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Photospheric Magnetic Activities Responsible for Soft X‐Ray Pointlike Microflares. I. Identifications of Associated Photospheric/Chromospheric Activities
Transverse Gradients of Longitudinal Magnetic Field in Active Regions with Different Levels of Flare Productivity. I. Calculation Methods and Dynamics of Selected Parameters
Response to “Comment on ‘Resolving the 180° Ambiguity in Solar Vector Magnetic Field Data: Evaluating the Effects of Noise, Spatial Resolution, and Method Assumptions’ ”
Effects of Field-Aligned Flows on Standing Kink and Sausage Modes Supported by Coronal Loops
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