Abstract

The US Strategic Command (USSTRATCOM) operated Space Surveillance Network (SSN) is tasked with Space Situational Awareness (SSA) for the U.S. military. This system is made up of Electro-Optic sensors, such as the Ground-based Electro-Optical Deep Space Surveillance (GEODSS) and RADAR based sensors, such as the Space Fence Gaps. They remain in the tracking of Resident Space Objects (RSO's) in Geosynchronous Orbits (GEO), due to limitations of SST and GEODSS system implementation. This research explores a reliable, ground-based technique used to quickly determine an RSO's altitude from a single or limited set of observations. Implementation of such sensors into the SSN would mitigate GEO SSA performance gaps. The research entails a method used to distinguish between the point spread function (PSF) observed by a star and the PSF observed from an RSO by using Multi-Hypothesis Testing with parallax as a test criterion. Parallax is the effect that an observed object will appear to shift when viewed from different positions. This effect is explored by generating PSFs from telescope observations of space objects at different baselines. The research has shown the PSF of an RSO can be distinguished from that of a star using single, simultaneous observations from reference and parallax sensing telescopes. This report validates these techniques with both simulations and experimental data from the SST and Naval Observatory sensors.

Highlights

  • The simulation showed that increasing the baseline difference between the reference and parallax sensing telescopes increases the performance of the Correlation Detection (CD) Multi-Hypothesis Test (MHT) algorithm when the luminosity of the target is closer to that of the background

  • The CD MHT algorithm could be used to determine the altitude of a given observation by using more hypothesized point spread function (PSF)’s or the speed of an observation by using successive frames and effects of horizontal or vertical tilt

  • With the altitude, speed, right ascension and declination, all orbital parameters of the satellite can be computed. These results show that implementation of the CD MHT algorithm proposed by the AF would be in line with AF leadership goals to network existing architecture for increased performance

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Summary

Objectives

Thesis Summary The purpose of this research is to demonstrate that a CD MHT detection algorithm can effectively categorize a detected target as either a stellar or NEO observation

Methods
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