Abstract
The principal characteristics of far-infrared (FIR) remote sensing of the atmosphere are: (i) the use of optical techniques at very long wavelengths, (ii) the fact that a relatively cold source, such as the atmosphere, can be observed in emission in the Rayleigh-Jeans region of the black-body distribution, (iii) the fact that many minor stratospheric constituents display a pure rotational spectrum in this region.
© 1991 Optical Society of America
PDF ArticleMore Like This
B.M. Dinelli, M. Carlotti, A. Valboni, and B. Carli
OWE1 Optical Remote Sensing of the Atmosphere (ORS) 1991
James M. Russell
MB7 Optical Remote Sensing of the Atmosphere (ORS) 1990
B. Carli
ThA1 Optical Remote Sensing of the Atmosphere (ORS) 1990