Optimization of smoothing by spectral dispersion with a sinusoidal phase modulation

IF 1.6 3区 物理与天体物理 Q3 PHYSICS, FLUIDS & PLASMAS
Denis Penninckx , Adrien Fusaro , Rodolphe Collin , Gilles Riazuelo , Pascal Loiseau , Osel Thauvin
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引用次数: 0

Abstract

In order to improve the propagation of a laser in a plasma, the intensity profile should be as uniform as possible. For this purpose, smoothing techniques are used. The most commonly used, smoothing by spectral dispersion (SSD), induces temporal fluctuations of the effective amplification length of Stimulated Brillouin scattering (SBS) or Stimulated Raman scattering (SRS). These fluctuations are random from shot to shot and may thus induce unpredictable levels of the efficient laser power used in laser-plasma experiments. Increasing the modulation frequency fm while maintaining the modulation bandwidth strongly reduces these fluctuations and even reduces the average SBS level. However, increasing fm has also an impact on laser propagation within the laser optical components. We show that, as long as chromatic dispersion is precompensated in the front-end, FM-to-AM conversion, a detrimental propagation effect, may remain sufficiently low and that anormal FM-to-AM conversion is not sensitive to the modulation frequency. Hence, there is no important bottleneck to an increase of the modulation frequency.

利用正弦相位调制的频谱色散优化平滑效果
为了改善激光在等离子体中的传播,强度曲线应尽可能均匀。为此,我们使用了平滑技术。最常用的是光谱色散平滑技术(SSD),它会引起受激布里渊散射(SBS)或受激拉曼散射(SRS)有效放大长度的时间波动。这些波动在每次发射时都是随机的,因此可能导致激光等离子体实验中使用的有效激光功率达到不可预测的水平。在保持调制带宽的情况下提高调制频率 fm 可以有效减少这些波动,甚至降低平均 SBS 水平。然而,提高 fm 也会对激光光学元件内的激光传播产生影响。我们的研究表明,只要在前端对色度色散进行预补偿,FM-AM 转换(一种有害的传播效应)就能保持足够低的水平,而且正常的 FM-AM 转换对调制频率并不敏感。因此,提高调制频率并不存在重要瓶颈。
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来源期刊
High Energy Density Physics
High Energy Density Physics PHYSICS, FLUIDS & PLASMAS-
CiteScore
4.20
自引率
6.20%
发文量
13
审稿时长
6-12 weeks
期刊介绍: High Energy Density Physics is an international journal covering original experimental and related theoretical work studying the physics of matter and radiation under extreme conditions. ''High energy density'' is understood to be an energy density exceeding about 1011 J/m3. The editors and the publisher are committed to provide this fast-growing community with a dedicated high quality channel to distribute their original findings. Papers suitable for publication in this journal cover topics in both the warm and hot dense matter regimes, such as laboratory studies relevant to non-LTE kinetics at extreme conditions, planetary interiors, astrophysical phenomena, inertial fusion and includes studies of, for example, material properties and both stable and unstable hydrodynamics. Developments in associated theoretical areas, for example the modelling of strongly coupled, partially degenerate and relativistic plasmas, are also covered.
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