Copious Imaging LLC — National Aeronautics and Space Administration SBIR Phase I: S1

Description

We propose to leverage on-going CPI work to enable a low-cost and low-risk program approach that can be executed as a Phase I SBIR program.nbsp; The scope of this phase I effort is limited to studying the feasibility of some fundamental parameters of a design targeting HOT MWIR and high data-rate FTIR applications.nbsp;nbsp; The following technical aspects of a NASA CPI design will be explored:nbsp;Model the basic CPI ROIC specifications needed to support NASA earth science and inter-planetary missions.nbsp; For HOT IR missions, survey thermo-electric cooler availability and performance as well as the needed LSB size to support shot-noise limited performance.nbsp; This will help form the power budget for the device.nbsp; For FTIR missions, explore availability of ldquo;2-colorrdquo; detector arrays and Avalanche Photodiodes (APD) for meeting stated requirements.nbsp; Evaluate the potential for meeting requirements with or without APD detector arrays.nbsp;Methods for reducing the quantization noise floor, which defines the performance associated with the least significant bit (LSB) of the digitized data. Past designs typically achieve approximately 2000e- as the minimum LSB size.nbsp; Experimental designs have achieved as low as 1e- LSB size, but with noise and linearity issues present.nbsp; The goal of this effort will be to explore new designs and feasibility to achieve between 30 ndash; 500e- LSB size with a low power and high performance front-end design.nbsp;nbsp;nbsp;Design trades to determine what counter bit depth can be accomplished as a function of pixel size to achieve global shuttering, read-while integrate, orthogonal transfer, and ldquo;2-colorrdquo; detector operation.nbsp; Several process nodes will be considered at Fabs found both on- and off-shore.nbsp; ITAR or EAR restrictions may limit the choice of Fabs in the long run, however this limitation will not be a consideration in this study.nbsp;