SBIR has passed the midpoint of delivering ten 1024x1024 IR Scene Projector Systems (IRSPs) to the Government. Six systems have been installed at Redstone Technical Test Center (RTTC), Patuxent River, and Edwards Air Force Base. Four more systems are in production and will be shipped by the end of this year. The commercial name of the LFRA IRSP is Mirage XL. This ground breaking projector technology is being leveraged on the Wide Format Resistive Array (WFRA) program and on the Mirage II product. The WFRA IRSP, also known as Mirage HD, features an even larger 1536x768 emitter array and will be in system integration by the end of the year. Mirage II, which also leverages LFRA, is being readied as the next generation 512x512 projector system.
Additional signal processing capabilities have been installed in the LFRA systems. Each system now has full Translation/Rotation Processing (TRP) capability. Systems also have image convolution and 400Hz 1024x512 windowing capabilities.
A persistent question in the infrared scene projection community has been the spectral characteristics of resistive array emission. This paper describes the results of a comprehensive study performed on two resistive array technologies; the Nuclear Optical Dynamic Display System (NODDS) and the Santa Barbara Infrared (SBIR) Large Format Resistive Array (LFRA) product lines. A Fourier Transform Infrared (FTIR) spectral radiometer is used to measure the spectral radiant emission of both resistive array technologies at multiple drive levels and substrate temperatures. Application of the results to scene projection and cross spectral non-uniformity correction is discussed.
KEYWORDS: Cryogenics, Analog electronics, Electronics, Prototyping, Packaging, Interfaces, Mid-IR, Digital electronics, Microelectromechanical systems, Temperature metrology
SBIR has completed the development of the first lot of OASIS emitter arrays and custom packaging for cryogenic IR scene projection applications. OASIS performance requirements include a maximum MWIR apparent temperature of greater than 600 K, with 10-90% radiance rise time of less than 6.5 ms. Four (4) arrays have been packaged, integrated, tested and delivered.
This paper will report on the first measurements taken of the OASIS resistive emitter arrays at both ambient and cryogenic temperatures. This paper will also provide a discussion of the OASIS cryogenic projector/electronics module (Cryo-PEM) design. We will also describe the novel thermal design employed within the array package and Cryo-PEM assemblies, which allows OASIS to produce radiometrically accurate imagery with reduced thermal lag/gradient artifacts compared to legacy Honeywell cryogenic IRSP assemblies. As OASIS supports both analog and digital input, we will discuss the differences between the two modes in terms of system integration, support electronics and overall array performance.
SBIR has completed design and development of prototype emitter arrays and is completing custom cryogenic vacuum device packaging and support electronics for the Optimized Arrays for Space-background Infrared Simulation (OASIS) program. The OASIS array is a 512 x 512 device featuring high output dynamic range, a selectable analog/digital scene data interface, and the capability to operate from cryogenic to ambient substrate temperatures - thereby providing an enabling technology for projection of simulated radiance of space-background scenes. Prototype emitter production has been completed at RTI International in support of initial deliveries. The OASIS array package incorporates novel electrical bussing schemes optimized for the OASIS RIIC and a modular architecture to allow user re-configuration of both window and emitter shield. The OASIS package leverages LFRA operation features, and supports both ambient and cryogenic chamber-based operation with a minimum of mechanical and electrical re-configuration. The OASIS close support electronics (CSE) supports both analog and digital input data modes, while providing easy electronic connection between arrays installed in the cryogenic chamber and the external control and scene-generation systems. We present a technical overview of the OASIS array/package and CSE designs, and will report on measured radiometric performance from prototype OASIS arrays.
SBIR has completed development of the Large Format Resistive Array (LFRA) Infrared Scene Projector (IRSP) and shipped the first production system. Nine more systems are in production and will be shipped to several US Government customers on approximately six week centers. The commercial name of the LFRA IRSP is Mirage XL. System performance meets a broad range of program requirements and SBIR has been extremely successful in producing this ground breaking projector. Tests performed on System #1 reveal broad compliance to the specification and, in particular, outstanding emitter array performance. Key emitter requirements that have been met or exceeded include Operability, Maximum Apparent Temperature, and Array Uniformity. Key System specifications are:
Large-format emitter array (1024x1024);
High maximum apparent temperature (>700K);
200 Hz full-frame operation;
400 Hz static window mode (1024x512);
Non Uniformity (uncorrected) <10%.
This paper provides a procedure for radiometric calibration of infrared target projectors using the RAD-9000 MWIR/LWIR spectral radiometer - a high-performance instrument supporting extremely accurate absolute and relative radiometric calibration of EO test systems. We describe the rationale for radiometric calibration, an analysis of error sources typically encountered by investigators during calibration of infrared imaging cameras when using target
projectors, and a strategy for performing an absolute system end-to-end radiometric calibration with emphasis on high accuracy and ease of use.
The leading IR scene projection (IRSP) device technology, resistive emitter arrays, has grown from its early roots in the uncooled microbolometer community into a separate and highly specialized field of its own. IRSP systems incorporating "microbolometers running backwards" are critical tools now ubiquitous in laboratory testing and evaluation of high performance IR sensors and their embedded algorithms. Adoption of IRSPs has reduced the scope of flight/field testing, producing dramatic resource savings and strong system development advantages.
Modern IRSP systems provide the capability to project high-resolution (1024 x 1024), high-temperature (750 K) dynamic MWIR-LWIR imagery at frame rates up to 200 Hz, with 16-bit input resolution. Novel IRSP systems are now being developed to test advanced FPAs and sensors requiring wide-format (768 x 1536), cryogenic background (50-80 K), fast-framing (400 Hz), and/or very high-temperature (2500 K) dynamic IR simulation in order to be properly evaluated.
The ongoing cycle of sensor improvement and test system evolution is perfectly illustrated by the parallel development of IRSP and emerging FPA/sensor technologies. The cross-pollination of technology between the sensor and projector domains continues to bring innovation to both communities. Technological trends related to semiconductor and microelectrical-mechanical system (MEMS) device fabrication, real-time digital video processing, and EO system design are being exploited by both sensor and projector developers alike - with advantages realized by both.
This paper presents a lighthearted overview of the technical evolution of IRSP from its early microbolometer roots, discusses current and emerging IRSP capabilities, illustrates the device-level to system-level synergy between sensors and projectors, and offers a peek into the advanced EO simulation capabilities and technologies which will be required to address emerging FPA and sensor trends.
SBIR's family of MIRAGE infrared scene projection systems is undergoing significant growth and expansion. The first two lots of production IR emitters have completed fabrication at Microelectronics Center of North Carolina/Research and Development Institute (MCNC-RDI), and the next round(s) of emitter production has begun. These latest emitter arrays support programs such as Large Format Resistive Array (LFRA), Optimized Array for Space-based Infrared Simulation (OASIS), MIRAGE 1.5, and MIRAGE II. We present the latest performance data on emitters fabricated at MCNC-RDI, plus integrated system performance on recently completed IRSP systems. Teamed with FLIR Systems/Indigo Operations, SBIR and the Tri-Services IRSP Working Group have completed development of the CMOS Read-In Integrated Circuit (RIIC) portion of the Wide Format Resistive Array (WFRA) program-to extend LFRA performance to a 768 x 1536 "wide screen" projection configuration. WFRA RIIC architecture and performance is presented. Finally, we summarize development of the LFRA Digital Emitter Engine (DEE) and OASIS cryogenic package assemblies, the next-generation Command & Control Electronics (C&CE).
This paper provides an update on the RAD9000 MWIR/LWIR spectral radiometer: a high-performance instrument supporting extremely accurate absolute and relative radiometric calibration of EO test systems. The system features an all-reflective optical system, internal and external thermal reference sources, a visible camera-based sighting/alignment capability, modular MWIR and LWIR detector/filter subassemblies, flexible control/display software, and a sophisticated graphical user interface (GUI). We present prototype performance data describing the instrument's thermal sensitivity, radiometric accuracy, spectral resolution, calibration, and other key parameters.
This paper presents the latest developments in instrumentation for military laser range-finder/designator (LRF/D) test and evaluation. SBIR has completed development of two new laser test modules designed to support a wide range of laser measurements including range accuracy and receiver sensitivity, pulse energy and temporal characteristics, beam spatial/angular characteristics, and VIS/IR to laser co-boresighting. The new Laser Energy Module (LEM) provides automated, variable attenuation of UUT laser energy, and performs measurement of beam amplitude and temporal characteristics. The new Laser/Boresight Module (LBM) supports range simulation and receiver sensitivity measurement, performs UUT laser beam analysis (divergence, satellite beams, etc), and supports high-accuracy co-boresighting of VIS, IR, and laser UUT subsystems. The LBM includes a three-color, fiber-coupled laser source (1064, 1540, and 1570 nm), a sophisticated fiber-optic module (FOM) for output energy amplitude modulation, a 1-2 μm SWIR camera, and a variety of advanced triggering and range simulation functions.
KEYWORDS: Sensors, Calibration, Optical filters, Control systems, Temperature metrology, Radiometry, Infrared radiation, Radio optics, Mid-IR, Long wavelength infrared
Santa Barbara Infrared, Inc (SBIR) has developed a dual-band infrared spectroradiometer for highly accurate radiometric calibration of electro-optical (EO) test stations, light sources, and optical surfaces. The "RAD-9000" design covers the 3-5 mm and 8-12 mm spectral bands, provides thermal sensitivity of better than 40 mK, supports object temperatures from 278-373 K, and delivers better than 2% spectral resolution (Dl/l). The RAD-9000 features computer-controlled operation, an intuitive graphical user interface (GUI), motorized focus adjustment, VIS-CCD sighting/alignment capability, less than 2 mrad detector IFOV, and an internal ambient reference for background subtraction and enhanced stability.
In addition to high-performance relative radiometry, the RAD-9000 offers a high degree of absolute radiometric accuracy by utilizing a dedicated radiometric reference module. The reference module incorporates two 8-inch, variable temperature, high-emissivity extended sources to provide a stable, accurate absolute radiometric reference external to the main optics.
Santa Barbara Infrared's (SBIR) family of MIRAGE infrared scene projection systems is undergoing significant growth and expansion. The first lot of production IR emitters is in fabrication at Microelectronics Center of North Carolina/Research and Development Institute (MCNC-RDI), the state-of-the-art MEMS foundry and R&D center which completed prototype fabrication in early 2003. The latest emitter arrays are being produced in support of programs such as Large Format Resistive Array (LFRA) and MIRAGE 1.5, MIRAGE II, and OASIS. The goal of these new development programs is to increase maximum scene temperature, decrease radiance rise time, support cryogenic operation, and improve operability and yield. After having completed an extremely successful prototype run in 2003, SBIR and MCNC-RDI have implemented a variety of emitter process improvements aimed at maximizing performance and process yield. SBIR has also completed development and integration of the next-generation MIRAGE command and control electronics (C&CE), an upgraded calibration radiometry system (CRS), and has developed test equipment and facilities for use in MIRAGE device wafer probing, test, evaluation, diagnostic, and assembly processes. We present the latest emitter performance data, an overview of emitter foundry processing and packaging improvements, and an update on MIRAGE II, LFRA, and OASIS development programs.
The DoD has determined that standardization of Electro-Optic testing is beneficial to current and future Automated Test Systems (ATS). Adopting standards will reduce cost of ownership of ATS and will improve flexibility through interoperability of ATS. The current state of the art in instrument standardization is the Interchangeable Virtual Instrument (IVI) Foundation standards already adopted for commercial standard test equipment such as Digital Multimeters. The Navy has formed a working group entitled “EO Software Working Group” that is meeting quarterly to come up with appropriate IVI standards for EO testing. Considerable progress has been made over the past two years. The first specification, for Blackbodies, has been produced (draft version). Over the next 18 months this will be finalized and submitted to the IVI Standards Committee for formal approval. In addition, other specifications for EO testing will be developed and submitted for formal incorporation. This paper will describe the needs for standardization in the ATS community and the progress in EO IVI standards.
SBIR's MIRAGE Infrared scene projector continues to break new ground in the area of dynamic IR scene projection. In July 2001, SBIR reached an exclusive licensing agreement with Honeywell Research Laboratories to fabricate emitter arrays using their industry standard process. SBIR has moved out aggressively to bring the benefits of this process coupled with the MIRAGE CMOS to the IR projection community. This paper discusses emitter array performance from Honeywell devices fabricated on legacy MIRAGE CMOS. It also discusses SBIR's upgraded CMOS plans, which will take advantage of the Honeywell process to extend the state-of-the-art of IR scene projector performance.
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