Laser-Plasma Interaction Experiment for Solar Burst Studies

被引：6

作者：

Marques, J-R ^{[1
]}

Briand, C. ^{[2
]}

Amiranoff, F. ^{[3
]}

Depierreux, S. ^{[4
]}

Grech, M. ^{[1
]}

Lancia, L. ^{[1
]}

Perez, F. ^{[1
]}

Sgattoni, A. ^{[2
,3
]}

Vinci, T. ^{[1
]}

Riconda, C. ^{[3
]}

机构：

[1] Sorbonne Univ, Ecole Polytech, CEA, Inst Polytech Paris,LULI,CNRS, F-91128 Palaiseau, France

[2] Sorbonne Univ, Univ Paris, CNRS, Observ Paris,Univ PSL,LESIA, F-92195 Meudon, France

[3] Sorbonne Univ, LULI, CNRS, CEA,Ecole Polytech,Inst Polytech Paris, F-75255 Paris, France

[4] CEA, DAM, DIF, F-91297 Arpajon, France

来源：

PHYSICAL REVIEW LETTERS | 2020年 / 124卷 / 13期

关键词：

ELECTROMAGNETIC-WAVES; SCATTERING; LANGMUIR; PROPAGATION; SIMULATION; EMISSION; FLASH;

D O I：

10.1103/PhysRevLett.124.135001

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

A new experimental platform based on laser-plasma interaction is proposed to explore the fundamental processes of wave coupling at the origin of interplanetary radio emissions. It is applied to the study of electromagnetic (EM) emission at twice the plasma frequency (2 omega(p)) observed during solar bursts and thought to result from the coalescence of two Langmuir waves (LWs). In the interplanetary medium, the first LW is excited by electron beams, while the second is generated by electrostatic decay of Langmuir waves. In the present experiment, instead of an electron beam, an energetic laser propagating through a plasma excites the primary LW, with characteristics close to those at near-Earth orbit. The EM radiation at 2 omega(p) is observed at different angles. Its intensity, spectral evolution, and polarization confirm the LW-coalescence scenario.

引用

页数：5

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