INFRARED ABSORPTION SPECTRUM OF $CH_{4}$ at $7500 cm^{-1}$

Loading...
Thumbnail Image

Date

1967

Journal Title

Journal ISSN

Volume Title

Publisher

Ohio State University

Research Projects

Organizational Units

Journal Issue

Abstract

A high resolution (0.06cm−1) infrared absorption spectrum, obtained using a multi-pass absorption cell and a scanning Ebert spectrometer, is presented for the region in which the combination band ν2+2ν3 of methane is expected to appear. A well-defined Q- and R-branch is observed. The R-branch consists of fine structure components in groups separated by about 10 to 11cm−1. An analysis of the R-branch is made, assuming it belongs to ν2+2ν2, and an explanation based on a successful analysis of other methane bands1 is given for the unexpectedly regular structure. The fine structure components arising from tetrahedral vibration-rotation interactions are examined and compared with other bands of methane.

Description

Support by NASA Contract NAS7-100 is acknowledged by John E. Beckman. Support (in part) by NASA Research Grant NSG-539 is acknowledged by Kenneth Fox. 1 K. Fox, J. Mol. Spectry. 9, 381 (1962).


Author Institution: Space Sciences Division Jet Propulsion Laboratory; Physics Department, The University of Tennessee

Keywords

Citation