Power spectral density analysis of UV clutter

Patricia K. Murphy; Larry J. Paxton; Daniel Morrison; James F. Carbary; Ching-I. Meng

doi:10.1117/12.140848

22 January 1993 Power spectral density analysis of UV clutter

Patricia K. Murphy, Larry J. Paxton, Daniel Morrison, James F. Carbary, Ching-I. Meng

Proceedings Volume 1764, Ultraviolet Technology IV; (1993) https://doi.org/10.1117/12.140848
Event: San Diego '92, 1992, San Diego, CA, United States

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.

Citation Download Citation

Patricia K. Murphy, Larry J. Paxton, Daniel Morrison, James F. Carbary, and Ching-I. Meng "Power spectral density analysis of UV clutter", Proc. SPIE 1764, Ultraviolet Technology IV, (22 January 1993); https://doi.org/10.1117/12.140848

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