meetings - Space Flight Mechanics Committee
meetings - Space Flight Mechanics Committee
meetings - Space Flight Mechanics Committee
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Feb 14, 2013 Kauai Salon 1<br />
SESSION 25: SPACE SITUATIONAL AWARENESS AND CONJUNCTION ANALYSIS -- II<br />
Chair: Dr. Ryan Russell, University of Texas at Austin<br />
8:00 AAS Application of a Laser Rangefinder for <strong>Space</strong> Object Imaging and Shape<br />
13-429 Reconstruction<br />
Michael Nayak, <strong>Space</strong> Development & Test Directorate, US Air Force; Bogdan<br />
Udrea, Embry-Riddle Aeronautical University<br />
This paper investigates the application of a laser rangefinder (LRF) for generation of a point<br />
cloud of a Resident <strong>Space</strong> Object (RSO), with sufficient resolution to provide comparable<br />
registration and shape reconstruction to an imaging LIDAR, for an SSA mission scenario.<br />
We examine a method that employs a combination of relative motion between the chaser<br />
and RSO & chaser attitude motion to perform 3D RSO imaging. These techniques are<br />
applied to reconstructing asteroid 1999-RQ36, of interest to NASA’s OSIRIS-REx mission,<br />
and RSOs shaped as generic geostationary telecommunications satellites, and validated with<br />
inclusion of stochastic & pulse-dilation error models.<br />
8:20 AAS Sensitivity Analysis of the Lightcurve Measurement Model for Use in Attitude<br />
13-430 and Shape Estimation of Resident <strong>Space</strong> Objects<br />
Laura Henderson, The University of Texas at Arlington; Kamesh Subbarao, The<br />
University of Texas at Arlignton<br />
This paper will focus on a recently used light curve measurement model that was based on<br />
developments in the computer graphics area and the information contained therein to<br />
evaluate the model's effectiveness in characterizing the attitude, angular velocty and shape<br />
parameters of an RSO. This evaluation will be performed using synthetic measurements<br />
generated for representative object attitude maneuvers. Numerical sensitivities (observation<br />
matrix) will be computed and a detailed study will be conducted to study the information<br />
present in this measurement.<br />
8:40 AAS Comparing the Reid Cost to the Mahalanobis Distance for Uncorrelated<br />
13-433 Track Association<br />
Cornelius Chow, Pacific Defense Solutions, LLC.; Keric Hill, Pacific Defense<br />
Solutions, LLC.; Joshua Horwood, Numerica Corporation; Chris Sabol, Air Force<br />
Maui Optical and Supercomputing<br />
A central problem faced by the space surveillance community is the problem of track-totrack<br />
association. Under Gaussian assumptions a track state can be characterized by its first<br />
two moments (mean and covariance). As such, the Mahalanobis distance is commonly used<br />
to parametrize the correlation of data sets. However, naive summations of information yield<br />
large association hypervolumes that increase the likelihood of false alarms. The Reid cost<br />
instead scales the product of the probability densities of both tracks by a third fused<br />
estimate. Simulations of 1000 space objects show tremendous improvement in resolving<br />
associations when using Reid’s function.<br />
23 rd AAS / AIAA <strong>Space</strong> <strong>Flight</strong> <strong>Mechanics</strong> Meeting Page 91