Polarization Properties of Whistler Waves From the First 17 Parker Solar Probe Encounters

Abstract We present statistics on the polarization properties of whistler waves in the solar wind down to 0.05 AU (10.75 RS) using data from Parker Solar Probe's first 17 encounters. These properties were previously uncharacterized due to a technical issue affecting one component of the search‐coil magnetometer after Encounter 1. Using a reconstruction technique, we show that whistlers are predominantly quasi‐parallel to the magnetic field across all distances and propagation directions, with 87% exhibiting a propagation angle relative to the background magnetic field below 25. Waves with above 25 are observed with significantly lower amplitudes. Sunward whistlers (including counter‐propagating (CP) cases, where anti‐sunward waves are observed at the same time) statistically exhibit higher normalized amplitudes and frequencies than anti‐sunward whistlers. We discuss generation mechanisms and wave‐particle interactions. Specifically, CP sunward and sunward waves interact via less efficient resonances with Strahl electrons ( eV).

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Publication Details

Journal
Geophysical Research Letters
Published
2025-05-26
DOI
https://doi.org/10.1029/2025gl114622
Citations
3
Primary Topic
Solar and Space Plasma Dynamics
Type
article
Field-Weighted Citation Impact
3.46
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article

Polarization Properties of Whistler Waves From the First 17 Parker Solar Probe Encounters

N. E. Raouafi, J. W. Bonnell, Lucas Colomban, F. S. Mozer et al.
3 citations
Geophysical Research Letters
Solar and Space Plasma Dynamics
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article

Polarization Properties of Whistler Waves From the First 17 Parker Solar Probe Encounters

N. E. Raouafi, J. W. Bonnell, Lucas Colomban, F. S. Mozer, O. V. Agapitov, M. Pulupa, D. Malaspina, Stuart D. Bale, V. Krasnoselskikh, Kyung‐Eun Choi, Thierry Dudok de Wit, M. Kretzschmar
article en
3 citations

Abstract

Abstract We present statistics on the polarization properties of whistler waves in the solar wind down to 0.05 AU (10.75 RS) using data from Parker Solar Probe's first 17 encounters. These properties were previously uncharacterized due to a technical issue affecting one component of the search‐coil magnetometer after Encounter 1. Using a reconstruction technique, we show that whistlers are predominantly quasi‐parallel to the magnetic field across all distances and propagation directions, with 87% exhibiting a propagation angle relative to the background magnetic field below 25. Waves with above 25 are observed with significantly lower amplitudes. Sunward whistlers (including counter‐propagating (CP) cases, where anti‐sunward waves are observed at the same time) statistically exhibit higher normalized amplitudes and frequencies than anti‐sunward whistlers. We discuss generation mechanisms and wave‐particle interactions. Specifically, CP sunward and sunward waves interact via less efficient resonances with Strahl electrons ( eV).

Geophysical Research LettersVol. 52(10)
Université d'Orléans (FR), Centre National de la Recherche Scientifique (FR), University of Colorado Boulder (US), Taras Shevchenko National University of Kyiv (UA), Johns Hopkins University Applied Physics Laboratory (US), Laboratory for Atmospheric and Space Physics (US), Laboratoire de Physique et Chimie de l’Environnement et de l’Espace (FR), International Space Science Institute (CH), University of California, Berkeley (US)
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Solar and Space Plasma Dynamics
3.46
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