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Sun-as-a-star Spectroscopic Observations of the Line-of-sight Velocity of a Solar Eruption on 2021 October 28

  • Authors: Yu Xu, 昱 徐, Hui Tian, 晖 田, Zhenyong Hou, 振永 侯, Zihao Yang, 子浩 杨, Yuhang Gao, 宇航 高, Xianyong Bai, 先勇 白

Yu Xu et al 2022 The Astrophysical Journal 931 .

  • Provider: AAS Journals

Caption: Figure 4.

(a) The pre-flare subtracted line profiles for O III 52.57 nm, (b) O V 62.96 nm, and (c) O VI 103.1 nm from 15:23:30 UT to 15:34:30 UT. The observation times are labeled on the right side of each profile and the y-axis is offset for a better illustration. The gray dashed lines indicate the level of spectral irradiance during the quiescent time. The vertical black lines indicate the rest wavelengths. The negative offset velocities represent the blue wings while the positive, the red.

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