Perpendicular Diffusion of Solar Energetic Particles: Model Results and Implications for Electrons
R.D. Strauss, N. Dresing, N.E. Engelbrecht

TL;DR
This study uses a 2D transport model with perpendicular diffusion to simulate solar energetic electron propagation, comparing results with observations to understand the role of perpendicular diffusion in SEP longitudinal transport.
Contribution
It introduces a model with transport coefficients derived from first principles, emphasizing the sensitivity to perpendicular diffusion and its impact on SEP transport.
Findings
Perpendicular diffusion significantly influences SEP longitudinal distribution.
Model results are highly sensitive to the magnitude of the perpendicular diffusion coefficient.
Perpendicular diffusion is most effective early in SEP events when intensity gradients are large.
Abstract
The processes responsible for the effective longitudinal transport of solar energetic particles (SEPs) are still not completely understood. We address this issue by simulating SEP electron propagation using a spatially 2D transport model that includes perpendicular diffusion. By implementing, as far as possible, the most reasonable estimates of the transport (diffusion) coefficients, we compare our results, in a qualitative manner, to recent observations {at energies of 55 -- 105 keV}, focusing on the longitudinal distribution of the peak intensity, the maximum anisotropy and the onset time. By using transport coefficients which are derived from first principles, we limit the number of free parameters in the model to: (i) the probability of SEPs following diffusing magnetic field lines, quantified by , and (ii) the broadness of the Gaussian injection function. It is found…
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Taxonomy
TopicsSolar Radiation and Photovoltaics · Solar Thermal and Photovoltaic Systems · Energy and Environment Impacts
