2026/04/30 by Anonymous, Adnane Osmane, Xin An +5
Physics and Astronomy · #Ionosphere and magnetosphere dynamics #Laser-Plasma Interactions and Diagnostics #Magnetic confinement fusion research #astro-ph.EP #physics.plasm-ph #physics.space-ph
paper · pdf · doi:10.1103/5mmn-fm2p
published as Phys. Rev. Research 8, 033104, (2026) · Accepted in Physical Review Research, 45 pages, 4 Figures. Shortened abstract
openalex publication_date 2026/07/06 · openalex created_date 2026/07/07 · arxiv created 2026/07/14 · arxiv updated 2026/07/30 · openalex updated_date 2026/07/30
Since the dawn of the space age, observations of energetic particles in planetary radiation belts have been interpreted within a diffusive transport framework, even though the dominant processes that populate and deplete these belts-such as injections and moon-driven absorption-produce highly structured, spatially localized particle distributions. This exposes a fundamental question: how can coherent phase-space structures evolving under collisionless dynamics give rise to observational signatures consistent with diffusion-based transport? Here we show that diffusion-like behaviour inferred from radiation belt observations can arise solely from an observational phase-mixing effect, independent of stochastic wave-particle transport. As orbiting spacecraft sweep across neighbouring drift shells while trapped particles undergo electromagnetic drifts, measurements inevitably sample regions with slightly different drift frequencies. This converts localized drift-phase structures into rapidly decorrelating temporal signals, making them observationally indistinguishable from those produced by stochastic wave-particle processes. We derive the associated correlation function analytically and show that the effective lifetime of these structures is only a few drift periods. Consequently, even highly localized injections rapidly lose coherence, preventing spacecraft from resolving fine-scale structure in the distribution function. These results show that collisionless dynamics can produce observational signatures that mimic diffusive transport on timescales shorter than those expected from radial transport, biasing inferred transport rates and long-term flux predictions. This calls for a reassessment of diffusion-based interpretations from sparse in-situ measurements of radiation belts at Earth, across the solar system, and in the recently discovered radiation belts of ultra-cool brown dwarfs.