TEMPORAL FILTERS FOR TRACKING WEAK SLOW POINT TARGETS IN EVOLVING CLOUD CLUTTER

Citation
J. Silverman et al., TEMPORAL FILTERS FOR TRACKING WEAK SLOW POINT TARGETS IN EVOLVING CLOUD CLUTTER, Infrared physics & technology, 37(6), 1996, pp. 695-710
Citations number
16
Categorie Soggetti
Optics,"Physics, Applied
ISSN journal
13504495
Volume
37
Issue
6
Year of publication
1996
Pages
695 - 710
Database
ISI
SICI code
1350-4495(1996)37:6<695:TFFTWS>2.0.ZU;2-2
Abstract
A class of temporal filters is presented for use with a staring infrar ed camera in detecting and tracking weak point targets moving slowly i n evolving cloud clutter. The generic temporal filter, originally sugg ested by the singular value decomposition of consecutive frame data, i s a zero mean damped sinusoid which can be recursively implemented in the complex plane. From this filter type, a composite triple temporal filter (TTF) is developed, consisting of two sinusoids of different pe riods in sequence followed by a third (averaging) filter. The TTF achi eves impressive cloud clutter suppression by responding strongly to pi xel temporal responses caused by moving point targets and weakly to re sponses caused by cloud edges moving into or out of pixels. An extensi ve database of local airfield scenes with targets of opportunity taken with two laboratory staring IR cameras was used in the design and tes ting of the filters. Issues and trade-offs in choosing the parameters of the TTF are explored by comparing two specific forms of the filter: the first based on a damped sinusoid with a period of 16 frames follo wed by one with a 10 frame period; the second filter has corresponding periods of 40 followed by 30 frames. The first TTF is very effective with targets having velocities from 0.1-0.5 pixels/frame in daytime dr ifting cloud scenes. However, target signal-to-noise values of greater than or equal to 6 are required for detection in white noise (close t o blue-sky conditions), The second TTF is more sensitive to slower, we aker targets in blue-sky or cloudless night scenes; however, in order to operate in daytime cloud scenes, spatial enhancements are required. Results are detailed for some representative scenes and given as well for the total database as signal-to-clutter gain plots based on a new ly formulated antimedian metric.