TL;DR
This paper reviews the physics of focused transport of solar energetic particles, compares common approximations, introduces a new finite-difference model, and demonstrates its application to observed solar electron events.
Contribution
It introduces a publicly available finite-difference model for solving the focused transport equation, improving understanding of particle acceleration and transport in solar energetic events.
Findings
Approximations like diffusion-advection and telegraph equations are insufficient for complex transport processes.
The finite-difference model accurately reproduces observed solar energetic electron events.
The paper clarifies misconceptions and reviews the evolution of modeling approaches.
Abstract
The basics of focused transport as applied to solar energetic particles are reviewed, paying special attention to areas of common misconception. The micro-physics of charged particles interacting with slab turbulence are investigated to illustrate the concept of pitch-angle scattering, where after the distribution function and focused transport equation are introduced as theoretical tools to describe the transport processes and it is discussed how observable quantities can be calculated from the distribution function. In particular, two approximations, the diffusion-advection and the telegraph equation, are compared in simplified situations to the full solution of the focused transport equation describing particle motion along a magnetic field line. It is shown that these approximations are insufficient to capture the complexity of the physical processes involved. To overcome such…
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