Electromagnetic emission at the Langmuir frequency from laser interaction with an unmagnetized plasma

We present the first experimental observation of electromagnetic emission at the Langmuir frequency, $ω_p$, resulting from laser-plasma interaction in an underdense and unmagnetised plasma. The emission is spatially resolved and analyzed in polarization. It originates from an electrostatic wave excited by the Raman instability. Despite its frequency being very close to the plasma's cutoff frequency, $ω_{pe}$, this radiation can escape the plasma by following the decreasing slope of the plasma density profile. Radiation at $2ω_p$, is also observed. This experimental platform offers a powerful tool to explore the processes of wave coupling at the origin of some radio solar bursts.

Authors

Publication Details

Journal
arXiv (Cornell University)
Published
2026-10-29
DOI
https://doi.org/10.48550/arxiv.2610.39864
Primary Topic
Laser-Plasma Interactions and Diagnostics
Type
preprint
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preprint

Electromagnetic emission at the Langmuir frequency from laser interaction with an unmagnetized plasma

P. Loiseau, Caterina Riconda, F. Pérez, M. Grech et al.
arXiv (Cornell University)
Laser-Plasma Interactions and Diagnostics
preprint

Electromagnetic emission at the Langmuir frequency from laser interaction with an unmagnetized plasma

P. Loiseau, Caterina Riconda, F. Pérez, M. Grech, L. Lancia, S. Depierreux, C. Briand, J. -R. Marquès
preprint en

Abstract

We present the first experimental observation of electromagnetic emission at the Langmuir frequency, $ω_p$, resulting from laser-plasma interaction in an underdense and unmagnetised plasma. The emission is spatially resolved and analyzed in polarization. It originates from an electrostatic wave excited by the Raman instability. Despite its frequency being very close to the plasma's cutoff frequency, $ω_{pe}$, this radiation can escape the plasma by following the decreasing slope of the plasma density profile. Radiation at $2ω_p$, is also observed. This experimental platform offers a powerful tool to explore the processes of wave coupling at the origin of some radio solar bursts.

arXiv (Cornell University)
Laser-Plasma Interactions and Diagnostics
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