The Ultra-Compact Imaging Spectrometer Moon (UCIS-Moon) instrument is a pushbroom shortwave infrared (SWIR) imaging spectrometer prototype developed at NASA’s Jet Propulsion Laboratory (JPL), California Institute of Technology under the Development and Advancement of Lunar Instrumentation (DALI) program. It is designed for integration with a lander or rover for lunar surface science missions. Operating over a 0.6 to 3.6 micron spectral range with 10 nm sampling and a 36 degree field of view, UCIS-Moon is capable of detecting spectral absorptions from common lunar materials, OH species, molecular H2O, water ice, organics, and placing mineral identifications within an established geologic context at the cm to m scale. We discuss instrument assembly, alignment, and measured laboratory optical performance, which meets or exceeds the high-uniformity and high-resolution requirements while achieving a wide spectral range, field of view, and environmental tolerance, with limited mass and power resources. As such, the UCIS-Moon imaging spectrometer is well-suited to address key science questions about lunar geology, the abundance, sources, and sinks of volatiles at the Moon, and the distribution of possible in situ resources for future human exploration.
Northrop Grumman Aerospace Systems (NGAS) has a long
legacy developing and fielding hyperspectral sensors,
including airborne and space based systems covering the
visible through Long Wave Infrared (LWIR) wavelength
ranges. Most recently NGAS has developed the
Hyperspectral Airborne Terrestrial Instrument (HATI) family
of hyperspectral sensors, which are compact airborne
hyperspectral imagers designed to fly on a variety of
platforms and be integrated with other sensors in NGAS's
instrument suite. The current sensor under development is
the HATI-2500, a full range Visible Near Infrared (VNIR)
through Short Wave Infrared (SWIR) instrument covering the
0.4 - 2.5 micron wavelength range with high spectral
resolution (3nm). The system includes a framing camera
integrated with a GPS/INS to provide high-resolution
multispectral imagery and precision geolocation. Its compact
size and flexible acquisition parameters allow HATI-2500 to
be integrated on a large variety of aerial platforms. This
paper describes the HATI-2500 sensor and subsystems and its
expected performance specifications.
Northrop Grumman Aerospace Systems (NGAS) has developed the Hyperspectral Airborne Tactical Instrument (HATI), a compact
airborne hyperspectral imager designed to fly on a variety of platforms and to be integrated with other sensors in the NGAS
instrument suite. HATI has taken part in a variety of missions and flown in conjunction with other NGAS airborne sensors including
the recently-developed NGAS 3-D flash ladar system to demonstrate a multi-sensor data fusion approach. HATI is a push-broom
sensor which gathers information in the 400 nm to 1700 nm wavelength range. Its compact size allows HATI to be mounted on
commercial-of-the-shelf (COTS) aerial photography stabilization platforms and on a large variety of aerial platforms. In its most
recent flight season, the HATI sensor was used to gather data for applications including remote classification of vegetation, forests,
and man-made materials. The HATI instrument has undergone laboratory and in-situ performance validation and radiometric
calibration. This paper describes the HATI sensor and recent data collection campaigns.
A new method of performing vicarious calibration of Visible-Near Infrared (VNIR) sensors has been developed which does not require the manual efforts of a field team to capture surface and atmospheric measurements. Instead, an array of unattended sensors captures the required data on a near continuous basis for recording to a web-based retrieval system. The LSpec (LED Spectrometer) facility, located at Frenchman Flat at the Nevada Test Site, began initial operations in November 2006. The LSpec sensors measure surface reflectance at several VNIR bands, and the accompanying atmospheric measurements allow the production of top-of-atmosphere radiance estimates to calibrate space-borne sensor products. Data are distributed via the Internet, and are available to the calibration community. This paper describes the test site, web-access to the data, and makes use of these data to compute top-of-atmosphere radiance (TOA) and compare to those from the Multi-angle Imaging SpectroRadiometer (MISR) imagery.
A number of factors affect the accuracy of aerosol retrievals from satellite imaging radiometers, including algorithm assumptions, the quality of the associated cloud masks, the prescribed aerosol optical and microphysical models, and calibration uncertainties. In this paper, we highlight a concerted effort by the Terra Multi-angle Imaging SpectroRadiometer (MISR) team to evaluate the accuracy and stability of the instrument's radiometric calibration, with the twofold objective of (1) making improvements in the absolute and relative calibration where supported by multiple lines of evidence, and (2) evaluating the effect of those calibration refinements on aerosol retrievals. Aspects of the instrument's on-board calibrator design, including careful pre-flight handling of the Spectralon diffusers and the novel use of detector-based standards, have contributed to excellent long-term radiometric stability. In addition, multiple methodologies, including comparisons with other Terra sensors, in-flight and laboratory tests involving AirMISR (the airborne counterpart to MISR), lunar observations, camera-to-camera radiometric comparisons at specialized viewing geometries, and investigations using surface-based radiometer data over dark water sites have provided a detailed picture of radiometric performance at the low light levels typical of a large fraction of global aerosol observations. We examine the sensitivity of aerosol property retrievals to small band-to-band and camera-to-camera calibration adjustments, and demonstrate the importance of calibration in meeting climate-quality accuracy requirements. Because combining downward-looking (satellite-based) and upward-looking (surface-based) radiometers can constrain the optical properties of an aerosol column to a greater extent than possible from either vantage point by itself, achieving radiometric consistency, or “closure” between them is essential to establishing a long-term aerosol/climate observing system.
To achieve the research objectives of the Airborne Visible/IR Imaging Spectrometer (AVIRIS), the sensor calibration must be valid while AVIRIS is acquiring data from the airborne platform. The operational environment inside the aircraft differs significantly from that in the AVIRIS laboratory environment where the sensor is calibrated prior to and following each flight season. To independently validate the calibration of AVIRIS in the flight environment an inflight calibration experiment is conducted at least twice each flight season. Results for a calibration experiment held on the 26th of September 1993 are presented.
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