4 Final Report - Emits - ESA
4 Final Report - Emits - ESA
4 Final Report - Emits - ESA
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4 <strong>Final</strong><br />
<strong>Report</strong><br />
Column decoder<br />
4 outputs 4 outputs<br />
Column readout circuit<br />
4 stitched 1k x 1k arrays<br />
15 µm pixel pitch<br />
Column readout circuit<br />
4 outputs 4 outputs<br />
Column decoder<br />
Figure 4.3-9: Architecture for the MWIR CMOS hybrid detector<br />
The 2k x 2k array with 15 µm pitch consists in 4 independent 1000x1000 pixels sub-arrays. Each subblock<br />
is read out via 4 video outputs with a 10 Mpixels/s output rate, so the read out period is 25 ms,<br />
much larger than the max. integration time (2.5 msec for Marine application).<br />
The operating temperature of the detector is dictated by the level of dark current, which can reduce<br />
the useful dynamic range and significantly increase the detection noise. A temperature of 130K is a<br />
typical choice for a 3.7 µm MWIR band.<br />
4.3.3.4 TIR focal plane<br />
As for MWIR, the two candidate technologies are TIR HgCdTe and AlGaAs/GaAs QWIP. From a<br />
qualitative point of view, the trade-off between both materials is identical: better sensitivity for HgCdTe<br />
and better yield / uniformity (spatial and spectral) / temporal stability / cosmetics for QWIP. The<br />
situation is however worse for TIR HgCdTe as its metallurgy complexity is strongly increasing with cutoff<br />
wavelength. A 25 µm pixel pitch is considered as the smallest achievable pixel pitch. The targeted<br />
format of 0.8k x 0.8k pixels has a 28 mm diagonal, larger than the HgCdTe state of the art. The<br />
development of the GIFTS array made by BAe in the US has shown that, despite important<br />
technological and financial efforts, it looks hard to produce with acceptable operability a 20 mm<br />
diagonal HgCdTe 2D array with very long cut-off wavelength. On the other hand, 640x480 pixels<br />
QWIP arrays with 25 µm pitch are currently produced by few manufacturers. The HgCdTe problem is<br />
well known by <strong>ESA</strong> detection experts, particularly in the framework of MTG studies, justifying the two<br />
ways approach proposed by the Agency:<br />
• Improve the weaknesses of HgCdTe, via technological development. This is the object of the<br />
running contract "initial design of thermal infrared detector array for MTG"<br />
• Improve performances of alternative ways. This is the object of the contract "Enhanced<br />
QWIP/Sb-superlattice Array Detector".<br />
About ROIC, the 800x800 pixels format with 25 µm pitch avoids the need for stitching.<br />
An alternative to quantum detectors that could be figured for Fire Monitoring applications (which have<br />
much relaxed noise requirements) is the emerging microbolometer technology.<br />
Page 4-36 Doc. No: GOC-ASG-RP-002<br />
Issue: 2<br />
Astrium GmbH Date: 13.05.2009