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Proceedings Paper

Power spectral density analysis of UV clutter
Author(s): Patricia K. Murphy; Larry J. Paxton; Daniel Morrison; James F. Carbary; Ching-I. Meng
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Paper Abstract

While visible and UV range sensors are frequently designed to see the ground, the short-wavelength region known as 'solar-blind' (below 320 nm wavelength) includes emissions originating at altitudes above 30-140 km. The solar-blind range is being investigated for remote sensing of the composition, dynamics, and energetics of the Earth atmosphere, as well as for use in passive sensor acquisition and tracking systems. An examination is presently conducted of the PSD of mid-UV images from a recently launched satellite.

Paper Details

Date Published: 22 January 1993
PDF: 12 pages
Proc. SPIE 1764, Ultraviolet Technology IV, (22 January 1993); doi: 10.1117/12.140848
Show Author Affiliations
Patricia K. Murphy, Johns Hopkins Univ. (United States)
Larry J. Paxton, Johns Hopkins Univ. (United States)
Daniel Morrison, Johns Hopkins Univ. (United States)
James F. Carbary, Johns Hopkins Univ. (United States)
Ching-I. Meng, Johns Hopkins Univ. (United States)


Published in SPIE Proceedings Vol. 1764:
Ultraviolet Technology IV
Robert E. Huffman, Editor(s)

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