Molecular Constants for the Ground Electronic State of Hydrogen
M. E. Mickelson (Denison University)
The resolution and accuracy of ground-based and space-craft
spectroscopy of solar system bodies has improved dramatically over the
last decade. This has driven the demand for high resolution and high
accuracy laboratory spectroscopic measurements of molecules having
significance for planetary atmospheres. Given the importance of
for planetary atmospheres, the results from the most recent and most
accurate measurements
have been compiled for easy reference. These
include measurements of the line positions, line strengths, shifts in
line position due to density, and self broadening parameters for the
ground electronic state of molecular hydrogen. This paper also presents
an improved set of vibration-rotation constants for the ground
electronic state. A non-linear least squares procedure was used to fit
all of the laboratory measurements for the approximately 35 observed
transitions in the 0-0 through the 5-0 bands. Terms to the fifth
order in the vibrational quantum number v and to the fourth order in
J(J+1) produced a fit with an rms standard deviation of 0.006
.
This work has been supported in part by NASA Grant NAGW 1765 and by Denison University.
References:
Bragg, S. L. 1981, PhD Dissertation, Washington University.
Bragg, S. L., Brault, J. W., and Smith, W. H. 1982, AJP,
263, 999.
Ferguson, D. W., Rao, K. N., Mickelson, M. E.,
and Larson, L. E. 1993, J. Mol. Spectrosc., 160, 315.
Jennings, D. W., Rahn, L. A., and Owyoung, A. 1985,
AJP Let, 291, L15.
Jennings, D. E., Weber, A., and
Brault, J. W. 1987, J. Mol. Spectrosc., 126, 19.
Rao, K. N., Mickelson, M.E., and Trauger, J. T. 1990,
J. Mol. Struct., 217, 85.