Abstract
The Fourier transform spectrum of CH3OH in the 10μm region has been re-examined at higher pressure and path length than heretofore, as part of a program to provide comprehensive CH3OH spectral data for astrophysical and atmospheric applications. With the increase in spectral sensitivity, it has been possible to assign new torsionally excited ν 12 = 1 and ν12 = 2 subbands plus further high-K, ν12 = 0 subbands of the ν8 CO-stretching band. Upper-state term values have been determined, and have been fitted to J(J+1) power-series expansions in order to obtain the excited ν8 substate origins. A variety of weaker subbands from other modes has also been identified in the 10μm spectrum including ν12 = 0, ν 12 = 1, and ν12 = 0←1 torsional subbands of the ν7 in-plane CH3 rock, ν12 = 0←1 and ν12 = 0←2 torsional combination subbands of the ν 6 OH bend, and ν12 = 0←2 subbands of the ν 5 symmetric CH3 bend. Line intensities have been retrieved line-by-line from the spectra. A large set of "unperturbed" ν8 transitions has been modeled using the same type of multi-parameter effective Hamiltonian employed successfully for the ground state, with inclusion of the intensities of a subset of the stronger ν 8 spectral lines in the fitting in order to obtain appropriate transition dipole terms. Together, a 10μm methanol database in HITRAN format has been generated.
| Original language | English |
|---|---|
| Pages (from-to) | 453-470 |
| Number of pages | 18 |
| Journal | Journal of Molecular Spectroscopy |
| Volume | 228 |
| Issue number | 2 SPEC. ISS. |
| DOIs | |
| State | Published - Dec 2004 |
| Externally published | Yes |
Keywords
- Infrared spectra
- Internal rotation
- Line intensities
- Line positions
- Methanol
- Torsional modeling