SRCVMar 13, 2015

Image patch analysis of sunspots and active regions. I. Intrinsic dimension and correlation analysis

arXiv:1503.04127v22 citations
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This work provides incremental improvements in solar physics by offering quantitative descriptors for active region complexity, aiding in more systematic studies of solar flare prediction.

The authors tackled the problem of quantifying the spatial complexity of solar active regions to better predict flare productivity, finding relationships between Mount Wilson classifications and intrinsic dimension measures, and identifying third-order Markov structures in partial correlation patterns.

The flare-productivity of an active region is observed to be related to its spatial complexity. Mount Wilson or McIntosh sunspot classifications measure such complexity but in a categorical way, and may therefore not use all the information present in the observations. Moreover, such categorical schemes hinder a systematic study of an active region's evolution for example. We propose fine-scale quantitative descriptors for an active region's complexity and relate them to the Mount Wilson classification. We analyze the local correlation structure within continuum and magnetogram data, as well as the cross-correlation between continuum and magnetogram data. We compute the intrinsic dimension, partial correlation, and canonical correlation analysis (CCA) of image patches of continuum and magnetogram active region images taken from the SOHO-MDI instrument. We use masks of sunspots derived from continuum as well as larger masks of magnetic active regions derived from the magnetogram to analyze separately the core part of an active region from its surrounding part. We find the relationship between complexity of an active region as measured by Mount Wilson and the intrinsic dimension of its image patches. Partial correlation patterns exhibit approximately a third-order Markov structure. CCA reveals different patterns of correlation between continuum and magnetogram within the sunspots and in the region surrounding the sunspots. These results also pave the way for patch-based dictionary learning with a view towards automatic clustering of active regions.

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