HITRAN

From Wikipedia, the free encyclopedia

HITRAN - HITRAN is a compilation of spectroscopic parameters that a variety of computer codes use to predict and simulate the transmittance and emission of light in the atmosphere. Original version was compiled by the Air Force Cambridge Research Laboratories (1960's). It is maintained and developed at the Harvard-Smithsonian Center for Astrophysics, Cambridge MA, USA.

[edit] See also:

[edit] References

Rothman L.S., Jacquemart D., Barbe A., Benner D.C., Birk M., Brown L.R., Carleer M.R., Chackerian C., Chance K., Coudert L.H., Dana V., Devi V.M., Flaud J.M., Gamache R.R., Goldman A., Hartmann J.M., Jucks K.W., Maki A.G., Mandin J.Y., Massie S.T., Orphal J., Perrin A., Rinsland C.P., Smith M.A.H., Tennyson J., Tolchenov R.N., Toth R.A., Vander Auwera J., Varanasi P., Wagner G., The HITRAN 2004 molecular spectroscopic database Source: Journal of Quantitative Spectroscopy & Radiative Transfer, 96 (2): 139-204 DEC 1 2005

[edit] External links:

http://www.cfa.harvard.edu/hitran/ Harvard link