Strong Perpendicular Velocity-space Diffusion in Proton Beams Observed by Parker Solar Probe

  • J. L. Verniero
  • , B. D.G. Chandran
  • , D. E. Larson
  • , K. Paulson
  • , B. L. Alterman
  • , S. Badman
  • , S. D. Bale
  • , J. W. Bonnell
  • , T. A. Bowen
  • , T. Dudok De Wit
  • , J. C. Kasper
  • , K. G. Klein
  • , E. Lichko
  • , R. Livi
  • , M. D. McManus
  • , A. Rahmati
  • , D. Verscharen
  • , J. Walters
  • , P. L. Whittlesey

Research output: Contribution to journalArticlepeer-review

40 Scopus citations

Abstract

The SWEAP instrument suite on Parker Solar Probe (PSP) has detected numerous proton beams associated with coherent, circularly polarized, ion-scale waves observed by PSP's FIELDS instrument suite. Measurements during PSP Encounters 4-8 revealed pronounced complex shapes in the proton velocity distribution functions (VDFs), in which the tip of the beam undergoes strong perpendicular diffusion, resulting in VDF level contours that resemble a "hammerhead."We refer to these proton beams, with their attendant "hammerhead"features, as the ion strahl. We present an example of these observations occurring simultaneously with a 7 hr ion-scale wave storm and show results from a preliminary attempt at quantifying the occurrence of ion-strahl broadening through three-component ion VDF fitting. We also provide a possible explanation of the ion perpendicular scattering based on quasilinear theory and the resonant scattering of beam ions by parallel-propagating, right circularly polarized, fast magnetosonic/whistler waves.

Original languageEnglish (US)
Article number112
JournalAstrophysical Journal
Volume924
Issue number2
DOIs
StatePublished - Jan 10 2022

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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