activity
20162020
most citedA New Comprehensive Data Set of Solar Filaments of 100 yr Interval. I

11 citations · 33 across the 5 of their papers we have counts for

collaborators

9 papers

astro-ph.SR20205 cited

Infrared diagnostics of the solar magnetic field with Mg I 12 m lines: forward-model results

Xin Li, YongLiang Song, H. Uitenbroek +3

The Mg I 12.32 and 12.22 m lines are a pair of emission lines that present a great advantage for accurate solar magnetic field measurement. They potentially contribute to the di…

astro-ph.SR20207 cited

A nonlinear solar magnetic field calibration method for the filter-based magnetograph by the residual network

Jingjing Guo, Xianyong Bai, Yuanyong Deng +5

The method of solar magnetic field calibration for the filter-based magnetograph is normally the linear calibration method under weak-field approximation that cannot generate the s…

astro-ph.SR2020

Doppler shift oscillations of a sunspot detected by CYRA and IRIS

D. Li, X. Yang, X. Y. Bai +4

Context. The carbon monoxide (CO) molecular line at around 46655 A in solar infrared spectra is often used to investigate the dynamic behavior of the cold heart of the solar atmosp…

astro-ph.SR202011 cited

A New Comprehensive Data Set of Solar Filaments of 100 yr Interval. I

GangHua Lin, GaoFei Zhu, Xiao Yang +12

Filaments are very common physical phenomena on the Sun and are often taken as important proxies of solar magnetic activities. The study of filaments has become a hot topic in the…

astro-ph.IM202010 cited

A Non-Linear Magnetic Field Calibration Method for Filter-Based Magnetographs by Multilayer Perceptron

JingJing Guo, XianYong Bai, YuanYong Deng +5

For filter-based magnetographs, the linear calibration method under the weak-field assumption is usually adopted; this leads to magnetic saturation effect in the regions with stron…

astro-ph.IM2019

Solar Filament Recognition Based on Deep Learning

GaoFei Zhu, GangHua Lin, DongGuang Wang +2

The paper presents a reliable method using deep learning to recognize solar filaments in H-alpha full-disk solar images automatically. This method cannot only identify filaments ac…