 HXI_DLA 方法生成的图像结果与广泛使用的成像方法 CLEAN 生成的图像结果相当。在某些情况下,DLA 图像甚至略胜一筹。此外,HXI_DLA 的成像速度超快,而且不需要参数。虽然这只是向全面开发实用的 DLA 方法迈出的第一步,但测试表明了深度学习在太阳硬 X 射线成像领域的潜力。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
A New Solar Hard X-ray Image Reconstruction Algorithm for ASO-S/HXI Based on Deep Learning

Most solar hard X-ray (HXR) imagers in the past and current solar missions obtain X-ray images via Fourier transform imaging technology, which requires proper imaging algorithms to reconstruct images from spatially-modulated or temporally-modulated signals. A variety of algorithms have been developed during the last 50 years for the characteristics of respective instruments. In this work, we present a new imaging algorithm developed based on deep learning for the Hard X-ray Imager (HXI) onboard the Advanced Space-based Solar Observatory (ASO-S) and the preliminary test results of the algorithm with both simulated data and observations. We first created a training dataset by obtaining modulation data from simulated HXR images of single, double and loop-shaped sources, respectively, and the patterns of HXI sub-collimators. Then, we introduced machine-learning algorithm to develop a pattern-based deep learning network model: HXI_DLA, which can directly produce an image from modulation counts. After training the model with simple sources, we tested DLA for simple sources, extended sources, and double sources for imaging dynamic range. Finally, we compared CLEAN and DLA images reconstructed from HXI observations of three flares. Overall, these imaging tests revealed that the current HXI_DLA method produces comparable image result to those from the widely used imaging method CLEAN. In some cases, DLA images are even slightly better. Besides, HXI_DLA is super fast for imaging and parameter-free. Although this is only the first step towards a fully developed and practical DLA method, the tests have shown the potential of deep learning in the field of solar hard X-ray imaging.

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来源期刊
Solar Physics
Solar Physics 地学天文-天文与天体物理
CiteScore
5.10
自引率
17.90%
发文量
146
审稿时长
1 months
期刊介绍: Solar Physics was founded in 1967 and is the principal journal for the publication of the results of fundamental research on the Sun. The journal treats all aspects of solar physics, ranging from the internal structure of the Sun and its evolution to the outer corona and solar wind in interplanetary space. Papers on solar-terrestrial physics and on stellar research are also published when their results have a direct bearing on our understanding of the Sun.
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