activity
20062023
most citedAdversarial Attack and Defense on Graph Data: A Survey

293 citations · 1.5k across the 77 of their papers we have counts for

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Showing astro-ph.SRShow all

8 papers · 1 filter

astro-ph.SR2022★ 8 cited

Three-Dimensional Propagation of Kink Wave Trains in Solar Coronal Slabs

Bo Li, Mingzhe Guo, Hui Yu +2

Impulsively excited wave trains are of considerable interest in solar coronal seismology. To our knowledge, however, it remains to examine the three-dimensional (3D) dispersive pro…

astro-ph.SR2022★ 8 cited

Impulsively Generated Kink Wave Trains in Solar Coronal Slabs

Mingzhe Guo, Bo Li, Tom Van Doorsselaere +1

We numerically follow the response of density-enhanced slabs to impulsive, localized, transverse velocity perturbations by working in the framework of ideal magnetohydrodynamics (M…

astro-ph.SR2022★ 10 cited

Standing Sausage Perturbations in solar coronal loops with diffuse boundaries: An initial-value-problem perspective

Bo Li, Shao-Xia Chen, Ao-Long Li

Working in pressureless magnetohydrodynamics, we examine the consequences of some peculiar dispersive properties of linear fast sausage modes (FSMs) in one-dimensional cylindrical…

astro-ph.SR2021★ 9 cited

Forward Modeling of Simulated Transverse Oscillations in Coronal Loops and the Influence of Background Emission

Mijie Shi, Tom Van Doorsselaere, Patrick Antolin +1

We simulate transverse oscillations in radiatively cooling coronal loops and forward-model their spectroscopic and imaging signatures, paying attention to the influence of backgrou…

astro-ph.SR2020★ 10 cited

Mixed properties of magnetohydrodynamic waves undergoing resonant absorption in the cusp continuum

Marcel Goossens, Shao-Xia Chen, Michaël Geeraerts +2

Observations of magnetohydrodynamic (MHD) waves in the structured solar atmosphere have shown that these waves are damped and can thus contribute to atmospheric heating. In this pa…

astro-ph.SR2020★ 15 cited

How eruptions of a small filament feed materials to a nearby larger-scaled filament

Hengyuan Wei, Zhenghua Huang, Zhenyong Hou +4

As one of the most common features in the solar atmosphere, filaments are significant not only in the solar physics but also in the stellar and laboratory plasma physics. With the…