3 papers
astro-ph.SR2024
Observing the evolution of the Sun's global coronal magnetic field over eight months
Zihao Yang, Hui Tian, Steven Tomczyk +4
The magnetic field in the Sun's corona stores energy that can be released to heat the coronal plasma and drive solar eruptions. Measurements of the global coronal magnetic field ha…
astro-ph.SR2024
Simulated Coronal Mass Ejections on a young Solar-Type Star and the Associated Instantaneous Angular Momentum Loss
Yu Xu, Julián D. Alvarado-Gómez, Hui Tian +3
Coronal mass ejections (CMEs) on stars can change the stars' magnetic field configurations and mass loss rates during the eruption and propagation and therefore, may affect the sta…
astro-ph.SR2024
Global Coronal Plasma Diagnostics Based on Multi-slit EUV Spectroscopy
Lami Chan, Hui Tian, Xianyu Liu +4
Full-disk spectroscopic observations of the solar corona are highly desired to forecast solar eruptions and their impact on planets and to uncover the origin of solar wind. In this…