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20112026
most citedDifferential Emission Measure Analysis of Multiple Structural Components of Coronal Mass Ejections in the Inner Corona

271 citations · 1.6k across the 38 of their papers we have counts for

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Showing 2023Show all

7 papers · 1 filter

astro-ph.SR2023★ 14 cited

A Statistical Study of Soft X-ray Flares on Solar-type Stars

Zhanhao Zhao, Ziqian Hua, Xin Cheng +2

The statistical characteristic of stellar flares at optical bands has received an extensive study, but it remains to be studied at soft X-ray bands, in particular for solar-type st…

astro-ph.SR2023★ 6 cited

A Method for Determining the Locations and Configurations of Magnetic Reconnection within 3D Turbulent Plasmas

Yulei Wang, Xin Cheng, Yang Guo +2

Context. Three-dimensional (3D) reconnection is an important mechanism for efficiently releasing energy during astrophysical eruptive events, which is difficult to be quantitativel…

astro-ph.SR2023

Identifying Footpoints of Pre-eruptive and Coronal Mass Ejection Flux Ropes with Sunspot Scars

Chen Xing, Guillaume Aulanier, Brigitte Schmieder +2

The properties of pre-eruptive structures and coronal mass ejections (CMEs) are characterized by those of their footpoints, the latter of which thus attract great interest. However…

astro-ph.SR2023

Spectral Features of the Solar Transition Region and Chromospheric Lines at Flare Ribbons Observed with IRIS

Lingfang Wang, Ying Li, Qiao Li +2

We report on the spectral features of the Si IV 1402.77 Å, C II 1334.53 Å, and Mg II h or k lines, formed in the layers from the transition region to the chromosphere, in three two…

astro-ph.SR2023★ 25 cited

Three-dimensional Turbulent Reconnection within Solar Flare Current Sheet

Yulei Wang, Xin Cheng, Mingde Ding +3

Solar flares can release coronal magnetic energy explosively and may impact the safety of near-earth space environments. Their structures and properties on macroscale have been int…

astro-ph.SR2023★ 24 cited

A Model for Confined Solar Eruptions Including External Reconnection

Jun Chen, Xin Cheng, Bernhard Kliem +1

The violent disruption of the coronal magnetic field is often observed to be restricted to the low corona, appearing as a confined eruption. The possible causes of the confinement…