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不同温度和压力下空气的瑞利-布里渊散射谱

Rayleigh-Brillouin scattering profiles of air at different temperatures and pressures.

作者信息

Gu Ziyu, Witschas Benjamin, van de Water Willem, Ubachs Wim

机构信息

LaserLaB, Department of Physics and Astronomy, VU University Amsterdam, De Boelelaan 1081, 1081 HV Amsterdam, The Netherlands.

出版信息

Appl Opt. 2013 Jul 1;52(19):4640-51. doi: 10.1364/AO.52.004640.

Abstract

Rayleigh-Brillouin (RB) scattering profiles for air have been recorded for the temperature range from 255 to 340 K and the pressure range from 640 to 3300 mbar, covering the conditions relevant for the Earth's atmosphere and for planned atmospheric light detection and ranging (LIDAR) missions. The measurements performed at a wavelength of λ=366.8 nm detect spontaneous RB scattering at a 90° scattering angle from a sensitive intracavity setup, delivering scattering profiles at a 1% rms noise level or better. The experimental results have been compared to a kinetic line-shape model, the acclaimed Tenti S6 model, considered to be most appropriate for such conditions, under the assumption that air can be treated as an effective single-component gas with temperature-scaled values for the relevant macroscopic transport coefficients. The elusive transport coefficient, the bulk viscosity η(b), is effectively derived by a comparing the measurements to the model, yielding an increased trend from 1.0 to 2.5×10(-5) kg·m(-1)·s(-1) for the temperature interval. The calculated (Tenti S6) line shapes are consistent with experimental data at the level of 2%, meeting the requirements for the future RB-scattering LIDAR missions in the Earth's atmosphere. However, the systematic 2% deviation may imply that the model has a limit to describe the finest details of RB scattering in air. Finally, it is demonstrated that the RB scattering data in combination with the Tenti S6 model can be used to retrieve the actual gas temperatures.

摘要

已记录了温度范围为255至340K、压力范围为640至3300毫巴的空气中瑞利 - 布里渊(RB)散射剖面,涵盖了与地球大气以及计划中的大气光探测与测距(激光雷达)任务相关的条件。在波长λ = 366.8nm下进行的测量,通过一个灵敏的腔内装置检测90°散射角处的自发RB散射,以1%均方根噪声水平或更好的水平提供散射剖面。在空气可被视为具有相关宏观输运系数的温度标度值的有效单组分气体这一假设下,将实验结果与一个动力学线形模型,即广受赞誉的Tenti S6模型进行了比较,该模型被认为最适合此类条件。通过将测量结果与模型进行比较,有效地推导出了难以捉摸的输运系数——体黏滞系数η(b),在该温度区间内,其呈现出从1.0到2.5×10⁻⁵kg·m⁻¹·s⁻¹的上升趋势。计算得到的(Tenti S6)线形与实验数据在2%的水平上一致,满足地球大气中未来RB散射激光雷达任务的要求。然而,2%的系统偏差可能意味着该模型在描述空气中RB散射的最精细细节方面存在局限性。最后,证明了RB散射数据与Tenti S6模型相结合可用于反演实际气体温度。

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