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Data-constrained Modeling of Electron Transport and Asymmetric Precipitation in the 2011 August 4 Solar Flare

  • Authors: Feiyu Yu, Xiangliang Kong, Ze Zhong, Zhentong Li, Zelong Jiang, Yingli Cui, Zhao Wu, Yao Chen, Gang Li

Feiyu Yu et al 2026 The Astrophysical Journal Letters 1003 .

  • Provider: AAS Journals

Caption: Figure 4.

Temporal evolution of precipitating electron counts at different energies under four turbulent scattering regimes: (a)–(b) no scattering (﹩{D}_{\mu \mu 0}^{t}=0﹩ s−1), (c)–(d) weak scattering (﹩{D}_{\mu \mu 0}^{t}=0.01﹩ s−1), (e)–(f) moderate scattering (﹩{D}_{\mu \mu 0}^{t}=0.5﹩ s−1), and (g)–(h) strong scattering (﹩{D}_{\mu \mu 0}^{t}=5﹩ s−1). Left and right columns are for the positive and negative polarities, respectively.

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