activity
20182021
most citedCoronal microjets in quiet-Sun regions observed with the Extreme Ultraviolet Imager onboard Solar Orbiter

45 citations · 87 across the 9 of their papers we have counts for

collaborators

13 papers

astro-ph.SR202145 cited

Coronal microjets in quiet-Sun regions observed with the Extreme Ultraviolet Imager onboard Solar Orbiter

Zhenyong Hou, Hui Tian, David Berghmans +8

We report the smallest coronal jets ever observed in the quiet Sun with recent high resolution observations from the High Resolution Telescopes (HRI-EUV and HRI-Lyα) of the Extreme…

astro-ph.SR202111 cited

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…

astro-ph.SR2021

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…

astro-ph.SR2021

Formation of solar quiescent coronal loops through magnetic reconnection in an emerging active region

Zhenyong Hou, Hui Tian, Hechao Chen +6

Coronal loops are building blocks of solar active regions. However, their formation mechanism is still not well understood. Here we present direct observational evidence for the fo…

astro-ph.SR20215 cited

Small-scale Bright Blobs Ejected from a Sunspot Light Bridge

Fuyu Li, Yajie Chen, Yijun Hou +3

Light bridges (LBs) are bright lanes that divide an umbra into multiple parts in some sunspots. Persistent oscillatory bright fronts at a temperature of K are commonly…

astro-ph.SR20205 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…