The smithsonian astrophysical observatory database SAO92

Abstract

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 -1. This database combines the best currently available line parameters, including the HITRAN 1.2 molecular database, the JPL submillimeter, millimeter, and microwave spectral line catalog 3 (JPLSMM), and other available measurements and calculations. The current version of the database contains 154.895 lines from H 2O, CO 2, O 3, N 2O, CO, CH 4, O 2 (including the 1Δ state), NO, SO 2, NO 2, NH 3, HNO 3, OH, HF, HCl, HBr, HI, ClO, OCS, H 2CO, HOCl, HCN, H 2O 2, O( 3 P), and HO 2. The database is available in both HITRAN-type 80 character (SAO92) and 100 character (SAO92A) formats. 1. L.S. Rothman, R.R. Gamache, A. Goldman, L.R. Brown, R.A. Toth, H.M. Pickett, R.L. Poynter, J.-M. Flaud, C. Camy-Peyret, A. Barbe, N. Husson, C.P. Rinsland, and M.A.H. Smith, Appl. Opt. 26, 4058 (1987). 2. L.S. Rothman, R.R. Gamache, R.H. Tipping, C.P. Rinsland, M.A.H. Smith, D. Chris Benner, V. Malathy Devi, J.-M. Flaud, C. Camy-Peyret, A. Perrin, A. Goldman, S.T. Massie, L.R. Brown, and R.A. Toth, JQSRT. 48, 469 (1992). 3. R.L. Poynter and H.M. Pickett, Submillimeter millimeter and microwave spectral line catalog, Publ. 80-23, revision 2, Jet Propulsion Laboratory, Pasadena, CA (1984).