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The spectroscopic line parameters are compared with the results from HITRAN database.
A spectroscopic line selection process identifies the most appropriate water absorption linepair for thermometry under these conditions.
Calculation of gas absorption spectra uses the HITRAN (HIgh-resolution TRANsmission molecular absorption) database of spectroscopic line parameters and other trace species cross-sections.
Measurements of the individual line positions and intensities are presented for the eight bands, and the final spectroscopic line positions and intensities are compiled as an electronic supplement.
Approaches related to graph theory are investigated which allow a better understanding and yield routes for systematic enlargement and improvement of experimental spectroscopic line lists of molecules.
Further, a set of clear air case studies have been used to test competing formulations of the CO2 line shape, water vapor spectroscopic line parameters and continuum.
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Normal spectroscopic lines, however, are slightly affected by nuclear properties.
The approach uses calculated libraries of transmission spectra at the spectroscopic resolutions of the IFTS, based on the HITRAN database of spectroscopic lines and our own line-by-line radiative transfer model (LBLRTM).
It deteriorates with spectroscopic lines broadening and merging, line intensity decreases and position shifting with decrease in annealing temperature.
This phenomenon is distinct from redshifting because the spectroscopic lines are not shifted to other wavelengths in reddened objects and there is an additional dimming and distortion associated with the phenomenon due to photons being scattered in and out of the line-of-sight.
It should also be stressed that the effective spectroscopic line-width corresponding to B0 field homogeneity is typically limited only by the homogeneity of the magnet at low magnetic fields (our study) rather than by subject-induced perturbations to B0 (i.e., inhomogeneity due to tissue magnetic susceptibility) at high magnetic fields.
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