activity
20122021
most citedSolar Filament Recognition Based on Deep Learning

35 citations · 186 across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.SR2021

Solar observation with the Fourier transform spectrometer I : Preliminary results of the visible and near-infrared solar spectrum

Xianyong Bai, Zhiyong Zhang, Zhiwei Feng +6

The Fourier transform spectrometer (FTS) is a core instrument for solar observation with high spectral resolution, especially in the infrared. The Infrared System for the Accurate…

astro-ph.SR2020★ 5 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.SR2020★ 7 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★ 11 cited

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.SR2020★ 7 cited

Automatic Detection and Correction Algorithms for Magnetic Saturation in the SMFT/HSOS longitudinal Magnetograms

Haiqing Xu, Suo Liu, Jiangtao Su +8

longitudinal magnetic field often suffers the saturation effect in strong magnetic field region when the measurement performs in a single-wavelength point and linear calibration is…

astro-ph.SR2020★ 11 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.IM2020★ 10 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★ 35 cited

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…

astro-ph.SR2019★ 4 cited

Intelligent Recognition of Time Stamp Characters in Solar Scanned Images from Film

JiaFeng Zhang, GuangZhong Lin, ShuGuang Zeng +5

Prior to the availability of digital cameras, the solar observational images are typically recorded on films, and the information such as date and time were stamped in the same fra…

astro-ph.SR2019

Standard Magnetic Field Production at Huairou Solar Observing Station

Suo Liu, Ganghua Lin, Xiao Yang +3

The regular solar observations are operated at Huairou Solar Observing Station (HSOS) since 1987, which make the construction of long-term magnetic field datasets available to unde…

astro-ph.SR2016★ 24 cited

Automatic Recognition of Sunspots in HSOS Full-Disk Solar Images

Cui Zhao, GangHua Lin, YuanYong Deng +1

A procedure is introduced to recognise sunspots automatically in solar full-disk photosphere images obtained from Huairou Solar Observing Station, National Astronomical Observatori…

astro-ph.SR2013★ 27 cited

Magnetic Nonpotentiality in Photospheric Active Regions as a Predictor of Solar Flares

Xiao Yang, GangHua Lin, HongQi Zhang +1

Based on several magnetic nonpotentiality parameters obtained from the vector photospheric active region magnetograms obtained with the Solar Magnetic Field Telescope at the Huairo…

astro-ph.SR2012★ 20 cited

A Statistical Study on Force-Freeness of Solar Magnetic Fields in the Photosphere

S. Liu, J. T. Su, H. Q. Zhang +4

It is an indisputable fact that solar magnetic fields are force-free in the corona, where force free fields means that current and magnetic fields are parallel and there is no Lore…

astro-ph.SR2012★ 25 cited

A Statistical Study on Photospheric Magnetic Nonpotentiality of Active Regions and Its Relationship with Flares during Solar Cycles 22-23

Xiao Yang, HongQi Zhang, Yu Gao +2

A statistical study is carried out on the photospheric magnetic nonpotentiality in solar active regions and its relationship with associated flares. We select 2173 photospheric vec…