太阳耀斑分级识别最优性能的研究

Q4 Computer Science
Aditya Kakde, Durgansh Sharma, B. Kaushik, N. Arora
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引用次数: 2

摘要

当太阳出现短暂的强烈亮度时,我们就可以说太阳耀斑出现了。由于太阳耀斑是由高能光子和粒子组成的,因此会产生强电场和强电流,从而导致天基或地面技术系统的中断。提取其重要特征用于预测也成为一项具有挑战性的任务。卷积神经网络在分类和定位任务中得到了广泛的应用。本文着重对不同年份出现的太阳耀斑进行了分类,通过叠加不同的卷积层,再加上最大池化层。从Alexnet的参考资料来看,本文采用的池化层是重叠池化。此外,我们还使用了两个不同的激活函数ELU和CReLU来研究具有特定激活函数的卷积层的数量在这个数据集上提供了最好的结果,因为这个领域的数据集的大小总是很小。该研究可进一步应用于一种新的太阳活动预测系统。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Investigation of Solar Flare Classification to Identify Optimal Performance
When an intense brightness for a small amount of time is seen in the sun, then we can say that a solar flare emerged. As solar flares are made up of high energy photons and particles, thus causing the production of high electric fields and currents and therefore results in the disruption in space-borne or ground-based technological system. It also becomes a challenging task to extract its important features for prediction. Convolutional Neural Networks have gain a significant amount of popularity in the classification and localization tasks. This paper has given stress on the classification of the solar flares emerged on different years by stacking different convolutional layers followed by max pooling layers. From the reference of Alexnet, the pooling layer employed in this paper is the overlapping pooling. Also two different activation functions that are ELU and CReLU have been used to investigate how many number of convolutional layers with a particular activation function provides with the best results on this dataset as the size of the dataset in this domain is always small. The proposed investigation can be further used in a novel solar prediction systems.
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来源期刊
Electronic Letters on Computer Vision and Image Analysis
Electronic Letters on Computer Vision and Image Analysis Computer Science-Computer Vision and Pattern Recognition
CiteScore
2.50
自引率
0.00%
发文量
19
审稿时长
12 weeks
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