Active Region Detection in Multi-spectral Solar Images

Majedaldein Almahasneh, A. Paiement, Xianghua Xie, J. Aboudarham
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引用次数: 2

Abstract

Precisely detecting solar Active Regions (AR) from multi-spectral images is a challenging task yet important in understanding solar activity and its influence on space weather. A main challenge comes from each modality capturing a different location of these 3D objects, as opposed to more traditional multi-spectral imaging scenarios where all image bands observe the same scene. We present a multi-task deep learning framework that exploits the dependencies between image bands to produce 3D AR detection where different image bands (and physical locations) each have their own set of results. We compare our detection method against baseline approaches for solar image analysis (multi-channel coronal hole detection, SPOCA for ARs (Verbeeck et al., 2013)) and a state-of-the-art deep learning method (Faster RCNN) and show enhanced performances in detecting ARs jointly from multiple bands.
太阳多光谱图像的活动区域检测
从多光谱图像中精确探测太阳活动区(AR)是一项具有挑战性的任务,但对于了解太阳活动及其对空间天气的影响至关重要。一个主要的挑战来自于每种模式捕获这些3D物体的不同位置,而不是更传统的多光谱成像场景,所有图像带观察相同的场景。我们提出了一个多任务深度学习框架,利用图像波段之间的依赖关系来产生3D AR检测,其中不同的图像波段(和物理位置)每个都有自己的一组结果。我们将我们的检测方法与太阳图像分析的基线方法(多通道日冕洞检测,用于ar的SPOCA (Verbeeck等人,2013))和最先进的深度学习方法(Faster RCNN)进行了比较,并在多波段联合检测ar方面显示出增强的性能。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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