activity
20142026
most citedWhy is a flare-rich active region CME-poor?

57 citations · 387 across the 27 of their papers we have counts for

collaborators
Showing 2021Show all

5 papers · 1 filter

astro-ph.SR2021★ 9 cited

Confined and eruptive catastrophes of solar magnetic flux ropes caused by mass loading and unloading

Quanhao Zhang, Rui Liu, Yuming Wang +2

It is widely accepted that coronal magnetic flux ropes are the core structures of large-scale solar eruptive activities, which inflict dramatic impacts on the solar-terrestrial sys…

astro-ph.SR2021★ 9 cited

Energy Partition in Four Confined Circular-Ribbon Flares

Z. M. Cai, Q. M. Zhang, Z. J. Ning +2

In this study, we investigated the energy partition of four confined circular-ribbon flares (CRFs) near the solar disk center, which are observed simultaneously by SDO, GOES, and R…

astro-ph.SR2021★ 3 cited

How flux feeding causes eruptions of solar magnetic flux ropes with the hyperbolic flux tube configuration?

Quanhao Zhang, Rui Liu, Yuming Wang +3

Coronal magnetic flux ropes are generally considered to be the core structure of large-scale solar eruptions. Recent observations found that solar eruptions could be initiated by a…

astro-ph.SR2021★ 4 cited

Population of Bright Plume Threads in Solar Polar Coronal Holes

Zhenghua Huang, Quanhao Zhang, Lidong Xia +8

Coronal holes are well accepted to be source regions of the fast solar wind. As one of the common structures in coronal holes, coronal plumes might contribute to the origin of the…

astro-ph.SR2021★ 9 cited

Three-dimensional Reconstruction of Coronal Mass Ejections by CORAR Technique through Different Stereoscopic Angle of STEREO Twin Spacecraft

Shaoyu Lyu, Yuming Wang, Xiaolei Li +3

Recently, we developed the Correlation-Aided Reconstruction (CORAR) method to reconstruct solar wind inhomogeneous structures, or transients, using dual-view white-light images (Li…