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Reanalysis Ties Voyager 2’s Extreme Uranus Radiation Belts to a Solar‑Wind Storm

The study argues a CIR-triggered chorus-wave episode briefly intensified electrons to make Voyager 2’s measurement a temporary state.

Overview

  • Southwest Research Institute scientists report in Geophysical Research Letters that a co-rotating interaction region was likely sweeping past Uranus during Voyager 2’s 1986 flyby.
  • By comparing Uranus measurements with well-studied Earth events, including a 2019 episode, the team links strong chorus waves to rapid electron acceleration.
  • The work addresses the long-standing puzzle of intense electron belts alongside a plasma-poor magnetosphere and reconciles tensions with Kennel–Petschek limits.
  • Researchers conclude the observed radiation belt reflects an extreme, transient condition rather than Uranus’s typical environment.
  • The findings bolster calls for a dedicated Uranus mission to obtain repeated in situ measurements under varying solar-wind conditions, with implications for Neptune as well.