Ziyao Hu, Kaifan Ji, Xianyong Bai, Xiao Yang, Yuanyong Deng, Wei Duan, Zhenyong Hou, Zihao Yang
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引用次数: 0
摘要
极紫外(EUV)波段的太阳观测是太阳活动研究和空间天气预报的重要组成部分。SATech-01卫星上的太阳上过渡区成像仪(SUTRI)设计用于在Ne vii 46.5 nm光谱线(T = 0.5 MK)上拍摄太阳全盘图像。它于2022年发射,科学数据于2023年1月10日发布。本文介绍了对SUTRI数据进行数据预处理的方法,消除仪器固有的影响,使原始数据标准化,从而获得科学的数据。除了常见的数据处理步骤外,我们的流水线还包括校正CMOS成像相机的水平条纹。作为实验有效载荷,SUTRI没有图像稳定系统。因此,由于卫星平台指向精度有限,开发了一种多步迭代算法来精确对准一系列漂移图像。我们的方法可能不限于SUTRI;为今后的太阳极紫外望远镜数据处理提供参考。
Data Processing Pipeline of the SUTRI EUV Imager on the SATech-01 Satellite
Solar observations in extreme ultraviolet (EUV) wavelengths are a crucial component of solar activity research and space weather forecasting. The Solar Upper Transition Region Imager (SUTRI) on the SATech-01 satellite is designed to take full-disk solar images in the Ne vii 46.5 nm spectral line (T = 0.5 MK). It was launched in 2022 and the science data were released on January 10, 2023. In this article, we describe the data preprocessing method employed to SUTRI data to eliminate inherent instrument effects and standardize the raw data to obtain scientific data. Alongside common data processing steps, our pipeline includes correcting for horizontal stripes from the CMOS imaging camera. As an experiment payload, SUTRI does not have an image stabilization system. Thus, a multi-step iterative algorithm has been developed to precisely align series of drifted images due to the limited pointing accuracy of the satellite platform. Our method may not be limited to SUTRI; it also serves as a reference for future solar EUV telescope data processing.
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.