{ "id": "2403.08141", "version": "v1", "published": "2024-03-13T00:00:35.000Z", "updated": "2024-03-13T00:00:35.000Z", "title": "Parallel Diffusion Coefficient of Energetic Charged Particles in the Inner Heliosphere from the Turbulent Magnetic Fields Measured by Parker Solar Probe", "authors": [ "Xiaohang Chen", "Joe Giacalone", "Fan Guo", "Kristopher G. Klein" ], "comment": "Accepted to ApJ", "categories": [ "astro-ph.SR", "physics.plasm-ph", "physics.space-ph" ], "abstract": "Diffusion coefficients of energetic charged particles in turbulent magnetic fields are a fundamental aspect of diffusive transport theory but remain incompletely understood. In this work, we use quasi-linear theory to evaluate the spatial variation of the parallel diffusion coefficient $\\kappa_\\parallel$ from the measured magnetic turbulence power spectra in the inner heliosphere. We consider the magnetic field and plasma velocity measurements from Parker Solar Probe made during Orbits 5-13. The parallel diffusion coefficient is calculated as a function of radial distance from 0.062 to 0.8 AU, and the particle energy from 100 keV to 1GeV. We find that $\\kappa_\\parallel$ increases exponentially with both heliocentric distance and energy of particles. The fluctuations in $\\kappa_\\parallel$ are related to the episodes of large-scale magnetic structures in the solar wind. By fitting the results, we also provide an empirical formula of $\\kappa_{\\parallel}=(5.16\\pm1.22) \\times 10^{18} \\: r^{1.17\\pm0.08} \\: E^{0.71\\pm 0.02} \\; (cm^2/s)$ in the inner heliosphere which can be used as a reference in studying the transport and acceleration of solar energetic particles as well as the modulation of cosmic rays.", "revisions": [ { "version": "v1", "updated": "2024-03-13T00:00:35.000Z" } ], "analyses": { "keywords": [ "parallel diffusion coefficient", "turbulent magnetic fields", "parker solar probe", "energetic charged particles", "inner heliosphere" ], "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable" } } }