Machine Learning for Astronomical Big Data Processing

被引:0
|
作者
Xu, Long [1 ]
Yan, Yihua [1 ]
机构
[1] Chinese Acad Sci, Key Lab Solar Act, Natl Astron Observ, Beijing, Peoples R China
基金
中国国家自然科学基金;
关键词
Solar radio astronomy; deep learning; classification; regression; machine learning; FLARE DETECTION; ALGORITHM;
D O I
暂无
中图分类号
TM [电工技术]; TN [电子技术、通信技术];
学科分类号
0808 ; 0809 ;
摘要
Recently, more and more high resolution, high precision telescopes have been developing in the world, such as SKA[1], Arecibo[2], ALMA[2], Muser[4][5]. By aid of these modern telescopes, human acquired more and in-depth knowledge about the universe; meanwhile, a "big data" challenge was raised for astronomical big data processing. For example, the MingantU SpEctral Radioheliograph (Muser) records about 100TB raw data per month for solar radio observation. The big data firstly causes a big challenge for archiving and classifying recorded data, especially as we need the fast processing of daily recorded data. The traditional data processing was usually implemented manually before the emergence of big data, so it is no longer applicable to current big data. It is urgent to develop automatic algorithms for processing the daily recorded data efficiently and timely. Secondly, the big data also cause great difficulty in the storage and transmission of data, so data compression is highly desirable. This paper reports our efforts on big data archiving, classification and activity forecast by using machine learning, especially deep learning.
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页数:4
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