activity
20102022
most citedChirality and Magnetic Configurations of Solar Filaments

117 citations · 308 across the 5 of their papers we have counts for

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8 papers · 1 filter

astro-ph.SR2022★ 78 cited

Calibration procedures for the CHASE/HIS science data

Ye Qiu, ShiHao Rao, Chuan Li +17

The Hα line is an important optical line in solar observations containing the information from the photosphere to the chromosphere. To study the mechanisms of solar eruptions and t…

astro-ph.SR2018

Three-dimensional MHD Simulations of Solar Prominence Oscillations in a Magnetic Flux Rope

Yu-Hao Zhou, C. Xia, R. Keppens +2

Solar prominences are subject to all kinds of perturbations during their lifetime, and frequently demonstrate oscillations. The study of prominence oscillations provides an alterna…

astro-ph.SR2017★ 29 cited

Material supply and magnetic configuration of an active region filament

P. Zou, C. Fang, P. F. Chen +3

It is important to study the fine structures of solar filaments with high-resolution observations since it can help us understand the magnetic and thermal structures of the filamen…

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.SR2016

Variations of the 3-D coronal magnetic field associated with the X3.4-class solar flare event of AR 10930

Han He, Huaning Wang, Yihua Yan +2

The variations of the 3-D coronal magnetic fields associated with the X3.4-class flare of active region 10930 are studied in this paper. The coronal magnetic field data are reconst…

astro-ph.SR2016

Bidirectional outflows as evidence of magnetic reconnection leading to a solar microflare

Jie Hong, M. D. Ding, Ying Li +5

Magnetic reconnection is a rapid energy release process that is believed to be responsible for flares on the Sun and stars. Nevertheless, such flare-related reconnection is mostly…