CH3N和CCN自由基射流冷却发射的傅里叶变换观测

C. Brazier, P. Carrick, N. Oliphant, P. Bernath
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引用次数: 0

摘要

甲基硝基自由基的气相光谱首先由Carrick和engleking1观察到,随后由Carrick等人获得了第一个旋转分辨光谱2。使用基特峰傅立叶变换光谱仪,检测由日冕激发的azaide甲基在氦中的超音速膨胀产生的发射,得到了一个旋转分辨光谱,其多普勒增宽限制为0.02 cm-1。然而,与nh3∏−X3∑−带类似的A ~ 3e - X ~ 3a2的过渡仍然非常复杂。由于情况(a) -情况(b)的性质,每个子带允许有27个分支。0- 1,1 -0和1-2子带共有81个分支,唯一可能在观测到的旋转温度15 K时填充的分支。因此,观测到的跃迁是一个多谱线光谱,只有很少的分支可识别。
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Fourier Transform Observation of Jet Cooled Emission from the CH3N and CCN radicals
The gas phase spectrum of the methyl nitrene radical was first observed by Carrick and Engleking1and subsequently the first rotationally resolved spectrum was obtained by Carrick et al.2The use of the Kitt Peak Fourier transform spectrometer, to detect the emission from a corona excited supersonic expansion of methyl azaide in helium, yielded a rotationally resolved spectrum limited by Doppler broadening of 0.02 cm-1. The transition, assigned as A ˜ 3 E- X ˜ 3 A 2 analagous to the A3∏ −X3∑−band of NH, was still extremely complicated however. Due to the case (a) - case (b) nature of the transition 27 branches are allowed for each subband. Giving a total of 81 branches for the 0-1, 1-0 and 1-2 subbands, the only ones likely to be populated at 15 K the observed rotational temperature. Hence the observed transition is a many line spectrum with few branches discernable.
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