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Statistics of Solar Filament Mass Based on CHASE Sun-as-a-star Spectroscopic Observations

  • Authors: T. Y. Xie, Z. H. Zhao, X. Cheng, Y. H. Chen, Z. Zheng, Q. Hao, C. Li, M. D. Ding

T. Y. Xie et al 2026 The Astrophysical Journal Letters 1008 .

  • Provider: AAS Journals

Caption: Figure 2.

Distributions of physical parameters derived from the Sun-as-a-star cloud-model fitting for the full filament sample. (A) Optical depth τ0; (B) absolute equivalent width ∣EW∣ in Hα; (C) volume density ρ; (D) total mass. The dashed vertical line in each panel marks the median of the distribution. In panel (A), the red dashed curve shows the best-fit log-normal distribution selected by the BIC, and the shaded region indicates the 1σ interval [τ0 = 1.39, 2.50]. The y-axis in all panels represents the normalized probability density.

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