Spectral structure of the solar radiation field reflected by the ocean-atmosphere system
(For abstract see issue 14, p. 2388, Accession no. A77-32580)
Engineering topics
Publications and source records attributed to Hovis, W. A., Jr..
(For abstract see issue 14, p. 2388, Accession no. A77-32580)
(For abstract see issue 13, p. 2231, Accession no. A77-31332)
The statistical characteristics of the spectral structure of the brightness field of the ocean/atmosphere system are determined from the spectra of incident radiation and the radiation reflected from the ocean, obtained from aircraft (Conveyor 990) at heights of 0.3 and 10 km above the Atlantic Ocean. Analysis of the spectral structure reveals a weak correlation between atmospheric brightness variations in the 0.4 to 0.5 micron and 0.55 to 0.70 micron regions of the spectrum. This is attributed to the possible influence of variations of the scattering coefficient or optical thickness on the brightness variations (whose sign depends on the predominance of damping or multiple scattering in a given spectral region).
Airborne measurements of the brightness spectrum of the Atlantic Ocean in the wavelength region from 0.4 to 0.7 micron are analyzed. These measurements were made over a tropical region of the Atlantic from an aircraft at heights of 0.3 and 10.5 km during the TROPEX-72 experiment. The results are used to estimate the contribution of the atmosphere to the overall brightness of the ocean-atmosphere system. It is concluded that: (1) the atmosphere decreases the absolute brightness of the ocean by a factor of 5 to 10 and also strongly affects the spectral behavior of solar radiation reflected from the ocean surface; (2) the atmospheric contribution to overall brightness may vary considerably under real conditions; (3) finely dispersed particles and Rayleigh scattering affect the spectral distribution of solar radiation; and (4) the spectral composition of ocean-atmosphere brightness may be completely governed by the atmosphere.
Investigations into the feasibility of sensing ocean color from high altitude for determination of chlorophyll and sediment distributions have been carried out using sensors on NASA aircraft, coordinated with surface measurements carried out by oceanographic vessels. Spectrometer measurements in 1971 and 1972 led to development of an imaging sensor now flying on a NASA U-2 and the Coastal Zone Color Scanner to fly on Nimbus G in 1978. Results of the U-2 effort have shown the imaging sensor to also be of great value in sensing pollutants in the ocean.
IR reflectance of cirrostratus and cirrus clouds and jet contrail measured by spectrometer on high altitude aircraft
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Remote sensing of surface composition of earth
IR spectra taken over desert by aircraft, showing attenuation of upwelling radiation by atmospheric gases and haze
Airborne filter wedge spectrometer recording of earth spectral radient emittance of desert terrain and lava in 8 to 16 microns range
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Optimum wavelength intervals for surface temperature radiometry from total reflectance measurement of common surface minerals
IR spectral reflectance of some common minerals and use in identifying extraterrestrial surfaces
IR reflectivity of iron oxide minerals and use in study of Mars surface
IR reflectivity of polyhydrated ferric oxide measured in connection with Martian surface hydration determination from reflection spectra
Infrared reflectance measurements of igneous rocks, tuffs, and red sandstone from 0.5 to 22 microns to obtain data for use in determining surface composition of planets