A CME Automatic Detection Method Based on Adaptive Background Learning Technology

IF 1.6 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS Advances in Astronomy Pub Date : 2019-11-07 DOI:10.1155/2019/6582104
Z. Qiang, X. Bai, Qinghui Zhang, Hong Lin
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引用次数: 3

Abstract

In this paper, we describe a technique, which uses an adaptive background learning method to detect the CME (coronal mass ejections) automatically from SOHO/LASCO C2 image sequences. The method consists of several modules: adaptive background module, candidate CME area detection module, and CME detection module. The core of the method is based on adaptive background learning, where CMEs are assumed to be a foreground moving object outward as observed in running-difference time series. Using the static and dynamic features to model the corona observation scene can more accurately describe the complex background. Moreover, the method can detect the subtle changes in the corona sequences while filtering their noise effectively. We applied this method to a month of continuous corona images, compared the result with CDAW, CACTus, SEEDS, and CORIMP catalogs and found a good detection rate in the automatic methods. It detected about 73% of the CMEs listed in the CDAW CME catalog, which is identified by human visual inspection. Currently, the derived parameters are position angle, angular width, linear velocity, minimum velocity, and maximum velocity of CMES. Other parameters could also easily be added if needed.
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一种基于自适应背景学习技术的CME自动检测方法
在本文中,我们描述了一种技术,该技术使用自适应背景学习方法从SOHO/LASCO C2图像序列中自动检测日冕物质抛射。该方法由几个模块组成:自适应背景模块、候选CME区域检测模块和CME检测模块。该方法的核心是基于自适应背景学习,其中CME被假设为在运行差分时间序列中观察到的向外移动的前景对象。利用静态和动态特征对电晕观测场景进行建模,可以更准确地描述复杂的背景。此外,该方法可以检测电晕序列的细微变化,同时有效地滤除其噪声。我们将该方法应用于一个月的连续电晕图像,并将结果与CDAW、CACTus、SEEDS和CORIMP目录进行了比较,发现自动方法具有良好的检测率。它检测到了CDAW CME目录中约73%的CME,这是通过人类视觉检查确定的。目前导出的参数有CMES的位置角、角宽度、线速度、最小速度和最大速度。如果需要,也可以很容易地添加其他参数。
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来源期刊
Advances in Astronomy
Advances in Astronomy ASTRONOMY & ASTROPHYSICS-
CiteScore
2.70
自引率
7.10%
发文量
10
审稿时长
22 weeks
期刊介绍: Advances in Astronomy publishes articles in all areas of astronomy, astrophysics, and cosmology. The journal accepts both observational and theoretical investigations into celestial objects and the wider universe, as well as the reports of new methods and instrumentation for their study.
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