QWIP-based thermal infrared sensor for the Landsat Data Continuity Mission

被引:37
作者
Jhabvala, M. [1 ]
Reuter, D. [1 ]
Choi, K. [2 ]
Jhabvala, C. [1 ]
Sundaram, M. [3 ]
机构
[1] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[2] USA, Res Lab, Adelphi, MD 20783 USA
[3] QmagiQ LLC, Nashua, NH 03063 USA
关键词
QWIP; Infrared detectors; Landsat; Quantum well structures;
D O I
10.1016/j.infrared.2009.05.027
中图分类号
TH7 [仪器、仪表];
学科分类号
0804 ; 080401 ; 081102 ;
摘要
The thermal infrared sensor (TIRS) is a QWIP based instrument intended to supplement the Operational Land Imager (OLI) for the Landsat Data Continuity Mission (LDCM) [See Landsat project description at: http://landsathandbook.gsfc.nasa.gov/handbook/handbook-htmis/chapterl/chapterl.html, [1]. The LDCM is planned to be launched in late 2012 and will continue the 35 year legacy of the Landsat program as Landsat 7 degrades. The LDCM is a joint NASA-US Geological Survey (USGS) mission. The TIRS instrument is a far infrared imager operating in the push broom mode with two IR channels: 10.8 mu m and 12 mu m. The focal plane will contain three 640 x 512 QWIP arrays mounted on a silicon substrate. The readout integrated circuit (ROIC) is intended to be the Indigo 9803. The focal plane operating temperature will be 43 K (nominally). Bandpass filters will define the precise spectral response of the focal plane. Two QWIP designs will be pursued, the corrugated structure and the grating structure. NASA/Goddard, the Army Research Lab and QmagiQ will work closely together to obtain the suite of arrays that will best meet the mission requirements (primarily adequate conversion efficiency at the required wavelengths). This paper will describe the design and fabrication of the TIRS instrument with particular emphasis on the QWIP detectors. The QWIP parameters that are driving the mission requirements include spectral response, dark current, conversion efficiency, read noise, temperature stability, pixel uniformity and pixel yield. Additional mechanical constraints such as co-registration between the three arrays, filter design and assembly and testing will also be discussed. Published by Elsevier B.V.
引用
收藏
页码:424 / 429
页数:6
相关论文
共 5 条
[1]  
CHOI KK, 2003, APS MARCH M AUST TX
[2]  
*FLIR SYST, 1998, COR IND LARG FORM RE
[3]   Development of a 1K x 1K, 8-12 μm QWIP array [J].
Jhabvala, M. ;
Choi, K. K. ;
Monroy, C. ;
La, A. .
INFRARED PHYSICS & TECHNOLOGY, 2007, 50 (2-3) :234-239
[4]   Applications of GaAs quantum well infrared photoconductors at the NASA/Goddard Space Flight Center [J].
Jhabvala, M .
INFRARED PHYSICS & TECHNOLOGY, 2001, 42 (3-5) :363-376
[5]  
USERS GUIDE ISC9803