C
Cheng Fang
Researcher at Nanjing University
Publications - 67
Citations - 1493
Cheng Fang is an academic researcher from Nanjing University. The author has contributed to research in topics: Solar flare & Magnetic reconnection. The author has an hindex of 24, co-authored 67 publications receiving 1294 citations. Previous affiliations of Cheng Fang include Chinese Ministry of Education.
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Journal ArticleDOI
Chirality and Magnetic Configurations of Solar Filaments
TL;DR: In this paper, a new method based on filament drainage was applied to 571 erupting filaments from 2010 May to 2015 December to determine the filament chirality and its hemispheric preference.
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Advanced Space-based Solar Observatory (ASO-S): an overview
Weiqun Gan,Cheng Zhu,Yuanyong Deng,Hui Li,Yang Su,Haiying Zhang,Bo Chen,Zhe Zhang,Jian Wu,Lei Deng,Yu Huang,Jianfeng Yang,Ji-Jun Cui,Jin Chang,Chi Wang,Ji Wu,Zeng-Shan Yin,Wen Chen,Cheng Fang,Yihua Yan,Jun Lin,Wei-Ming Xiong,Bin Chen,Hai-Chao Bao,Cai-Xia Cao,Yan-Ping Bai,Tao Wang,Bing-Long Chen,Xin-Yu Li,Ye Zhang,Li Feng,Jiangtao Su,Ying Li,Wei Chen,You-Ping Li,Ying-Na Su,Hai-Yan Wu,Mei Gu,Lei Huang,Xue-Jun Tang +39 more
TL;DR: The Advanced Space-based Solar Observatory (ASO-S) is a mission proposed for the 25th solar maximum by the Chinese solar community as mentioned in this paper, where three payloads are deployed: the Full-disk vector MagnetoGraph (FMG), the Lyman-alpha Solar Telescope (LST) and the Hard X-ray Imager (HXI).
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Ellerman Bombs, Type II White-light Flares and Magnetic Reconnection in the Solar Lower Atmosphere
TL;DR: In this paper, the authors present numerical simulations of magnetic reconnection occurring in such a deep atmosphere, with the aim to account for the common features of the two phenomena, e.g., Ellerman bombs and Type II white-light flares.
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Spectral observations of ellerman bombs and fitting with a two-cloud model
TL;DR: In this paper, a two-cloud model was proposed to fit the observed line profiles of four typical Ellerman bombs in the active region NOAA 11765 on 2013 June 6, observed with the Fast Imaging Solar Spectrograph installed at the 1.6 m New Solar Telescope at Big Bear Solar Observatory.
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Numerical simulation of solar microflares in a canopy-type magnetic configuration
TL;DR: In this article, a 2.5-dimensional, compressible, resistive magnetohydrodynamic simulation of magnetic reconnection with gravity considered is performed. And the authors successfully simulate the coronal and chromospheric microflares whose current sheets are located at the corona and the chromosphere, respectively.