An analytic expression for the radial dependence of the diffusion coefficient for quiet time energetic helium and oxygen in the heliosphere

Physics – Nuclear Physics

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Heliosphere, Helium, Nuclei (Nuclear Physics), Oxygen, Particle Diffusion, Solar Cosmic Rays, Atmospheric Diffusion, Differential Equations, Energetic Particles, Energy Spectra, Fokker-Planck Equation, Interplanetary Medium, Particle Energy, Solar Protons, Solar Terrestrial Interactions

Scientific paper

Taking into account recent observations of the differential radial gradients and energy spectra of quiet time energetic particles of different energies and masses and over a large heliocentric radial distance from 0.3 to 18 ALL, it is shown that the transport equation for these particles (Fokker-Planck equation) reduces to a first-order differential equation for the radial diffusion coefficient (which can then be solved analytically). For energetic helium and oxygen nuclei, the radial dependence of their diffusion coefficient is then discussed.

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