The Smithsonian Astrophysical Observatory database SAO92

Details The Smithsonian Astrophysical Observatory database SAO92 The Smithsonian Astrophysical Observatory database SAO92

Oct 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994jqsrt..52..447c&link_type=abstract

Journal of Quantitative Spectroscopy & Radiative Transfer (ISSN 0022-4073), vol. 52, no. 3-4, p. 447-457

Other

16

Data Bases, Data Structures, Earth Atmosphere, Molecular Spectra, Data Processing, Data Reduction, Data Retrieval, Data Transfer (Computers)

Scientific paper

The Smithsonian Astrophysical Observatory (SAO) maintains a molecular line database (the SAO line database) for analysis of atmospheric spectra in the far i.r. and longer-wave mid i.r., from 10-800/cm. This database combines the best currently available line parameters, including the HITRAN molecular database, the JPL submillimeter, millimeter, and microwave spectral line catalog (JPLSMM), and other available measurements and calculations. The current version of the database contains 154,895 lines from H2O, CO2, O3, N2O, CO, CH4, O2 (including the (1)Delta state), NO, SO2, NO2, NH3, HNO3, OH, HF, HCl, HBr, HI, ClO, OCS, H2CO, HOCl, HCN, H2O2, O((3)P), and HO2. The database is available in both HITRAN-type 80 character (SAO92) and 100 character (SAO92A) formats.

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