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The Solar-like Latitudinal Distribution of Flaring Activities Revealed by TESS, APOGEE, and GALAH

  • Authors: Huiqin Yang, Shuai Liu, Yang Huang, Bowen Zhang, Jifeng Liu

Huiqin Yang et al 2026 The Astrophysical Journal Supplement Series 283 .

  • Provider: AAS Journals

Caption: Figure 4.

Rossby number vs. the mean latitude of active regions. Each black point represents the best match between the observation and the simulated LaDAR in a Ro bin (the green dashed line in Figure 3). The blue point is obtained by the upper envelope of the sini–flaring activity relationship in Figure C3. The Sun is marked with a red ⊙ symbol. The uncertainty of the mean latitude is ±7°, which is the same as the Sun. The uncertainty of Ro represents the range of each Ro bin used to fit the sini–flaring activity relationship.

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