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20222026
most citedWhere and how does a decay-index profile become saddle-like?

13 citations · 13 across the 1 of their papers we have counts for

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astro-ph.SR2026

What Causes the Asymmetry of Conjugate Hard X-Ray Footpoints in Solar Flares?

Mirabbos Mirkamalov, Rui Liu, Runbin Luo +1

Hard X-ray (HXR) emission in solar flares critically diagnoses nonthermal electron acceleration, transport, and precipitation. Observations commonly show asymmetric HXR photon flux…

astro-ph.SR2025

High-Resolution Observation of Solar Prominence Plumes Induced by Enhanced Spicular Activity

Wensi Wang, Rui Liu, Runbin Luo +1

Solar prominences are the most prominent large-scale structures observed above the solar limb in emission in chromospheric lines but in absorption in coronal lines. At the bottom o…

astro-ph.SR20251 cited

Falling Threads During Solar Filament Eruptions

Yidian Wu, Rui Liu, Runbin Luo +1

Mass drainage is frequently observed in solar filaments. During filament eruptions, falling material most likely flows along magnetic field lines, which may provide important clues…

astro-ph.SR2024

High-resolution Observation of Blowout Jets Regulated by Sunspot Rotation

Tingyu Gou, Rui Liu, Yang Su +4

Coronal jets are believed to be the miniature version of large-scale solar eruptions. In particular, the eruption of a mini-filament inside the base arch is suggested to be the tri…

astro-ph.SR202213 cited

Where and how does a decay-index profile become saddle-like?

Runbin Luo, Rui Liu

The decay index of solar magnetic fields is known as an important parameter in regulating solar eruptions from the standpoint of the torus instability. In particular, a saddle-like…