Remote detection of radiation is a difficult problem due to the 1/r2 fall-off. Recent advances in polymer
research and nanoscale fabrication methods along with advances in optical polarimetric remote sensing
systems suggest a solution. The basic device uses a micro-wiregrid infrared polarizer fabricated in
conductive polymer. When the polymer is exposed to hard radiation, its conductivity will be affected and the
polarization properties of the device will change in a corresponding manner. This change in polarization
properties can be determined by optically interrogating the device, possibly from a remote location. We will
report on the development of a radiation-sensitive passive dosimeter polymer with very low optical visibility.
Progress on material development, lithographic fabrication and optical characterization will be presented.
We report on the design, fabrication, and simulation of a four-state pixelated subwavelength optical device that
enables mid-wave infrared (MWIR) or long-wave infrared (LWIR) snapshot polarimetric imaging. The
polarization information can help to classify imaged materials and identify objects of interest for remote sensing
and military applications. The fabricated pixelated polarizers have measured extinction ratios larger than 100:1
for pixel sizes greater than 9 microns by 9 microns, with transmitted signals greater than 50%. That exceeds, by
7 times, previously reported device extinction ratios for 15 micron by 15 micron pixels.
Traditionally, sequential polarimetric imaging sensors produce scenes with polarization information through a
series of assembled images. Snapshot polarimetric imaging collects the spatial distribution of all four Stokes'
parameters simultaneously. In this way any noise due to scene movement from one frame to the next is
eliminated.
In this paper, we will quantify near-field and diffractive effects of the finite pixel apertures upon detection. We
have designed and built an experimental setup that models a pixel within a focal plane array (FPA) to measure
crosstalk from adjacent gold wiregrid micropolarizers. This configuration simulates a snapshot polarization
imaging device where the two substrates are stacked; micropolarizer array substrate on top of an FPA. Modeling
and measured data indicate crosstalk between the adjacent pixels up to a few microns behind the polarizer plane.
Crosstalk between adjacent pixels increases uncertainty in the measured polarization states in a scene of interest.
Measured and simulated data confirm that the extinction ratio of a micropolarizer pixel in a super-cell will be
reduced by 17% when moving the FPA from 0.5 microns to 1.0 microns away from the polarizer. These
changes in extinction ratio are significant since typical glue separation is on the order of 10 microns.
KEYWORDS: Clouds, Image segmentation, Prototyping, Image classification, Infrared imaging, Long wavelength infrared, Signal to noise ratio, Satellites, Thermography, Algorithm development
This paper reports on a novel approach to atmospheric cloud segmentation from a space based multi-spectral pushbroom satellite system. The satellite collects 15 spectral bands ranging from visible, 0.45 um, to long wave infa-red (IR), 10.7um. The images are radiometrically calibrated and have ground sample distances (GSD) of 5 meters for visible to very near IR bands and a GSD of 20 meters for near IR to long wave IR. The algorithm consists of a hybrid-classification system in the sense that supervised and unsupervised networks are used in conjunction. For performance evaluation, a series of numerical comparisons to human derived cloud borders were performed. A set of 33 scenes were selected to represent various climate zones with different land cover from around the world. The algorithm consisted of the following. Band separation was performed to find the band combinations which form significant separation between cloud and background classes. The potential bands are fed into a K-Means clustering algorithm in order to identify areas in the image which have similar centroids. Each cluster is then compared to the cloud and background prototypes using the Jeffries-Matusita distance. A minimum distance is found and each unknown cluster is assigned to their appropriate prototype. A classification rate of 88% was found when using one short wave IR band and one mid-wave IR band. Past investigators have reported segmentation accuracies ranging from 67% to 80%, many of which require human intervention. A sensitivity of 75% and specificity of 90% were reported as well.
The Multispectral Thermal Imager Satellite (MTI), launched on March 12, 2000, is a multispectral pushbroom system that acquires 15 unique spectral bands of data from 0.45-10.7 microns, with resolutions of 5 m for the visible bands and 20 m for the infrared. Scene data are collected on three separate sensor chip assemblies (SCAs) mounted on the focal plane. The process of image registration for MTI satellite imagery therefore requires two separate steps: (1) the multispectral data collected by each SCA must be coregistered and (2) the SCAs must be registered with respect to each other. An automated algorithm was developed to register the MTI imagery. This algorithm performs a phase correlation on edge-maps generated from paired bands of data and then spatial-filters the result to calculate the relative shifts between bands. The process is repeated on every combination of band pairs to generate a vector of coregistration results for each SCA. The three SCAs are then registered to each other using a similar process operating on just one spectral band. The resulting registration values are used to produce a linearly shifted un-resampled coregistered image cube. This study shows the results of 791 image registration attempts using the EdgeReg registration code and compares them to a perfect reference data set of the same images registered manually.
The Multispectral Thermal Imager Satellite (MTI) has been used to test a sub-pixel sampling technique in an effort to obtain higher spatial frequency imagery than that of its original design. The MTI instrument is of particular interest because of its infrared detectors. In this spectral region, the detector size is traditionally the limiting factor in determining the satellite’s ground sampling distance (GSD). Additionally, many over-sampling techniques require flexible command and control of the sensor and spacecraft. The MTI sensor is well suited for this task, as it is the only imaging system on the MTI satellite bus. In this super-sampling technique, MTI is maneuvered such that the data are collected at sub-pixel intervals on the ground. The data are then processed using a deconvolution algorithm using in-scene measured point spread functions (PSF) to produce an image with synthetically-boosted GSD.
The Remote Sensing Group at the University of Arizona has used ground-based test sites for the vicarious calibration of airborne and satellite-based sensors. Past work has focused on high-spatial-resolution sensors that are well-suited to the reflectance-, irradiance-, and radiance-based methods. Application of these methods to the recently launched Moderate Resolution Imaging Spectroradiometer (MODIS) with its lower spatial resolution poses a challenge for vicarious calibration. This work presents the modifications that must be made to reflectance-, irradiance-, and radiance-based approaches in order to use them for MODIS. The reflectance-based method described here relies on ground-based measurements of the reflectance of both large- and small-scale areas of the test site as well as low-level aircraft data to scale the ground-based measurements to the spatial scale of a MODIS pixel. The radiance-based approach relies on a recently-developed airborne, non-imaging radiometer with an 80-m footprint sampling the test site with a predetermined strategy to account for the differing spatial resolutions. Because this sampling strategy depends upon the test site being use, this work describes the two primary test sites of Railroad Valley Playa in Nevada and White Sands Missile Range in New Mexico and the spectral and spatial effects these sites will have on the calibration of MODIS. Early results from application of the reflectance-based method to MODIS using data from April 2000 indicate that the radiometric response of MODIS has not changed significantly.
The Remote Sensing Group at the University of Arizona has been successfully using vicarious calibration techniques since the mid-1980s to calibrate both airborne and satellite-based imaging spectroradiometers using vicarious techniques. These approaches use ground-based measurements of atmospheric and surface properties of a selected test site as input to a radiative transfer code to predict at-sensor radiances at 1-nm intervals from 350-2500 nm for a given sensor overpass. Past work has focused on sensors with view angles less than 30 degrees from nadir but recently-developed sensors use much larger view angles and these sensors will still benefit from vicarious calibrations. However, calibrations at such angles require more accurate atmospheric and surface characterizations. This paper examines the sensitivity of vicarious calibrations at large view angles to uncertainties in the atmospheric characterization and surface bi-directional reflectance. The results show that the inclusion of surface BRDF effects are critical to ensuring accurate results. Furthermore, the uncertainty in the vicarious calibration of a large view angle sensor will be of the same level as or less than that of the near-nadir case when aerosol optical thickness is less than 0.10, the aerosols have low imaginary index, and the solar zenith angle is less than 50 degrees. From the results of this study it is found that currently-used test sites are adequate for use in the vicarious calibration of large view-angle sensors and should give reflectance-based results with uncertainties less than 5%.
The University of Arizona, Optical Sciences Center, Remote Sensing Group is involved with the vicarious calibration of satellite sensors in support of NASA’s Earth Observing System (EOS) program. Sensor calibration coefficients are calculated by comparing sensor DN values to top of the atmosphere (TOA) radiance values, calculated from radiative transfer code (RTC). The RTC output is based on measurements of site spectral reflectance and atmospheric parameters at a selected test site. The bidirectional reflectance distribution function (BRDF) which relates the angular scattering of a given beam of incident radiation on a surface, is an important factor in these radiative transfer calculations. The inclusion of BRDF data into RTC calculations improves the level of accuracy of the vicarious calibration method by up to 5% over some target sites. BRDF data is also valuable in the validation of Multi-Angle Imaging Spectroradiometer (MISR) data sets.
The Remote Sensing Group has developed an imaging radiometer system for ground-based measurements of BRDF. This system relies on a commercially-available 1024- by 1024-pixel silicon CCD array. Angular measurements are accomplished with a 8-mm focal length fisheye lens that has a full 180-degree field of view. Spectral selection is through four interference filters centered at 470, 575, 660 and 835 nm, mounted internally in the fisheye lens. This paper discusses the effect of calibration errors in this camera system on the retrieval of Hapke/Jacquemoud surface parameters from modeled BRDFs. The effect of these retrieved BRDFs on vicarious calibration results is discussed. Data processing schemes for the retrieval of these parameters from BRDF camera data sets are described. Based on these calculations, calibration requirements for digital camera BRDF-retrieval systems are presented.
Keywords: BRDF, CCD, Reflectance, Vicarious Calibration, Digital Camera
Recent results of the vicarious calibration of the Landsat-7 ETM+ sensor are presented based on the reflectance-based vicarious method using results from a smaller test site local to the University of Arizona area. This test site is not as bright, nor as spatially-uniform and as large as typical sites. However, the proximity of the site allows for more frequent calibrations and hopefully a better understanding of the calibration as a function of time. The selection of the test site, its properties, and example results of calibrations at this site are presented. The results from seven dates are presented and show that the ETM+ sensor has been stable to better than 5% since launch. The results from these seven dates have larger variability than those from the large test sites, but agree for the most part to better than 5% with the large test sites.
The Remote Sensing Group of the Optical Science Center at the University of Arizona has developed a four-band, multi- spectral, wide-angle, imaging radiometer for the retrieval of the bi-directional reflectance distribution function (BRDF) for vicarious calibration applications. The system consists of a fisheye lens with four interference filters centered at 470 nm, 575 nm, 660 nm, and 835 nm for spectral selection and an astronomical grade 1024 X 1024-pixel, silicon CCD array. Data taken by the system fit in the array as a nominally 0.2 degree per pixel image. This imaging radiometer system has been used in support of the calibration of Landsat-5 and SPOT- satellite sensors. This paper presents the results of laboratory characterization of the system to determine linearity of the detector, point spread function (PSF) and polarization effects. The linearity study was done on detector array without the lens, using a spherical-integrating source with a 1.5-mm aperture. This aperture simulates a point source for distances larger than 60 cm. Data were collected as both a function of exposure time and distance from the source. The results of these measurements indicate that each detector of the array is linear to better than 0.5%. Assuming a quadratic response improves this fit to better than 0.1% over 88% of the upper end of the detector's dynamic range. The point spread function (PSF) of the lens system was measured using the sphere source and aperture with the full camera system operated at a distance of 700 mm from the source, thus the aperture subtends less than the field of view of one pixel. The PSF was measured for several field angles and the signal level was found to fall to less than 1% of the peak signal within 1.5-degrees (10 pixels) for the on-axis case. The effect of this PSF on the retrieval of modeled BRDFs is shown to be less than 0.2% out to view angles of 70 degrees. The final test presented is one to assess the polarization effects of the lens system by illuminating the camera system with the same spherical-integrating source with a 50-mm aperture with a linear polarizing filter. The degree of polarization of the system is shown to be negligible for on-axis imaging but to have up to a 20% effect for field angles of 70 degrees. The effect of the system polarization on the retrieval of modeled BRDFs is shown to be up to 3% for field angles of 70 degrees off nadir and solar zenith angle of 70 degrees. Polarization response is therefore found to be the greatest source of error in the system. A method to account for polarization effects in digital camera imagery is proposed.
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