Ultimate sensitivity of space-camera imaging devices with particular reference to the slow- scan vidicon.
Ultimate sensitivity of space camera imaging devices with particular reference to slow scan vidicon
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Ultimate sensitivity of space camera imaging devices with particular reference to slow scan vidicon
Panoramic facsimile camera for unmanned space operation providing 360 degrees IR and visible spectrum imagery
Image dissector camera providing high resolving power, photometric fidelity and long life for use in meteorological satellite
ATS-1 spin scan camera experiment for photographic recording of weather motions
ATS-1 spin scan camera experiment for photographic recording of weather motions
In this paper, we discuss the development of this very sensitive long wavelength infrared camera base on a GaAs/AlGaAs QWIP focal plane array and its performance in quantum efficiency, NETD, uniformity and operability.
This paper presents the design and preliminary results of a custom high-speed CCD camera utilizing a Texas Instruments TC237 CCD imager chip with sub-frame window read out.
In this paper, we discuss the development of this very sensitive long wavelength infrared (LWIR) camera based on a GaAs/AlGaAs QWIP focal plane array (FPA) and its performance in quantum efficiency, NE(delta)T, uniformity, and operability.
In this paper, we discuss the development of very sensitive long wavelength infrared (LWIR) GaAs/AlGal-xAs Quantum well infrared photodetectors (QWIPS), fabrication of random reflectors for efficient light coupling, and the demonstration of a LWIR 256 X 256 focal plane array imaging camera. Excellent imagery, with a noise equivalent differential temperature (NE-delta-T) of 25 mK has been achieved.
Long wavelength infrared (LWIR) detectors, 8 (micro)m to 12 (micro)m, are of great interest for a variety of ground-based and space-borne applications. These applications have placed stringent requirements on the performance of the infrared detectors and arrays including high detectivity, low dark current, uniformity, radiation hardness, and low power dissipation. I will discuss the development and progress of GaAs based long-wavelength quantum well infrared photodetectors (QWIPs) to meet those stringent requirements and the demonstration of a 9 (micro)m cutoff 640x480 QUIP focal plane array camera. The noise equivalent temperature difference of the focal plane array is 25 mK at 300 K background and the operating temperature is 70 K.
Recent advancements in CMOS image sensor technology are reviewed, including both passive pixel sensors and active pixel sensors. On- chip analog to digital converters and on-chip timing and control circuits permit realization of an electronic camera-on-a-chip. Highly miniaturized imaging systems based on CMOS image sensor technology are emerging as a competitor to charge-coupled devices for low cost uses.
The Hubble Space Telescope Wide Field Planetary Camera 2 was used to observe Neptune on 28-29 June 1994.
A new multi-axis multi-camera, robotic inspection system has been developed for use inside JPL's thermal/vacuum test chambers wherein satellites and other flight hardware are tested in a simulated space environment.
In this paper, we discuss the development of this very sensitive long-wavelength infrared (LWIR) camera based on a GaAs/AlGaAs QWIP focal plane array (FPA) and its performance in terms of quantum efficiency, NEAT, uniformity, and operability.
In this paper, we discuss the development of this very sensitive long-wavelength infrared (LWIR) camera based on a GaAs/AlGaAs QWIP focal plane array (FPA) and its performance in terms of quantum efficiency, NET, MRDT, uniformity, and operability.
In this paper, we discuss the development of this very sensitive long waelength infrared (LWIR) camera based on a GaAs/AlGaAs QWIP focal plane array (FPA) and its performance in quantum efficiency, NEAT, uniformity, and operability.
This paper discusses the design, development, testing, and demonstration of a highly miniaturized, battery operated, digital wireless camera.
A method is described for accurately calibrating cameras including radial lens distortion, by using points such as those measured from a calibration fixture.