Image Details
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.
© 2026. The Author(s). Published by the American Astronomical Society.