Khlifi M, Nollet M, Paillous P, Bruston P, Raulin F, Bénilan Y, Khanna RK
LISA (Laboratoire Interuniversitaire des Systèmes Atmosphériques), UMR 7583 du CNRS, 61 Av. du Géneral de Gaulle, Créteil Cedex, 94010, France
J Mol Spectrosc. 1999 Apr;194(2):206-210. doi: 10.1006/jmsp.1998.7795.
Laboratory spectral data (peak positions and integrated band intensities) of the infrared bands of acrylonitrile (CH2CHCN) gas in the region 4000-220 cm-1 are presented. Even though CH2CHCN has not yet been identified in Titan's atmosphere, it is among the possible photochemical and cosmic irradiation products of CH4 + N2 chemistry in the atmosphere of Titan. Laboratory simulations of Titan's atmospheric chemistry also give CH2CHCN as a product species. The results of our evaluation of the infrared intensity data provide an upper limit of the stratospheric abundance of CH2CHCN. Copyright 1999 Academic Press.
本文给出了丙烯腈（CH2CHCN）气体在4000 - 220 cm-1区域的红外波段的实验室光谱数据（峰值位置和积分谱带强度）。尽管在土卫六的大气中尚未鉴定出CH2CHCN，但它是土卫六大气中CH4 + N2化学过程可能的光化学和宇宙辐射产物之一。土卫六大气化学的实验室模拟也给出了CH2CHCN作为产物物种。我们对红外强度数据评估的结果给出了平流层中CH2CHCN丰度的上限。版权所有1999年，学术出版社。
