Ion‐Acoustic Waves Associated With Interplanetary Shocks

Abstract Ion‐acoustic waves (IAWs) commonly occur near interplanetary (IP) shocks. These waves are important because of their potential role in the dissipation required for collisionless shocks to exist. We study IAW occurrence statistically at different heliocentric distances using Solar Orbiter to identify the processes responsible for IAW generation near IP shocks. We show that close to IP shocks the occurrence rate of IAW increases and peaks at the ramp. In the upstream region, the IAW activity is highly variable among different shocks and increases with decreasing distance from the Sun. We show that the observed currents near IP shocks are insufficient to reach the threshold for the current‐driven instability. We argue that two‐stream proton distributions and suprathermal electrons are likely sources of the waves.

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Publication Details

Journal
Geophysical Research Letters
Published
2024-08-23
DOI
https://doi.org/10.1029/2024gl109956
Citations
10
Primary Topic
Solar and Space Plasma Dynamics
Type
article
Field-Weighted Citation Impact
3.32

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article

Ion‐Acoustic Waves Associated With Interplanetary Shocks

A. P. Dimmock, P. Louarn, M. André, D. B. Graham et al.
10 citations
Geophysical Research Letters
Solar and Space Plasma Dynamics
3.32
article

Ion‐Acoustic Waves Associated With Interplanetary Shocks

A. P. Dimmock, P. Louarn, M. André, D. B. Graham, Christopher John Owen, M. Morooka, J. Souček, Y. V. Khotyaintsev, David Píša, Georgios Nicolaou, J. J. Boldú, M. Maksimovic, A. Fedorov
article en
10 citations

Abstract

Abstract Ion‐acoustic waves (IAWs) commonly occur near interplanetary (IP) shocks. These waves are important because of their potential role in the dissipation required for collisionless shocks to exist. We study IAW occurrence statistically at different heliocentric distances using Solar Orbiter to identify the processes responsible for IAW generation near IP shocks. We show that close to IP shocks the occurrence rate of IAW increases and peaks at the ramp. In the upstream region, the IAW activity is highly variable among different shocks and increases with decreasing distance from the Sun. We show that the observed currents near IP shocks are insufficient to reach the threshold for the current‐driven instability. We argue that two‐stream proton distributions and suprathermal electrons are likely sources of the waves.

Geophysical Research LettersVol. 51(16)
Uppsala University (SE), Centre National de la Recherche Scientifique (FR), Swedish Institute of Space Physics (SE), Délégation Paris 7 (FR), Université Fédérale de Toulouse Midi-Pyrénées (FR), Université Paris Cité (FR), Université Paris Sciences et Lettres (FR), Sorbonne Université (FR), Sorbonne Paris Cité (FR), Laboratoire d’études spatiales et d’instrumentation en astrophysique (FR), Czech Academy of Sciences, Institute of Atmospheric Physics (CZ), Institut de Recherche en Astrophysique et Planétologie (FR), University College London (GB)
Grantová Agentura České Republiky, Science and Technology Facilities Council
Life below water
Openalex Percentile: Top 8%
Solar and Space Plasma Dynamics
3.32
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