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

27 papers

astro-ph.SR2026

The coronal mass ejection productivity of solar active region 13664/8

Lijuan Liu, Yuming Wang, Quanhao Zhang +2

In May 2024, NOAA active region (AR) complex 13664/8 was one of the most productive regions of the current solar cycle, producing 12 X-class flares and over 20 coronal mass ejectio…

astro-ph.EP2026

Jovian Zonal Winds Revealed from Cassini/VIMS Observations

Shenghan Ma, Yuming Wang, Tao Li +3

Understanding Jupiter's zonal winds is crucial to unraveling the dynamics of its atmosphere. Over the last decades, multiple data sources and techniques have been used to study zon…

astro-ph.SR2025

Solar magnetic flux rope eruptions caused by inverse flux feeding processes

Quanhao Zhang, Shangbin Yang, Rui Liu +6

Large-scale solar eruptions are generally accepted to have coronal magnetic flux ropes as their core structures. Recent studies found that the solar eruptions could be initiated by…

astro-ph.SR2025

Minifilament Eruptions as the Last Straw to Break the Equilibrium of a Giant Solar Filament

Hechao Chen, Hui Tian, Quanhao Zhang +8

Filament eruptions are magnetically driven violent explosions commonly observed on the Sun and late-type stars, sometimes leading to monster coronal mass ejections that directly af…

astro-ph.SR2022

Influence of magnetic reconnection on the eruptive catastrophes of coronal magnetic flux ropes

Quanhao Zhang, Xin Cheng, Rui Liu +3

Large-scale solar eruptive activities have a close relationship with coronal magnetic flux ropes. Previous numerical studies have found that the equilibrium of a coronal flux rope…

astro-ph.SR2022★ 21 cited

Solar Ring Mission: Building a Panorama of the Sun and Inner-heliosphere

Yuming Wang, Xianyong Bai, Changyong Chen +50

Solar Ring (SOR) is a proposed space science mission to monitor and study the Sun and inner heliosphere from a full 360° perspective in the ecliptic plane. It will deploy three 120…

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…

astro-ph.SR2020★ 13 cited

Cause and Kinematics of a Jet-Like CME

Reetika Joshi, Yuming Wang, Ramesh Chandra +3

In this article, we present the multi-viewpoint and multi-wavelength analysis of an atypical solar jet based on the data from Solar Dynamics Observatory, SOlar, and Heliospheric Ob…

astro-ph.SR2020★ 19 cited

Eruption of Solar Magnetic Flux Ropes Caused by Flux Feeding

Quanhao Zhang, Yuming Wang, Rui Liu +5

Large-scale solar eruptions are believed to have a magnetic flux rope as the core structure. However, it remains elusive as to how the flux rope builds up and what triggers its eru…

astro-ph.SR2020★ 11 cited

Reconstructing solar wind inhomogeneous structures from stereoscopic observations in white-light: Solar wind transients in 3D

Xiaolei Li, Yuming Wang, Rui Liu +7

White-light images from Heliospheric Imager-1 (HI1) onboard the Solar Terrestrial Relations Observatory (STEREO) provide 2-dimensional (2D) global views of solar wind transients tr…

astro-ph.SR2020★ 30 cited

Concept of the Solar Ring Mission: Overview

Yuming Wang, Haisheng Ji, Yamin Wang +10

The concept of the Solar Ring mission was gradually formed from L5/L4 mission concept, and the proposal of its pre-phase study was funded by the National Natural Science Foundation…

astro-ph.SR2018★ 21 cited

Unraveling the Links among Sympathetic Eruptions

Dong Wang, Rui Liu, Yuming Wang +4

Solar eruptions occurring at different places within a relatively short time interval are considered to be sympathetic. However, it is difficult to determine whether there exists a…

astro-ph.SR2018★ 14 cited

Reconstructing solar wind inhomogeneous structures from stereoscopic observations in white-light: Small transients along the Sun-Earth line

Xiaolei Li, Yuming Wang, Rui Liu +5

The Heliospheric Imagers (HI) on board the two spacecraft of the Solar Terrestrial Relations Observatory (STEREO) provided white-light images of transients in the solar wind from d…

astro-ph.SR2017★ 3 cited

Upward and downward catastrophes of coronal magnetic flux ropes in quadrupolar magnetic fields

Quanhao Zhang, Yuming Wang, Youqiu Hu +3

Coronal magnetic flux ropes are closely related to large-scale solar activities. Using a 2.5-dimensional time-dependent ideal magnetohydrodynamic (MHD) model in Cartesian coordinat…

astro-ph.SR2017★ 20 cited

The causes of quasi-homologous CMEs

Lijuan Liu, Yuming Wang, Rui Liu +8

In this paper, we identified the magnetic source locations of 142 quasi- homologous (QH) coronal mass ejections (CMEs), of which 121 are from solar cycle (SC) 23 and 21 from SC 24.…

astro-ph.SR2016★ 8 cited

On the Observation and Simulation of Solar Coronal Twin Jets

Jiajia Liu, Fang Fang, Yuming Wang +3

We present the first observation, analysis and modeling of solar coronal twin jets, which occurred after a preceding jet. Detailed analysis on the kinetics of the preceding jet rev…

physics.space-ph2016★ 42 cited

On the Propagation of a Geoeffective Coronal Mass Ejection during March 15 -- 17, 2015

Yuming Wang, Quanhao Zhang, Jiajia Liu +11

The largest geomagnetic storm so far in the solar cycle 24 was produced by a fast coronal mass ejection (CME) originating on 2015 March 15. It was an initially west-oriented CME an…

astro-ph.SR2016★ 57 cited

Why is a flare-rich active region CME-poor?

Lijuan Liu, Yuming Wang, Jingxiu Wang +6

Solar active regions (ARs) are the major sources of two kinds of the most violent solar eruptions, namely flares and coronal mass ejections (CMEs). The largest AR in the past 24 ye…

astro-ph.SR2016★ 11 cited

Downward catastrophe of solar magnetic flux ropes

Quanhao Zhang, Yuming Wang, Youqiu Hu +1

2.5D time-dependent ideal magnetohydrodynamic (MHD) models in Cartesian coordinates were used in previous studies to seek MHD equilibria involving a magnetic flux rope embedded in…

astro-ph.SR2016★ 5 cited

Damped large amplitude oscillations in a solar prominence and a bundle of coronal loops

Quanhao Zhang, Yuming Wang, Rui Liu +7

We investigate the evolutions of two prominences (P1,P2) and two bundles of coronal loops (L1,L2), observed with SDO/AIA near the east solar limb on 2012 September 22. It is found…