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observations of Optically Thin Ozone Lines in the 3-mm Wavelength Range

机译:波长范围为3 mm的光学细臭氧线的观测

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The results of simultaneous observations of two telluric ozone lines with ~96.228- and ~101.736- GHz resonance frequencies are presented. A spectral radiometer of the 3-mm wavelength range that performs the parallel, as well as the sequential, spectrum analysis was employed. The integral atmospheric radiation was recorded in two ~1 -GHz-wide channels separated by ~3 GHz. In order to eliminate fluctuations of atmospheric origin, the spectrometer was calibrated by the atmospheric radiation measured in the wideband channel. The decrement of the optical line thickness for a 25- to 27-MHz detuning from the line center and the excess of the optical line thickness at the line center above the nonresonance component (the absolute line intensity) were measured. It was established that the ratio of the decrements of the observed lines tended to increase by ~30/100 in the period form February 7 to March 24, 1996. The average absolute line intensities were 0.0117 ± 0.0003 neper and 0.0229 ± 0.0014 neper at 96.2 and 101.7 GHz, respectively, which is in good agreement with their theoretical values calculated for the Nizhni Novgorod region.
机译:给出了同时观察两条共振频率分别为〜96.228-和〜101.736-GHz的臭氧臭氧线的结果。使用执行平行以及顺序光谱分析的3毫米波长范围的光谱辐射仪。大气总辐射记录在两个〜1 GHz宽的通道中,相隔〜3 GHz。为了消除大气起源的波动,通过在宽带通道中测量的大气辐射对光谱仪进行了校准。测量了从线路中心失谐25至27 MHz的光线路厚度的减少量,以及非谐振分量上方线路中心处光线路厚度的多余量(绝对线路强度)。可以确定,在1996年2月7日至3月24日期间,所观察到的线的减量比例趋于增加〜30/100。平均绝对线强度在96.2时为0.0117±0.0003奈泊和0.0229±0.0014奈泊。和101.7 GHz,这与下诺夫哥罗德地区计算的理论值非常吻合。

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