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首页> 外文期刊>Atmospheric Measurement Techniques >Towards imaging of atmospheric trace gases using Fabry-Perot interferometer correlation spectroscopy in the UV and visible spectral range
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Towards imaging of atmospheric trace gases using Fabry-Perot interferometer correlation spectroscopy in the UV and visible spectral range

机译:在UV和可见光谱范围内使用法布里 - 珀罗干涉仪相关光谱法对大气痕量气体成像

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摘要

Many processes in the lower atmosphere including transport, turbulent mixing and chemical conversions happen on timescales of the order of seconds (e.g. at point sources). Remote sensing of atmospheric trace gases in the UV and visible spectral range (UV-Vis) commonly uses dispersive spectroscopy (e.g. differential optical absorption spectroscopy, DOAS). The recorded spectra allow for the direct identification, separation and quantification of narrow-band absorption of trace gases. However, these techniques are typically limited to a single viewing direction and limited by the light throughput of the spectrometer set-up. While two-dimensional imaging is possible by spatial scanning, the temporal resolution remains poor (often several minutes per image). Therefore, processes on timescales of seconds cannot be directly resolved by state-of-the-art dispersive methods.
机译:较低气氛中的许多过程包括运输,湍流的混合和化学转换,在秒的时间表上发生(例如,在点来源)。 遥感UV和可见光谱范围(UV-VI)中的大气痕量气体通常使用分散光谱(例如差分光学吸收光谱,DOA)。 记录的光谱允许直接识别,分离和定量痕量气体吸收的痕量气体。 然而,这些技术通常限于单个观察方向和受光谱仪设置的光吞吐量的限制。 虽然通过空间扫描可以实现二维成像,但时间分辨率仍然差(通常每张图像几分钟)。 因此,不能通过最先进的分散方法直接解决时间震中的过程。

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