Research Progress on Detection of Coronal Mass Ejection

Guo Min; Shang Zhenhong; Qiang Zhenping; Li Jingtao; Xian Xianggui; Yang Zhipeng

Astronomical Research and Technology > 2020 > 17(1): 39-51.

Guo Min, Shang Zhenhong, Qiang Zhenping, Li Jingtao, Xian Xianggui, Yang Zhipeng. Research Progress on Detection of Coronal Mass Ejection[J]. Astronomical Research and Technology, 2020, 17(1): 39-51.

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Research Progress on Detection of Coronal Mass Ejection

1. Faculty of Information Engineering and Automation, Kunming University of Science and Technology, Kunming 650500, China;
2. College of Big Data and Intelligent Engineering, Southwest Forestry University, Kunming 650224, China

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Received Date: May 16, 2019
Revised Date: June 11, 2019
Available Online: November 20, 2023

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Abstract

Abstract

A Coronal Mass Ejection (CME) is a large-scale, severely explosive phenomenon that is the main solar outburst affecting the Earth. As this kind of explosion will cause serious interference to the terrestrial environment, detecting CMEs is of great significance for forecasting severe space weather. In order to more clearly sort out the existing CME detection methods, this paper analyzes and summarizes the typical methods. Firstly,CMEs and their characteristics are introduced. Then, CMEs detection methods are summarized and analyzed from two aspects:manual methods and automatic methods. Finally, problems of the current algorithms are discussed and the future research direction is proposed.
- Solar burst activity,
- Corona material,
- CME detection

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References (33)

References

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