Non-thermal Broadening of IRIS Fe XXI Line Caused by Turbulent Plasma Flows in the Magnetic Reconnection Region During Solar EruptionsDOI: info:10.3389/fspas.2023.1096133v. 1019
Shen, Chengcai, Polito, Vanessa, Reeves, Katharine K., Chen, Bin, Yu, Sijie, and Xie, Xiaoyan. 2023. "Non-thermal Broadening of IRIS Fe XXI Line Caused by Turbulent Plasma Flows in the Magnetic Reconnection Region During Solar Eruptions." Frontiers in Astronomy and Space Sciences, 10 19. https://doi.org/10.3389/fspas.2023.1096133.