Open Access
Add to BibSonomyAbstract
During November of 1991, a Fourier transform infrared spectrometer was used to measure emission spectra of the sky under both clear and cloudy conditions. Spectral resolution was 1 cm−1 over the region from 500 to 2000 cm−1. These spectra were calibrated by using two blackbody cavities, one at 77 K and the other at ambient temperature. These spectra will be compared with spectra calculated by using radiosonde profiles of the atmosphere and the U.S. Air Force radiative transfer code MODTRAN.
© 1992 Optical Society of America
PDF ArticleMore Like This
A. Goldman, F. J. Murcray, R. D. Blatherwick, F. H. Murcray, J. J. Kosters, S. J. David, D. G. Murcray, and C. P. Rinsland
FY3 OSA Annual Meeting (FIO) 1992
A. Goldman, F.J. Murcray, R.D. Blatherwick, F.H. Murcray, J.J. Kosters, F.S. Bonomo, S.J. David, D.G. Murcray, and C.P. Rinsland
FD5 High Resolution Fourier Transform Spectroscopy (FTS) 1992
A. Goldman, F.J. Murcray, R.D. Blatherwick, F.H. Murcray, J.J. Kosters, F.S. Bonomo, S.J. David, D.G. Murcray, and C.P. Rinsland
ThD.1 Optical Remote Sensing of the Atmosphere (ORS) 1993