activity
20152021
most citedChirality and Magnetic Configurations of Solar Filaments

117 citations · 237 across the 6 of their papers we have counts for

collaborators

6 papers

cond-mat.str-el2021★ 15 cited

Projection of Infinite- Hubbard Model and Algebraic Sign Structure

Yunqing Ouyang, Xiao Yan Xu

We propose a projection approach to perform quantum Monte Carlo (QMC) simulation on the infinite- Hubbard model at some integer fillings where either it is sign problem free or…

cond-mat.str-el2020★ 11 cited

Computing classification of interacting fermionic symmetry-protected topological phases using topological invariants

Yunqing Ouyang, Qing-Rui Wang, Zheng-Cheng Gu +1

In recent years, great success has been achieved on the classification of symmetry-protected topological (SPT) phases for interacting fermion systems by using generalized cohomolog…

cond-mat.stat-mech2018★ 21 cited

Equivalent-neighbor percolation models in two dimensions: crossover between mean-field and short-range behavior

Yunqing Ouyang, Youjin Deng, Henk W. J. Blöte

We investigate the influence of the range of interactions in the two-dimensional bond percolation model, by means of Monte Carlo simulations. We locate the phase transitions for se…

astro-ph.SR2017★ 35 cited

Solar Filament Longitudinal Oscillations along a Magnetic Field Tube with Two Dips

Yu-Hao Zhou, Li-Yue Zhang, Y. Ouyang +2

The large-amplitude longitudinal oscillations of solar filaments have been observed and explored for more than ten years. Previous studies are mainly based on the one-dimensional r…

astro-ph.SR2016★ 117 cited

Chirality and Magnetic Configurations of Solar Filaments

Y. Ouyang, Y. H. Zhou, P. F. Chen +1

It has been revealed that the magnetic topology in the solar atmosphere displays hemispheric preference, i.e., negative/positive helicity in the northern/southern hemisphere, respe…

astro-ph.SR2015★ 38 cited

Is flux rope a necessary condition for the progenitor of coronal mass ejections?

Y. Ouyang, K. Yang, P. F. Chen

A magnetic flux rope structure is believed to exist in most coronal mass ejections (CMEs). However, it has been long debated whether the flux rope exists before eruption or is form…