1994
DOI: 10.1117/12.176727
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<title>Hyperspectral observations of space objects</title>

Abstract: The Phillips Laboratory (PL) and the Florida Institute of Technology have developed several advanced visible (0.4 -0.8 jim) Imaging Fourier Transform Spectrometer (IFTS) brassboards. These instruments simultaneously acquire one spatial and one spectral dimension of the hyperspectral image cube, and may be scanned across a scene or configured with a scan mirror to pick up the second spatial dimension. Initial laboratory and field demonsti-ations bave indicated the utility hyperspectral imagery as a diagnostic t… Show more

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Cited by 3 publications
(2 citation statements)
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“…(a) The basic Doppler phenomenon combined with target rigidity enables observer not only to oblain highangular-resolution images, but also to uniquely tag cross-range position of each scattering center attributed to (1) STD does not presume knowledge of the instantaneous PSF and infinite-ensemble statistics models for PSF and its moments, as well as excludes seeing parameter measurement, (2) STD, in application to static astronomical object, permits double statistical averaging, i.e., empirical summing up of the extra-long series of snapshots (or ones extra-separated in time) pertaining to different seeing parameter realizations, ro(t), if a temporal wide-sense-stationarity of the resultant unknown OTF SP takes place, (3) STD unnecessitates the long image sequence registration for each of M monochrome object's signatures and subsequent averaging over many snapshots if object (f.e., booster plume or satellite) is bright enough (At low light level, the price to be paid is that the large series of snapshots is recorded. (a) The basic Doppler phenomenon combined with target rigidity enables observer not only to oblain highangular-resolution images, but also to uniquely tag cross-range position of each scattering center attributed to (1) STD does not presume knowledge of the instantaneous PSF and infinite-ensemble statistics models for PSF and its moments, as well as excludes seeing parameter measurement, (2) STD, in application to static astronomical object, permits double statistical averaging, i.e., empirical summing up of the extra-long series of snapshots (or ones extra-separated in time) pertaining to different seeing parameter realizations, ro(t), if a temporal wide-sense-stationarity of the resultant unknown OTF SP takes place, (3) STD unnecessitates the long image sequence registration for each of M monochrome object's signatures and subsequent averaging over many snapshots if object (f.e., booster plume or satellite) is bright enough (At low light level, the price to be paid is that the large series of snapshots is recorded.…”
Section: Goregistration Of Doppler-shifted Monochrome Imagesmentioning
confidence: 99%
“…(a) The basic Doppler phenomenon combined with target rigidity enables observer not only to oblain highangular-resolution images, but also to uniquely tag cross-range position of each scattering center attributed to (1) STD does not presume knowledge of the instantaneous PSF and infinite-ensemble statistics models for PSF and its moments, as well as excludes seeing parameter measurement, (2) STD, in application to static astronomical object, permits double statistical averaging, i.e., empirical summing up of the extra-long series of snapshots (or ones extra-separated in time) pertaining to different seeing parameter realizations, ro(t), if a temporal wide-sense-stationarity of the resultant unknown OTF SP takes place, (3) STD unnecessitates the long image sequence registration for each of M monochrome object's signatures and subsequent averaging over many snapshots if object (f.e., booster plume or satellite) is bright enough (At low light level, the price to be paid is that the large series of snapshots is recorded. (a) The basic Doppler phenomenon combined with target rigidity enables observer not only to oblain highangular-resolution images, but also to uniquely tag cross-range position of each scattering center attributed to (1) STD does not presume knowledge of the instantaneous PSF and infinite-ensemble statistics models for PSF and its moments, as well as excludes seeing parameter measurement, (2) STD, in application to static astronomical object, permits double statistical averaging, i.e., empirical summing up of the extra-long series of snapshots (or ones extra-separated in time) pertaining to different seeing parameter realizations, ro(t), if a temporal wide-sense-stationarity of the resultant unknown OTF SP takes place, (3) STD unnecessitates the long image sequence registration for each of M monochrome object's signatures and subsequent averaging over many snapshots if object (f.e., booster plume or satellite) is bright enough (At low light level, the price to be paid is that the large series of snapshots is recorded.…”
Section: Goregistration Of Doppler-shifted Monochrome Imagesmentioning
confidence: 99%
“…Hyperspectral imaging systems, which are systems capable of detecting unique spectral information for identification purposes, were first pioneered for use in fields such as the earth and planetary sciences [1] . Since then, hyperspectral imaging systems have emerged in fields including ophthalmology [2][3][4] , oncology [5,6] , fluorescence microscopy [7] , bioinformatics [8] , vascular physiology [9,10] , archeology and art conservation [11] , and even forensic science [12,13] .…”
Section: Introductionmentioning
confidence: 99%