most citedThree-dimensional magnetic reconnection in astrophysical plasmas

40 citations

15 papers

astro-ph.SR2022★ 6 cited

The deformation of an erupting magnetic flux rope in a confined solar flare

Ruisheng Zheng, Yihan Liu, Liang Zhang +7

Magnetic flux ropes (MFRs), sets of coherently twisted magnetic field lines, are believed as core structures of various solar eruptions. Their evolution plays an important role to…

astro-ph.SR2022★ 21 cited

On the Nature of the Three-part Structure of Solar Coronal Mass Ejections

Hongqiang Song, Jie Zhang, Leping Li +4

Coronal mass ejections (CMEs) result from eruptions of magnetic flux ropes (MFRs) and can possess a three-part structure in white-light coronagraphs, including a bright front, dark…

astro-ph.SR2022★ 20 cited

Diagnostic functions of solar coronal magnetic fields from radio observations

Baolin Tan

In solar physics, it is a big challenge to measure the magnetic fields directly from observations in the upper solar atmosphere, including the chromosphere and corona. Radio observ…

astro-ph.SR2022★ 28 cited

Toward a Unified Explanation for the Three-part Structure of Solar Coronal Mass Ejections

Hongqiang Song, Leping Li, Yao Chen

Coronal mass ejections (CMEs) are associated with the eruption of magnetic flux ropes (MFRs), which usually appear as hot channels in active regions and coronal cavities in quiet-S…

astro-ph.SR2022★ 8 cited

Birth places of extreme ultraviolet waves driven by impingement of solar jets upon coronal loops

Liang Zhang, Ruisheng Zheng, Huadong Chen +1

Solar extreme ultraviolet (EUV) waves are large-scale propagating disturbances in the corona. It is generally believed that the vital key for the formation of EUV waves is the rapi…

astro-ph.SR2022★ 1 cited

Formation and Immediate Deformation of a Small Filament Through Intermittent Magnetic Interactions

Ruisheng Zheng, Liang Zhang, Changhui Rao +4

It is generally believed that filament formation involves a process of the accumulation of magnetic energy. However, in this paper we discuss the idea that filaments will not erupt…