Academic Journal

Mapping Solar X-Ray Images from SDO/AIA EUV Images by Deep Learning

التفاصيل البيبلوغرافية
العنوان: Mapping Solar X-Ray Images from SDO/AIA EUV Images by Deep Learning
المؤلفون: Hong JC(洪俊超), Liu H(刘辉), Bi Y(毕以), Xu, Zhe, Yang B(杨波), Yang JY(杨家艳), Su, Yang, Xia, Yuehan, Ji KF(季凯帆)
بيانات النشر: IOP PUBLISHING LTD
سنة النشر: 2021
المجموعة: Yunnan Observatories: YNAO OpenIR (Chinese Academy of Sciences, CAS) / 中国科学院云南天文台机构知识库
مصطلحات موضوعية: 天文学, 天文学::太阳与太阳系, 天文学::太阳与太阳系::太阳物理学, 计算机科学技术, 计算机科学技术::人工智能, 计算机科学技术::计算机应用, 理学, 理学::天文学, Astronomy & Astrophysics, ERUPTIONS, JETS
الوصف: The full-Sun corona is now imaged every 12 s in extreme ultraviolet (EUV) passbands by Solar Dynamics Observatory/Atmospheric Imaging Assembly (AIA), whereas it is only observed several times a day at X-ray wavelengths by Hinode/X-Ray Telescope (XRT). In this paper, we apply a deep-learning method, i.e., the convolution neural network (CNN), to establish data-driven models to generate full-Sun X-ray images in XRT filters from AIA EUV images. The CNN models are trained using a number of data pairs of AIA six-passband (171, 193, 211, 335, 131, and 94 angstrom) images and the corresponding XRT images in three filters: Al_mesh, Ti_poly, and Be_thin. It is found that the CNN models predict X-ray images in good consistency with the corresponding well-observed XRT data. In addition, the purely data-driven CNN models are better than the conventional analysis method of the coronal differential emission measure (DEM) in predicting XRT-like observations from AIA data. Therefore, under conditions where AIA provides coronal EUV data well, the CNN models can be applied to fill the gap in limited full-Sun coronal X-ray observations and improve pool-observed XRT data. It is also found that DEM inversions using AIA data and our deep-learning-predicted X-ray data jointly are better than those using AIA data alone. This work indicates that deep-learning methods provide the opportunity to study the Sun based on virtual solar observation in future.
نوع الوثيقة: article in journal/newspaper
report
اللغة: English
Relation: ASTROPHYSICAL JOURNAL; http://ir.ynao.ac.cn/handle/114a53/24453; https://dx.doi.org/10.3847/1538-4357/ac01d5
DOI: 10.3847/1538-4357/ac01d5
الاتاحة: http://ir.ynao.ac.cn/handle/114a53/24453
https://doi.org/10.3847/1538-4357/ac01d5
Rights: cn.org.cspace.api.content.CopyrightPolicy@78d702ba
رقم الانضمام: edsbas.A8C8867F
قاعدة البيانات: BASE
الوصف
DOI:10.3847/1538-4357/ac01d5