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Dispersive Suprathermal Ion Events Observed by the Parker Solar Probe Mission

  • S. T. Alnussirat
  • , R. Livi
  • , D. E. Larson
  • , A. Rahmati
  • , P. L. Whittlesey
  • , O. Romeo
  • , S. T. Badman
  • , Milo Buitrago-Casas
  • , Juan Carlos Martínez Oliveros
  • , M. Pulupa
  • , S. D. Bale
  • , J. Huang
  • , J. Verniero
  • , N. Raouafi
  • , Donald Mitchell
  • , D. J. McComas
  • , Matt Hill
  • , Christina Cohen

Research output: Contribution to journalArticlepeer-review

Abstract

During Encounter 11, Parker Solar Probe observed a low-energy dispersive ions event of solar origin. The event was observed in the SPAN-I and IS⊙IS EPI-Lo sensors. The event started at a few MeV energy in the EPI-Lo sensor and progressed down in energy to ≈1 keV and merged with the bulk of the solar wind. This event is substantially different from typical solar energetic particles because the energetic population shows a distinct peak in the energy spectrum that descends in energy (not a power-law tail). In this Letter, we explore this event’s nature, origin, and characteristics.

Original languageEnglish (US)
Article numberL32
JournalAstrophysical Journal Letters
Volume954
Issue number1
DOIs
StatePublished - Sep 1 2023

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

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