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Cited article:

Sympathetic Solar Eruption on 2024 February 9

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Breaking of Large-Scale Filament due to Magnetic Reconnection and Consequent Partial Eruption

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The Triggering Process of an X-class Solar Flare on a Small Quadrupolar Active Region

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Sympathetic Partial Filament Eruptions Caused by the Interaction between Two Nearby Filaments

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Magnetic Activity and Parameters of 43 Flare Stars in the GWAC Archive

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Partial Eruption of Solar Filaments. I. Configuration and Formation of Double-decker Filaments

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Oscillations and Mass Draining that Lead to a Sympathetic Eruption of a Quiescent Filament

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Dynamical Evolution of an Active-region Filament Driven by Magnetic Reconnection

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Sympathetic Standard and Blowout Coronal Jets Observed in a Polar Coronal Hole

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Imaging Evidence for Solar Wind Outflows Originating from a Coronal Mass Ejection Footpoint

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Dynamics Evolution of a Solar Active-region Filament from a Quasi-static State to Eruption: Rolling Motion, Untwisting Motion, Material Transfer, and Chirality

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