The earth from space at 2500-3000 A - Brightness and camera design

Details The earth from space at 2500-3000 A - Brightness and camera design The earth from space at 2500-3000 A - Brightness and camera design

Jan 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988spie..932...36l&link_type=abstract

IN: Ultraviolet technology II; Proceedings of the Meeting, Orlando, FL, Apr. 4, 5, 1988 (A89-29476 11-19). Bellingham, WA, Socie

Physics

Cameras, Earth Observations (From Space), Solar Backscatter Uv Spectrometer, Solar Mesosphere Explorer, Spaceborne Photography, Systems Engineering, Brightness, Signal To Noise Ratios, Ultraviolet Reflection

Scientific paper

The brightness of sunlight reflected from the earth was measured in the
UV by the SME and the solar backscatter UV experiment. A graph is
presented of the nadir brightness versus wavelength at a 60-deg solar
zenith angle. The minimum spectral flux density produced by a point
source required to obtain a signal to noise ratio of 3 is determined.

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