2026-10-06T22:39:34Z https://www.scidb.cn/oai

10.57760/sciencedb.space.0032d 2026-09-29T10:21:54Z

2026-09-29 Modeling of Heavy-Ion Spectral and Flux Variations with Interplanetary Turbulence Intensity in Solar Energetic Particle Events doi:10.57760/sciencedb.space.0032d en The dataset contains simulated omnidirectional flux time profiles for six ion species (H, He, O, Mg, S, Fe) in solar energetic particle events. The data were generated by solving the focused transport equation using a backward stochastic differential equation method. The simulations assume a Parker spiral magnetic field with solar wind speed 400 km/s and magnetic field strength 3.54 nT at 1 AU. Particles are injected at 0.1 AU with a Reid-type diffusive temporal profile and a power-law source injection. The data are stored as plain-text .dat files in a single compressed archive (.zip). Each file corresponds to one species and one turbulence level, with columns for time and omnidirectional flux. Solar Energetic particle; Interplanetray turbulence; Heavy ion Lian Wanyi PUBLIC https://creativecommons.org/licenses/by/4.0/ dataset Science Data Bank