Xm. Liu et al., HIGH-RESOLUTION ELECTRON-IMPACT STUDY OF THE FAR-ULTRAVIOLET EMISSION-SPECTRUM OF MOLECULAR-HYDROGEN, The Astrophysical journal. Supplement series, 101(2), 1995, pp. 375-399
The emission spectrum of molecular hydrogen produced by electron-impac
t excitation at 100 eV has been measured in the wavelength range 1140-
1690 Angstrom. High-resolution, optically thin spectra (Delta lambda =
0.136 Angstrom) of the far-ultraviolet( FUV) Lyman and Werner band sy
stems have been obtained with a newly constructed 3 m spectrometer. Sy
nthetic spectral intensities based on the transition probabilities cal
culated by Abgrall et al. are in very good agreement with experimental
ly observed intensities. Previous modeling that utilized Allison & Dal
garno band transition probabilities with Honl-London factors breaks do
wn when the transition moment has significant J dependence or when re-
vibrational coupling is significant. Ro-vibrational perturbation betwe
en v = 14 of the B (1) Sigma(u)(+) state and v = 3 of the C (1) Pi(u),
state and the rotational dependence of the transition moment in the (
6, 12) and (7, 13) bands of the Lyman system are examined. Complete hi
gh-resolution experimental reference FUV spectra, together with the mo
del synthetic spectra based on the Abgrall transition probabilities, a
re presented. An improved calibration standard is obtained, and an acc
urate calibration of the 3 m spectrometer has been achieved.