This model was developed to provide a means for comparative assessments of HgCdTe FPA's and sensors operating in the infrared spectral bands that coincide with the atmospheric windows -(SW1(1.5-1.8µ), SW2(2-2.5µ), MW(3-5µ), and LW(8-12µ). As a true imaging model it also functions as an assessment tool for single-band imagery and for multi-color imagery. The HgCdTe model characterizes both n-on-p and p-on-n homojunctions and heterostructures. Diffusion and depletion dark currents and RoA's are calculated for the three common configurations (mesa heterojunction, planar ionimplanted or diffused junction, and the vertically integrated photodiode). The model places the specified FPA into an optical system, evaluates system performance (NEI, NETD, MRTD, and SNR) and creates two-point corrected imagery complete with 3D noise image effects. This model was exercised here as a predictive tool for performance of state-ofthe-art detector arrays in optical systems in the four spectral bands (atmospheric windows) from the SW to the MW (1.5-1.8, 2.0-2.5, 3.4-4.2 and 4.5-5.0 um) which are the bands commonly considered for hot target and plume exhaust detection. Results from the literature and model runs for various target and scene sets show promise for HgCdTe FPA's and sensors developed for the 2-2.5 um band for a variety of missions such as threat detection from UAV or satellite platforms, perimeter defense, and high-altitude intercepts.
INTRODUCTIONAssessments of scenes and targets in the MW (3-5µ) and LW (8-12µ) are common and fairly straightforward as radiances are simple functions of the materials' emittances and temperatures. The SW1 (1.5-1.8µ) and SW2 (2-2.5µ) bands are more complex as reflected light from natural and artificial sources plays a major role in determining the background radiance. The scene contrast generated here is from a combination of SW reflectance values and the level of SW illumination which can come from a variety of sources. In the SW1 band, the NETD is irrelevant and should be replaced by a figure-of-merit that specifies reflectivity differences under scene radiance levels. The SW1 band has been investigated and utilized as a new band for tactical vehicle and personnel imaging, in addition to the shorter wavelength image intensifier band. SW1 background radiance, however, is quite variable and under rural, cloudy nighttime skies, passive SW1 sensors are ineffective as imagers. InGaAs focal plane arrays are the current choice in this band; however, HgCdTe can provide similar performance but at a higher cost. The SW2 atmospheric window at 2-2.5µ and high-quality HgCdTe FPA's at this wavelength provide an opportunity to utilize this band for imaging or missile detection. This study shows that many missile plumes and jet engines emit well in this band, atmospheric transmittances are high, SW2 detectors are unaffected by hot dome or window temperatures, and large-format, high-quality and lower cost HgCdTe on silicon FPA's have been developed whose performance is adequate at operating temperatures from ...