activity
20162024
most citedDo All Interplanetary Coronal Mass Ejections Have A Magnetic Flux Rope Structure Near 1 AU?

18 citations · 123 across the 12 of their papers we have counts for

collaborators

19 papers

astro-ph.SR2024

Failure of a solar filament eruption caused by magnetic reconnection with overlying coronal loops

Leping Li, Hongqiang Song, Yijun Hou +11

Failure of a filament eruption caused by magnetic reconnection between the erupting filament and the overlying magnetic field has been previously proposed in numerical simulations.…

astro-ph.SR2024

Three types of solar coronal rain during magnetic reconnection between open and closed magnetic structures

Fangfang Qiao, Leping Li, Hui Tian +4

Coronal rain (CR) is a crucial part of the mass cycle between the corona and chromosphere. It includes the flare-driven CR and two types of quiescent CR separately along the non-fl…

astro-ph.SR202112 cited

Formation of a solar filament by magnetic reconnection and coronal condensation

Leping Li, Hardi Peter, Lakshmi Pradeep Chitta +1

In solar filament formation mechanisms, magnetic reconnection between two sets of sheared arcades forms helical structures of the filament with numerous magnetic dips, and cooling…

astro-ph.SR20211 cited

The Inhomogeneity of Composition along the Magnetic Cloud Axis

Hongqiang Song, Qiang Hu, Xin Cheng +6

It is generally accepted that CMEs result from eruptions of magnetic flux ropes, which are dubbed as magnetic clouds in interplanetary space. The composition (including the ionic c…

astro-ph.SR202117 cited

Solar Cycle Dependence of ICME Composition

Hongqiang Song, Leping Li, Yanyan Sun +3

Coronal mass ejections (CMEs) are one of the most energetic explosions in the solar atmosphere, and their occurrence rates exhibit obvious solar cycle dependence with more events t…

astro-ph.SR202116 cited

On-disk solar coronal condensations facilitated by magnetic reconnection between open and closed magnetic structures

Leping Li, Hardi Peter, Lakshmi Pradeep Chitta +1

Coronal condensation and rain are a crucial part of the mass cycle between the corona and chromosphere. In some cases, condensation and subsequent rain originate in the magnetic di…