Ponderomotive Disturbance of the Solar Wind Velocity before the Fronts of Shock Waves

The solar wind speed perturbation before the fronts of shock waves is theoretically investigated. It is shown that there is a small, but quite detectable deceleration in front of the Earth’s bow shock in the Earth-bound frame of reference. The perturbation is caused by the ponderomotive Abraham force. The Abraham force results from the excitation of fast magnetosonic waves in the foreshock region. The theoretical estimate of the solar wind deceleration by ~10 km/s agrees with measurements of the directional plasma flow velocity on the spacecraft in the foreshock region of the Earth’s bow shock. The use of the velocity addition theorem for interplanetary foreshocks with a structure similar to Earth’s foreshock allows to predict acceleration rather than deceleration of the solar wind in front of interplanetary shocks in the Earth-bound reference frame. The main conclusion is that the theory of ponderomotive plasma modification is of undoubted interest for the interpretation of in situ measurements in the interplanetary environment.

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Publication Details

Journal
Solar System Research
Published
2025-05-20
DOI
https://doi.org/10.1134/s0038094624602093
Primary Topic
Solar and Space Plasma Dynamics
Type
article
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article

Ponderomotive Disturbance of the Solar Wind Velocity before the Fronts of Shock Waves

A. V. Guglielmi, A. S. Potapov, F. Z. Feygin
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Solar System Research
Solar and Space Plasma Dynamics
article

Ponderomotive Disturbance of the Solar Wind Velocity before the Fronts of Shock Waves

A. V. Guglielmi, A. S. Potapov, F. Z. Feygin
article en

Abstract

The solar wind speed perturbation before the fronts of shock waves is theoretically investigated. It is shown that there is a small, but quite detectable deceleration in front of the Earth’s bow shock in the Earth-bound frame of reference. The perturbation is caused by the ponderomotive Abraham force. The Abraham force results from the excitation of fast magnetosonic waves in the foreshock region. The theoretical estimate of the solar wind deceleration by ~10 km/s agrees with measurements of the directional plasma flow velocity on the spacecraft in the foreshock region of the Earth’s bow shock. The use of the velocity addition theorem for interplanetary foreshocks with a structure similar to Earth’s foreshock allows to predict acceleration rather than deceleration of the solar wind in front of interplanetary shocks in the Earth-bound reference frame. The main conclusion is that the theory of ponderomotive plasma modification is of undoubted interest for the interpretation of in situ measurements in the interplanetary environment.

Solar System ResearchVol. 59(5)
Institute of Solar-Terrestrial Physics (RU), Schmidt Institute of Physics of the Earth (RU)
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Solar and Space Plasma Dynamics
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Ponderomotive Disturbance of the Solar Wind Velocity before the Fronts of Shock Waves — A. V. Guglielmi, A. S. Potapov, et al. · Solar System Research (2025) | TGRS Research Map | TGRS