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Electron-ion recombination measurements in a flowing afterglow plasma.

机译:流动的余辉等离子体中的电子离子重组测量。

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The dissociative recombination of molecular ions with electrons involves the capture of a slow electron by an ion to form an intermediate complex which subsequently dissociates into neutral products. The objective of this work was to measure the recombination coefficients for several ions of interest in planetary ionospheres and in the interstellar medium, to identify some of the neutral products and to measure absolute yields for specific products.; The measurements were performed in a Flowing Afterglow Langmuir Probe-Laser Induced Fluorescence (FALP-LIF) apparatus, which consists of a plasma flow tube with Langmuir probe, mass spectrometer, emission spectroscopy and Laser Induced Fluorescence (LIF) diagnostics. The initial period of work involved building of and extensive testing of the apparatus. The first set of experiments involved measurements of the recombination coefficient for several ions. A novel method of data analysis was employed, and although we were able to confirm previous observations of Adams and Smith that the electron density decay of {dollar}rm Hsb3sp+/Dsb3sp+{dollar} plasmas does not obey the simple recombination law, we found no evidence for persistence of vibrational excitation in the ions invoked by these authors to explain their experimental observations. Instead, we proposed that a three-body process, and not dissociative recombination, was responsible for the experimental observations. For other ions our measurements were in good agreement with previous results, and we found no other examples of "abnormal" recombination.; Spatially resolved emission spectroscopy was used for the identification of electronically excited products for several ions. A recombination-dominated afterglow is a rather complicated system, and for that reason spatially resolved LIF measurements in conjunction with computer modeling of the afterglow were used for measuring absolute yields for the production of ground state OH in v = 0,1 by the dissociative recombination of {dollar}rm Hsb3Osp+, HCOsb2sp+, HNsb2Osp+,{dollar} and HCO{dollar}sp+{dollar} ions. The OH(v = 0) yields were in good agreement with a previous measurement of Herd and Adams while for OH(v = 1) we found serious discrepancies which we attributed to the contribution of extraneous reaction not accounted for in the experiment of the above mentioned authors.
机译:分子离子与电子的解离重组涉及离子捕获慢速电子以形成中间体配合物,该中间体随后解离为中性产物。这项工作的目的是测量行星电离层和星际介质中几种感兴趣离子的复合系数,确定一些中性产物并测量特定产物的绝对产率。测量是在流动余辉Langmuir探针激光诱导荧光(FALP-LIF)仪器中进行的,该仪器由带有Langmuir探针的等离子流管,质谱仪,发射光谱和激光诱导荧光(LIF)诊断程序组成。最初的工作阶段涉及设备的制造和广泛测试。第一组实验涉及几个离子的重组系数的测量。采用了一种新颖的数据分析方法,尽管我们能够证实亚当斯和史密斯的先前观察结果,即{rm} rm Hsb3sp + / Dsb3sp + {dollar}等离子体的电子密度衰减不遵循简单的重组规律,但我们发现没有这些作者为了解释他们的实验观察而调用的离子中,振动激发持续存在的证据。取而代之的是,我们提出了三体过程而不是解离重组来负责实验观察。对于其他离子,我们的测量结果与先前的结果非常吻合,并且我们没有发现“异常”重组的其他例子。空间分辨发射光谱法用于鉴定几种离子的电子激发产物。重组为主的余辉是一个相当复杂的系统,因此,空间分解的LIF测量与余辉的计算机建模一起用于通过解离重组来测量v = 0,1时基态OH的产生的绝对收率{美元} rm Hsb3Osp +,HCOsb2sp +,HNsb2Osp +,{美元}和HCO {美元} sp + {美元}离子。 OH(v = 0)的产量与先前对Herd和Adams的测量结果非常吻合,而对于OH(v = 1),我们发现了严重的差异,这归因于上述实验中未考虑的无关反应的贡献提到的作者。

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