activity
20172023
most citedGlobal maps of the magnetic field in the solar corona

175 citations · 1.2k across the 27 of their papers we have counts for

collaborators
Showing 2022Show all

8 papers · 1 filter

astro-ph.SR2022★ 16 cited

Application of a magnetic-field-induced transition in Fe X to solar and stellar coronal magnetic field measurements

Yajie Chen, Wenxian Li, Hui Tian +3

Magnetic fields play a key role in driving a broad range of dynamic phenomena in the atmospheres of the Sun and other stars. Routine and accurate measurements of the magnetic field…

astro-ph.SR2022★ 6 cited

Forward Modeling of Magnetic-field Measurements at the Bases of Stellar Coronae through Extreme-Ultraviolet Spectroscopy

Xianyu Liu, Hui Tian, Yajie Chen +4

Measurements of the stellar coronal magnetic field are of great importance in understanding the stellar magnetic activity, yet the measurements have been extremely difficult. Recen…

astro-ph.SR2022★ 9 cited

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…

astro-ph.SR2022★ 44 cited

Possible detection of coronal mass ejections on late-type main-sequence stars in LAMOST medium-resolution spectra

Hong-peng Lu, Hui Tian, Li-yun Zhang +9

Context. Stellar coronal mass ejections (CMEs) are the primary driver of the exoplanetary space weather and they could affect the habitability of exoplanets. However, detections of…

astro-ph.SR2022★ 21 cited

Can we detect coronal mass ejections through asymmetries of Sun-as-a-star extreme-ultraviolet spectral line profiles?

Zihao Yang, Hui Tian, Xianyong Bai +8

Coronal mass ejections (CMEs) are the largest-scale eruptive phenomena in the solar system. Associated with enormous plasma ejections and energy release, CMEs have an important imp…

astro-ph.SR2022★ 47 cited

Decayless oscillations in solar coronal bright points

Yuhang Gao, Hui Tian, Tom Van Doorsselaere +1

Decayless kink oscillations of solar coronal loops (or decayless oscillations for short) have attracted great attention since their discovery. Coronal bright points (CBPs) are mini…

astro-ph.SR2022★ 7 cited

Doppler shifts of spectral lines formed in the solar transition region and corona

Yajie Chen, Hardi Peter, Damien Przybylski +2

Context. Emission lines formed in the transition region and corona show dominantly redshifts and blueshifts, respectively. Aims. We investigate the Doppler shifts in a 3D radiation…

astro-ph.SR2022★ 37 cited

Three-dimensional Propagation of the Global EUV Wave associated with a solar eruption on 2021 October 28

Zhenyong Hou, Hui Tian, Jing-Song Wang +16

We present a case study for the global extreme ultraviolet (EUV) wave and its chromospheric counterpart `Moreton-Ramsey wave' associated with the second X-class flare in Solar Cycl…