42 citations · 67 across the 5 of their papers we have counts for
9 papers
Spectroscopic Observations of the Solar Corona during the 2017 August 21 Total Solar Eclipse: Comparison of Spectral Line Widths and Doppler Shifts Between Open and Closed Magnetic Structures
Yingjie Zhu, Shadia R. Habbal, Adalbert Ding +5
The spectroscopic observations presented here were acquired during the 2017 August 21 total solar eclipse with a three-channel partially multiplexed imaging spectrometer (3PAMIS) o…
Is it possible to detect coronal mass ejections on solar-type stars through extreme-ultraviolet spectral observations?
Zihao Yang, Hui Tian, Yingjie Zhu +3
Stellar coronal mass ejections (CMEs) from host stars are an important factor that affects the habitability of exoplanets. Although their solar counterparts have been well observed…
Estimating Ion Temperatures at the Polar Coronal Hole Boundary
Yingjie Zhu, Judit Szente, Enrico Landi
The temperatures of the heavy ions () in the solar corona provide critical information about the heating mechanism of the million-degree corona. However, the measurement of $T…
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…
Fe XII and Fe XIII Line Widths in the Polar Off-limb Solar Corona up to 1.5 Rsun
Yingjie Zhu, Judit Szente, Enrico Landi
The nonthermal broadening of spectral lines formed in the solar corona is often used to seek the evidence of Alfvén waves propagating in the corona. To have a better understanding…
Modeling Mg II h, k and Triplet Lines at Solar Flare Ribbons
Yingjie Zhu, Adam F. Kowalski, Hui Tian +3
Observations from the \textit{Interface Region Imaging Spectrograph} (\textsl{IRIS}) often reveal significantly broadened and non-reversed profiles of the Mg II h, k and triplet li…