Tracing Hα Fibrils through Bayesian Deep Learning

نویسندگان

چکیده

We present a new deep learning method, dubbed FibrilNet, for tracing chromospheric fibrils in Halpha images of solar observations. Our method consists data pre-processing component that prepares training from threshold-based tool, model implemented as Bayesian convolutional neural network probabilistic image segmentation with uncertainty quantification to predict fibrils, and post-processing containing fibril-fitting algorithm determine fibril orientations. The FibrilNet tool is applied high-resolution an active region (AR 12665) collected by the 1.6 m Goode Solar Telescope (GST) equipped high-order adaptive optics at Big Bear Observatory (BBSO). quantitatively assess comparing its those employed tool. experimental results major findings are summarized follows. First, (i.e., detected fibrils) two tools quite similar, demonstrating good capability FibrilNet. Second, finds more accurate smoother orientation angles than Third, faster maps produced not only provide quantitative way measure confidence on each fibril, but also help identify structures inferred through machine learning. Finally, we apply full-disk other observatories additional BBSO/GST, tool's usability diverse datasets.

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ژورنال

عنوان ژورنال: Astrophysical Journal Supplement Series

سال: 2021

ISSN: ['1538-4365', '0067-0049']

DOI: https://doi.org/10.3847/1538-4365/ac14b7