207 citations · 586 across the 27 of their papers we have counts for
27 papers
The AIMS Site Survey
Xingming Bao, Jian Wang, Shuai Jing +2
This paper reports site survey results for the Infrared System for the Accurate Measurement of Solar Magnetic Field, especially in Saishiteng Mountain, Qinghai, China. Since 2017,…
Observation of two splitting processes in a partial filament eruption on the sun: the role of breakout reconnection
Zheng Sun, Ting Li, Hui Tian +5
Partial filament eruptions have often been observed, however, the physical mechanisms that lead to filament splitting are not yet fully understood. In this study, we present a uniq…
A Type II Radio Burst Driven by a Blowout Jet on the Sun
Zhenyong Hou, Hui Tian, Wei Su +5
Type II radio bursts are often associated with coronal shocks that are typically driven by coronal mass ejections (CMEs) from the Sun. Here, we conduct a case study of a type II ra…
Traveling kink oscillations of coronal loops launched by a solar flare
Dong Li, Xianyong Bai, Hui Tian +5
We investigate the traveling kink oscillation triggered by a solar flare on 2022 September 29. The observational data is mainly measured by the Solar Upper Transition Region Imager…
Heating of quiescent coronal loops caused by nearby eruptions observed with the Solar Dynamics Observatory and the Solar Upper Transition Region Imager
Leping Li, Hui Tian, Huadong Chen +5
How structures, e.g., magnetic loops, in the upper atmosphere, i.e., the transition region and corona, are heated and sustained is one of the major unresolved issues in solar and s…
The Solar Upper Transition Region Imager (SUTRI) onboard the SATech-01 satellite
Xianyong Bai, Hui Tian, Yuanyong Deng +56
The Solar Upper Transition Region Imager (SUTRI) onboard the Space Advanced Technology demonstration satellite (SATech-01), which was launched to a sun-synchronous orbit at a heigh…
Observations of pores and surrounding regions with CO 4.66 μm lines by BBSO/CYRA
Yongliang Song, Xianyong Bai, Xu Yang +6
Solar observations of carbon monoxide (CO) indicate the existence of lower-temperature gas in the lower solar chromosphere. We present an observation of pores, and quiet-Sun, and n…
Solar Ring Mission: Building a Panorama of the Sun and Inner-heliosphere
Yuming Wang, Xianyong Bai, Changyong Chen +50
Solar Ring (SOR) is a proposed space science mission to monitor and study the Sun and inner heliosphere from a full 360° perspective in the ecliptic plane. It will deploy three 120…
A new post-hoc flat field measurement method for the Solar X-ray and Extreme Ultraviolet Imager onboard the Fengyun-3E satellite
Qiao Song, Xianyong Bai, Bo Chen +13
The extreme ultraviolet (EUV) observations are widely used in solar activity research and space weather forecasting since they can observe both the solar eruptions and the source r…
Measurements of the magnetic field strengths at the bases of stellar coronae using the magnetic-field-induced transition theory
Yajie Chen, Xianyu Liu, Hui Tian +6
Measurements of the magnetic field in the stellar coronae are extremely difficult. Recently, it was proposed that the magnetic-field-induced transition (MIT) of the Fe X 257 Å line…
Forward Modeling of Solar Coronal Magnetic Field Measurements Based on a Magnetic-field-induced Transition in Fe X
Yajie Chen, Wenxian Li, Hui Tian +6
It was recently proposed that the intensity ratios of several extreme ultraviolet spectral lines from the Fe X ion can be used to measure the solar coronal magnetic field based on…
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…
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…
Critical Science Plan for the Daniel K. Inouye Solar Telescope (DKIST)
Mark P. Rast, Nazaret Bello González, Luis Bellot Rubio +84
The Daniel K. Inouye Solar Telescope (DKIST) will revolutionize our ability to measure, understand and model the basic physical processes that control the structure and dynamics of…
Non-LTE Calculations of the Mg I 12.32 m Line in a Flaring Atmosphere
Jie Hong, Xianyong Bai, Ying Li +2
The infrared Mg I lines near 12 microns are a pair of emission lines which are magnetically sensitive and have been used to measure solar magnetic fields. Here we calculate the res…
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…
Spectro-polarimetric Observations at the NVST: I. Instrumental Polarization Calibration and Primary Measurements
Jun-Feng Hou, Zhi Xu, Shu Yuan +8
This paper is devoted to the primary spectro-polarimetric observation performed at the New Vacuum Solar Telescope of China since 2017, and our aim is to precisely evaluate the real…
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…
Signatures of magnetic reconnection at the footpoints of fan shape jets on a light bridge driven by photospheric convective motions
Xianyong Bai, Hector Socas-Navarro, Daniel Nóbrega-Siverio +5
Dynamical jets are generally found on Light bridges (LBs), which are key to studying sunspots decays. So far, their formation mechanism is not fully understood. In this paper, we u…
A Complex Solar Coronal Jet with Two Phases
Jie Chen, Jiangtao Su, Yuanyong Deng +1
Jets often occur repeatedly from almost the same location. In this paper, a complex solar jet was observed with two phases to the west of NOAA AR 11513 on July 2nd, 2012. If it had…
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…
Improved magnetogram calibration of SMFT and its comparison with the HMI
Xianyong Bai, Yuanyong Deng, Fei Teng +3
In this paper, we try to improve the magnetogram calibration method of the Solar Magnetic Field Telescope (SMFT). The improved calibration process fits the observed full Stokes inf…
Tracking Back the Solar Wind to its Photospheric Footpoints from Wind Observations -- A Statistical Study
C. Huang, Y. Y. Yan, G. Li +2
It is of great importance to track the solar wind back to its photospheric source region and identify the related current sheets; this will provide key information for investigatin…
The Induced Electric Field Distribution in Solar Atmosphere
Rong Chen, Zhiliang Yang, Yuanyong Deng
A method of calculating induced electric field is presented in this paper. Induced electric field in solar atmosphere is derived by the time variation of magnetic field when the ch…