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Experimentally-Derived Bidirectional Reflectance Distribution Function Data in Support of the Orbital Debris Program OfficeThe NASA Orbital Debris Program Office (ODPO) has used various optical assets to acquire photometric data of Earth-orbiting objects to define the orbital debris environment. To better characterize and model optical data acquired from ground-based telescopes, the Optical Measurements Center (OMC) at NASA Johnson Space Center emulates illumination conditions seen in space by using equipment and techniques that parallel telescopic observations and source-target-sensor orientations. One of the OMC goals is to improve the size calculation used for optical data by developing an optical-based Size Estimation Model. The current size estimation requires applying a Lambertian phase function, a set albedo value, and range to the observed magnitude. The first step to improving the sampled brightness of laboratory targets is to remove aspect-angle dependencies. Then, the volume of possible object viewing angles is sampled at 21 combinations of azimuth and zenith angles for each solar phase angle. Finally, the acquired images are input into an image processing program that generates approximations for the object’s Bidirectional Reflectance Distribution Function (BRDF) and phase function. The BRDF is a radiometric concept that identifies an object’s material composition by matching a BRDF approximated with photometric data collected by ground-based telescopes with a BRDF generated experimentally from a known object in the laboratory. This paper discusses the validation of experimental BRDF and phase function approximations produced in the OMC and how the findings will be incorporated into ODPO models. A Lambertian sphere is imaged and the subsequent experimental functions are scrutinized to confirm that they correspond to an object that has an isotropic luminance. With the image processing algorithm validated, test objects with varying optical properties are then imaged to confirm that the produced photometric functions are both unique and repeatable. Once the validation is complete, the OMC will be used to evaluate a subset of fragments from a hypervelocity impact test of a mock-up satellite and assess the appropriate phase function and size estimates using BRDF measurements for a large volume of targets composed of various shapes, sizes, and materials.
Document ID
20190030914
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
Hostetler, J.
(Jacobs Engineering Group Houston, TX, United States)
Cowardin, H.
(Jacobs Engineering Group Houston, TX, United States)
Date Acquired
September 20, 2019
Publication Date
September 17, 2019
Subject Category
Numerical Analysis
Report/Patent Number
JSC-E-DAA-TN71320
Meeting Information
Meeting: Advanced Maui Optical and Space (AMOS) Surveillance Technologies Conference
Location: Maui, HI
Country: United States
Start Date: September 17, 2019
End Date: September 20, 2019
Sponsors: Maui Economic Development Board, Inc.
Funding Number(s)
CONTRACT_GRANT: NNJ13HA01C
Distribution Limits
Public
Copyright
Public Use Permitted.
Technical Review
Single Expert
Keywords
Orbital Debris Program Office (ODPO)
Optical Measurements Center (OMC)
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