The Improved Radiometric calibration of land Imaging Systems or IRIS is a compact full-spectrum calibration system that reduces the size, weight and power of conventional on-board radiometric sources into a single flat panel format by combining both carbon nanotube and LED technology within a Jones source design. Introduced in this presentation is a methodology that maintains in-flight traceability through a fusion of the on-board IRIS LED reference with Labsphere’s FLARE vicarious calibration system. The process known as IRIS-V provides SI traceability of the on-board VSWIR calibration system through the mission's lifetime without impacting operational land or coastal image collection.
Labsphere has created automated vicarious calibration sites using convex mirror technology in the new FLARE (Field Line-of-sight Automated Radiance Exposure) Network. FLARE has been operational for over two years, with network expansion and performance validation against industry standards and common methods for calibration and validation (cal/val) of 350-2500nm optical Earth Observation Systems (EOS). The FLARE point sources provide absolute and traceable data, creating a new tool in harmonization of satellites with ground sampling distances (GSD) of 0.3m to 60m. This paper provides an overview of the FLARE system and presents findings and improvements in operational hardware and software performance. Once commissioned, all FLARE nodes have been repeatedly targeting Landsat 8, Landsat 9 (starting 2022), and Sentinel 2A/B. This has produced a multi-year archive of radiometric and spatial calibration imagery. Landsat and Sentinel are the premier reference programs for Earth Observation performance and utilize both on-board calibration equipment and on-ground reference sites such as RadCalNet and PICS. This work compares the results of the FLARE technique to current official radiometric coefficients and spatial performance metrics for these satellites. Discussion will center on new insights gleaned from the archive analysis and FLARE’s contribution to the community’s capability for data fusion, instrument harmonization, and the potential to support the concept of Analysis Ready Data (ARD) for easier data use and information extraction. Finally, the future progression of FLARE sites, capabilities, and activities will be outlined.
The NASA Earth Science Technology Office (ESTO) funded Improved Radiometric calibration of future land Imaging Systems (IRIS) Advanced Technology Development (ATD) is developing and demonstrating technology to simplify onboard calibration systems and reduce risk, cost, size, mass, and development time for next generation small satellite instruments, while meeting or exceeding current capabilities. IRIS addresses this objective in two different, but complementary ways. The first way involves designing and building an ultra-compact, full spectrum (0.4-2.3 µm and 4- 13 µm) end-to-end calibration source and testing this source with the existing NASA ESTO Advanced Technology Land Imaging Spectroradiometer-Prototype (ATLIS-P) built by Raytheon. IRIS extends ATLIS-P by reducing volume of the onboard calibration assembly by 90% relative to current flight systems using an innovative, full-spectrum Jones source. IRIS will demonstrate a functionally complete full-spectrum prototype land imager with much reduced size and mass by verifying calibration performance across the full spectral range and full imager field of view by comparison with well-understood NIST traceable full aperture laboratory sources. The second way involves in-flight absolute solar radiometric calibration of L8 and L9 OLI onboard lamp assemblies based on Raytheon’s patented Specular Array Calibration (SPARC) method. SPARC uses spherical convex mirrors to create a collection of “solar stars” with identical spectra and well-defined radiometric properties directly traceable to the exoatmospheric solar spectral constant. This IRIS-Vicarious (IRIS-V) aspect of the project involving SPARC site observations provides in-flight absolute calibration and image quality validation. IRIS-V intends to image a commercial SPARC site on Mauna Loa developed by Labsphere. NASA ESTO funded this work through grant 80NSSC20K1676 to Raytheon Company.
Labsphere has created automated vicarious calibration sites using the SPecular Array Radiometric Calibration (SPARC) mirror technology in the new Field Line-of-sight Automated Radiance Exposure (FLARE) network. A short introduction to FLARE and SPARC will be given showing how arduous field ground calibrations can now be done remotely through FLARE nodes via an internet portal. Preliminary results of the performance of the system’s absolute radiometric and spatial calibration capability were published in 2020, demonstrating validation and uncertainty against current methods of remote calibration and spatial and geometric performance against edge and line targets. This paper will describe FLARE’s impact to ongoing evaluation and maturation of automated analysis processes for all data processing levels for space satellite and UAV imagers.
The SPecular Array Radiometric Calibration (SPARC) methodology uses convex mirrors to relay an image of the sun to a satellite, airborne sensor, or other Earth Observation platform. The signal created by SPARC can be used to derive absolute, traceable calibration coefficients of Earth remote sensing systems in the solar reflective spectrum. This technology has been incorporated into an automated, on-demand commercial calibration network called FLARE (Field Line-of-site Automated Radiance Exposure). The first station, or node, has been successfully commissioned and tested with several government and commercial satellites. Radiometric performance is being validated against existing calibration factors for Sentinel 2A and diffuse target methodologies. A radiometric uncertainty budget indicates conservative 1-sigma uncertainties that are comparable to or below existing vicarious cal/val methods for the VIS-NIR wavelengths. In addition to radiometric performance, SPARC and FLARE can be utilized for characterization of a sensor’s spatial performance. Line and Point Spread Functions, and resulting Modulation Transfer Functions, derived with SPARC mirrors are virtually identical to those measured with traditional diffuse edge targets. Ongoing development of the FLARE network includes improved radiometric calibration, web portal scheduling and data access, and planned expansion of the network to Railroad Valley Playa and Mauna Loa, Hawaii.
This paper describes a Coastal Water Camera System (CWCS) that provides the wide field of view, high spatial resolution and high SNR imaging spectroradiometry at ultraviolet (UV) through near infrared (NIR) wavelengths needed to meet challenging requirements for coastal water measurements from polar sun synchronous orbit (SSO). CWCS uses a flexible, modular architecture that can be scaled to fit within a wide range of mission resource constraints. CWCS includes 12 spectral bands selected from across a 375-960 nm spectral range. CWCS delivers the high spatial resolution (~50 m), high SNR (>775 in ~100 m pixel) UV-NIR measurements across a wide (~540 km) swath needed for effective coastal water imaging.
Resolving the complexity of coastal and estuarine waters requires high spatial resolution, hyperspectral
imaging spectroradiometry. Hyperspectral measurements also provide capability for measuring bathymetry
and bottom types in optically shallow water and for detailed cross calibration with other instruments in
polar and geosynchronous orbit. This paper reports on recent design studies for a hyperspectral Coastal
Imager (CI - pronounced "sea") that measures key data products from sun synchronous orbit. These
products include water-leaving radiances in the near-ultraviolet, visible and near-infrared for separation of
absorbing and scattering coastal water constituents and for calculation of chlorophyll fluorescence. In
addition, CI measures spectral radiances in the near-infrared and shortwave infrared for atmospheric
corrections while also measuring cloud radiances without saturation to enable more accurate removal of
instrument stray light effects. CI provides contiguous spectral coverage from 380 to 2500 nm at 20 m
GIFOV at nadir across 5000+ km2 scenes with spectral sampling, radiometric sensitivity and calibration
performance needed to meet the demanding requirements of coastal imaging. This paper describes the CI
design, including concepts of operation for data collection, calibration (radiometric, spectral and spatial),
onboard processing and data transmission to Earth. Performance characteristics for the instrument and all
major subsystems including the optics, focal plane assemblies, onboard calibration, onboard processing and
thermal subsystem are presented along with performance predictions for instrument sensitivity and
calibration. Initial estimates of size, mass, power and data rate are presented.
Physics-based exploitation of image data from Earth observing sensors requires knowledge of the accuracy, stability and
repeatability of a sensor's radiometric response within its in-flight environment. Vicarious radiometric calibration
techniques, using terrestrial targets, provide an effective approach to obtaining this knowledge by measuring system
performance under actual operational conditions. This paper introduces a new capability for performing the vicarious
radiometric calibration of high spatial resolution sensors. The SPecular Array Radiometric Calibration (SPARC) method
employs convex mirrors to create two arrays of calibration targets for deriving absolute calibration coefficients of Earth
remote sensing systems in the solar reflective spectrum. The first is an array of single mirrors used to oversample the
sensor's point spread function (PSF) providing necessary spatial quality information needed to perform the radiometric
calibration of a sensor when viewing small targets. The second is a set of panels consisting of multiple mirrors designed
to stimulate detector response with known at-sensor irradiance traceable to the exo-atmospheric solar spectral constant.
The outcome is improved radiometric performance knowledge compared to other in-flight vicarious techniques through
reduced uncertainties in target reflectance, atmospheric effects, and temporal variability. The only ground truth needed is
the measurement of atmospheric transmittance. In addition, the simplification of calibration targets and ground truth
collection in the SPARC method makes the deployment more cost effective and portable, thus creating the opportunity
to imbed spectral, spatial and radiometric targets at a study site providing references that improve a sensor's interactivity
as a phenomenological tool. A demonstration of the SPARC method is presented based on data collected with the
IKONOS satellite operated by GeoEye. A SPARC measurement of absolute calibration coefficients for the IKONOS
multispectral bands is compared to coefficients derived from the established reflectance-based vicarious calibration
method.
Reflectance-based vicarious calibration of satellite sensors is a method by which in-situ radiometric measurements of a surface target and the atmosphere are used to constrain a radiative transfer model for estimating a top-of-atmosphere (TOA) radiance. The procedure provides an at-sensor radiance, independent of the on-board calibrator, that can be used to maintain knowledge of the in-flight calibration performance of the remote sensing system. However, an estimate of the TOA radiance is incomplete unless accompanied with an uncertainty that quantifies the random and systematic errors associated with that estimate. Presented in this paper is a methodology for predicting a TOA radiance with an absolute accuracy estimate derived using an error propagation analysis based principally on validation data recorded by calibrated ground-based radiometer measurements. A vicarious calibration data collect for the airborne sensor ATLAS and the IKONOS satellite on June 30, 2000 at Brookings, South Dakota provides a test case for this technique in the solar reflective spectrum. The results show that using a natural grass covered target under moderate aerosol loading, absolute accuracies between 3% and 5% are achieved for band integrated TOA radiances between 0.4 and 1.6 microns.
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