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

Authors :
Verniero, J. L.
Chandran, B. D. G.
Larson, D. E.
Paulson, K.
Alterman, B. L.
Badman, S.
Bale, S. D.
Bonnell, J. W.
Bowen, T. A.
de Wit, T. Dudok
Kasper, J. C.
Klein, K. G.
Lichko, E.
Livi, R.
McManus, M. D.
Rahmati, A.
Verscharen, D.
Walters, J.
Whittlesey, P. L.
Source :
Astrophysical Journal. 1/10/2022, Vol. 924 Issue 2, p1-10. 10p.
Publication Year :
2022

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. [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
0004637X
Volume :
924
Issue :
2
Database :
Academic Search Index
Journal :
Astrophysical Journal
Publication Type :
Academic Journal
Accession number :
154944644
Full Text :
https://doi.org/10.3847/1538-4357/ac36d5