A. Goldman

TL;DR: A description and summary of the latest edition of the AFGL HITRAN molecular absorption parameters database are presented and a FORTRAN program is now furnished to allow rapid access to the molecular transitions and for the creation of customized output.

TL;DR: The Atmospheric Trace Molecule Spectroscopy experiment uses a Fourier-transform spectrometer on board the Space Shuttle to record infrared solar occultation spectra of the atmosphere at 0.01-cm(-1) resolution.

TL;DR: The calculations of the partition functions and weighted transition-moments squared in the HITRAN database are reviewed in this paper, and it was found that corrections are needed for several of the hitRAN molecules corrections were needed to the partition function.

TL;DR: In this paper, the authors derived vertical enrichment profiles of stratospheric O(16)O^(16), O(18)O, O(19)O, O(20)O and O(21)O from space-based solar occultation spectra recorded at 0.01 cm−1 resolution by the ATMOS (Atmospheric Trace MOlecule Spectroscopy) Fourier transform infrared (FTIR) spectrometer.

TL;DR: Over 4500 absorption lines have been marked on the spectra and the corresponding line positions tabulated and the high resolution and the low Sun spectra greatly enhance the sensitivity limits for identification of trace constituents.