| Developing an advanced automated method for solar filament recognition and its scientific application to a solar cycle of MLSO Hα data Q Hao, C Fang, PF Chen Solar Physics 286, 385-404, 2013 | 37 | 2013 |
| Developing an advanced automated method for solar filament recognition and its scientific application to a solar cycle of MLSO Hα data Q Hao, C Fang, PF Chen Solar Physics 286, 385-404, 2013 | 37 | 2013 |
| A circular white-light flare with impulsive and gradual white-light kernels Q Hao, K Yang, X Cheng, Y Guo, C Fang, MD Ding, PF Chen, Z Li Nature Communications 8 (1), 2202, 2017 | 33 | 2017 |
| A two-ribbon white-light flare associated with a failed solar eruption observed by ONSET, SDO, and IRIS X Cheng, Q Hao, MD Ding, K Liu, PF Chen, C Fang, YD Liu The Astrophysical Journal 809 (1), 46, 2015 | 31 | 2015 |
| Material supply and magnetic configuration of an active region filament P Zou, C Fang, PF Chen, K Yang, Q Hao, W Cao The Astrophysical Journal 831 (2), 123, 2016 | 25 | 2016 |
| Understanding the white-light flare on 2012 March 9: evidence of a two-step magnetic reconnection Q Hao, Y Guo, Y Dai, MD Ding, Z Li, XY Zhang, C Fang Astronomy & Astrophysics 544, L17, 2012 | 25 | 2012 |
| Chinese Hα solar explorer (CHASE)–a complementary space mission to the ASO-S C Li, C Fang, Z Li, MD Ding, PF Chen, Z Chen, LK Lin, CZ Chen, CY Chen, ... Research in Astronomy and Astrophysics 19 (11), 165, 2019 | 24 | 2019 |
| Transition from circular-ribbon to parallel-ribbon flares associated with a bifurcated magnetic flux rope Z Zhong, Y Guo, MD Ding, C Fang, Q Hao The Astrophysical Journal 871 (1), 105, 2019 | 23 | 2019 |
| Can the temperature of Ellerman Bombs be more than 10 000 K? C Fang, Q Hao, MD Ding, Z Li Research in Astronomy and Astrophysics 17 (4), 031, 2017 | 17 | 2017 |
| Statistical analysis of filament features based on the Hα solar images from 1988 to 2013 by computer automated detection method Q Hao, C Fang, W Cao, PF Chen The Astrophysical Journal Supplement Series 221 (2), 33, 2015 | 16 | 2015 |
| 2.5 m wide-field and high-resolution telescope C Fang, B Gu, X Yuan, M Ding, P Chen, Z Dai, X Li, Y Shi, J Xie, J Bai, ... Scientia Sinica Physica, Mechanica & Astronomica 49 (5), 059603, 2019 | 11 | 2019 |
| Can we determine the filament chirality by the filament footpoint location or the barb-bearing? Q Hao, Y Guo, C Fang, PF Chen, WD Cao Research in Astronomy and Astrophysics 16 (1), 001, 2016 | 10 | 2016 |
| Revisiting the spectral features of ellerman bombs and uv bursts. i. Radiative hydrodynamic simulations J Hong, Y Li, MD Ding, Q Hao The Astrophysical Journal 921 (1), 50, 2021 | 6 | 2021 |
| Automated detection methods for solar activities and an application for statistic analysis of solar filament Q Hao, PF Chen, C Fang Proceedings of the International Astronomical Union 13 (S340), 101-107, 2018 | 5 | 2018 |
| Statistical analysis of the Si I 6560.58 Å line observed by CHASE J Hong, Y Qiu, Q Hao, Z Xu, C Li, M Ding, C Fang Astronomy & Astrophysics 668, A9, 2022 | 4 | 2022 |
| Calibration procedures for the CHASE/HIS science data Y Qiu, SH Rao, C Li, C Fang, MD Ding, Z Li, YW Ni, WB Wang, J Hong, ... Science China Physics, Mechanics & Astronomy 65 (8), 289603, 2022 | 4 | 2022 |
| Spectral diagnostics of solar photospheric bright points Q Hao, C Fang, MD Ding, Z Li, W Cao The Astrophysical Journal 900 (2), 130, 2020 | 3 | 2020 |
| Developing an Automated Detection, Tracking and Analysis Method for Solar Filaments Observed by CHASE via Machine Learning Z Zheng, Q Hao, Y Qiu, J Hong, C Li, MD Ding arXiv preprint arXiv:2402.14209, 2024 | 1 | 2024 |
| Denoising Astronomical Images with an Unsupervised Deep Learning Based Method T Liu, Y Quan, Y Su, Y Guo, S Liu, H Ji, Q Hao, Y Gao | 1 | 2023 |
| Statistical Analyses of Solar Prominences and Active Region Features in 304\AA {} Filtergrams detected via Deep Learning T Zhang, Q Hao, PF Chen arXiv preprint arXiv:2402.13502, 2024 | | 2024 |
