NASA SBIR 2010 Solicitation

FORM B - PROPOSAL SUMMARY


PROPOSAL NUMBER: 10-1 S1.04-9109
SUBTOPIC TITLE: Sensor and Detector Technology for Visible, IR, Far IR and Submillimeter
PROPOSAL TITLE: Radiation-Hardened, Substrate-Removed, Metamorphic InGaAs Detector Arrays

SMALL BUSINESS CONCERN (Firm Name, Mail Address, City/State/Zip, Phone)
Voxtel, Inc.
15985 NW Schendel Avenue, Suite 200
Beaverton, OR 97006 - 6703
(971) 223-5646

PRINCIPAL INVESTIGATOR/PROJECT MANAGER (Name, E-mail, Mail Address, City/State/Zip, Phone)
Andrew Huntington
andrewh@voxtel-inc.com
15985 NW Schendel Avenue, Suite 200
Beaverton, OR 97006 - 6703
(971) 223-5646

Estimated Technology Readiness Level (TRL) at beginning and end of contract:
Begin: 3
End: 5

TECHNICAL ABSTRACT (Limit 2000 characters, approximately 200 words)
High-performance radiation-hardened metamorphic InGaAs imaging arrays sensitive from the ultraviolet (UV) through the short-wavelength infrared (SWIR) will be developed. The proposed detector arrays will offer near-BLIP sensitivity, with R0A values comparable to HgCdTe detectors, but with superior sensitivity, better uniformity, lower dark current, and much better pixel yield. Typical InGaAs detectors have little response beyond 1650 nm due to the band edge of the InGaAs alloy composition that is lattice-matched to the InP substrate, and the InP substrate blocks short wavelength response below 950 nm in back-illuminated focal plane arrays. The proposed detector will employ low-dislocation-density metamorphic InGaAs to extend long wavelength response to 2.6 um. Chemical/mechanical substrate removal and a surface doping gradient designed to collect photocarriers generated near the light-entry surface of the detector will extend its short-wavelength response. Prototype single-element detectors and segmented arrays will be demonstrated in Phase I. In Phase II, material quality will be refined through additional manufacturing development, and large area arrays will be fabricated. By the end of Phase II, extended-spectral-range InGaAs imagers based upon the new metamorphic detector and a radiation-hardened readout integrated circuit (ROIC) will be demonstrated.
Voxtel anticipates that its technology will enter the program at TRL=3, finish Phase I at TRL=5, and exit the Phase II program at TRL=6.

POTENTIAL NASA COMMERCIAL APPLICATIONS (Limit 1500 characters, approximately 150 words)
The proposed radiation-hard, extended-spectral-range InGaAs imager technology is applicable to the planned Jupiter Europa Orbiter mission, for which spectral and imaging instruments capable of surviving the Jovian radiation environment are required.

POTENTIAL NON-NASA COMMERCIAL APPLICATIONS (Limit 1500 characters, approximately 150 words)
The innovation has application in a wide range of research, industrial, medical, and military markets. A wide band UV-SWIR imager will benefit applications in the following industries: automobile, security/law enforcement, medical imaging, border patrol, homeland security, military, and others. The innovation can be used to replace both visible imagers and HgCdTe for a variety of applications, including star trackers. For the US military it can be used as a single integrated sensor with high resolution and fast temporal response, with small size, weight and power (SWAP) for the protection of Army rotary and fixed-wing platforms from their three primary threat classes, consisting of MANPAD missiles, ballistic hostile fire and laser targeting devices. These capabilities extend to commercial aircraft protection as well.

TECHNOLOGY TAXONOMY MAPPING (NASA's technology taxonomy has been developed by the SBIR-STTR program to disseminate awareness of proposed and awarded R/R&D in the agency. It is a listing of over 100 technologies, sorted into broad categories, of interest to NASA.)
Detectors (see also Sensors)
Image Capture (Stills/Motion)
Infrared
Materials & Structures (including Optoelectronics)
Materials (Insulator, Semiconductor, Substrate)
Multispectral/Hyperspectral
Optical/Photonic (see also Photonics)
Radiometric
Visible


Form Generated on 09-03-10 12:12