Powered by OpenAIRE graph
Found an issue? Give us feedback
image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/ UNSWorksarrow_drop_down
image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/
UNSWorks
Doctoral thesis . 2022
License: CC BY
https://dx.doi.org/10.26190/un...
Doctoral thesis . 2022
License: CC BY
Data sources: Datacite
versions View all 1 versions
addClaim

Machine Learning for Inverse Problems in Space Domain Awareness

Authors: Abay, Rasit;

Machine Learning for Inverse Problems in Space Domain Awareness

Abstract

Space Domain Awareness (SDA) is concerned with space objects and their interactions in the space environment in temporal and spatial dimensions. The amount of SDA data to be processed is rapidly increasing as SDA sensors improve and resident space objects (RSO) proliferate. Recently, data-driven methods are being proposed for efficiently pro- cessing large amounts of data, reducing the complexity and workload associated with SDA activities, and to build and maintain space catalogues with more realistic space object characteristics and orbital elements. The primary objective of this research is to develop and validate a set of robust and gen- eralisable overarching machine learning models for two inverse problems in SDA, namely TLE estimation and light curve inversion for HAMR objects. This thesis is the first to investigate the feasibility of applying machine learning to predict TLEs from time-series osculating orbital elements. It is also the first to apply proba- bilistic deep generative neural networks to predict the physical characteristics of HAMR objects from light curves. A 6DoF space object simulator software suite for complex- shaped objects and Monte-Carlo based two line element (TLE) estimation programme were developed to achieve this. The key finding was that machine learning can be used to predict physical parameters such as TLEs and shapes, sizes, and attitude rates of complex- shaped HAMR objects. Secondly, the results showed that probabilistic deep generative neural networks are better than neural networks and gradient boosting trees when there are epistemic and aleatoric uncertainties in the data. The predictions of probabilistic deep neural network ensembles are physically more bounded. This has demonstrated that the proposed overarching machine learning models can reduce the complexity and workload associated with SDA activities, such as building and maintaining space catalogues with more realistic space object characteristics and orbital elements by efficiently processing large amounts of data.

Country
Australia
Related Organizations
Keywords

spaceflight, 4001 Aerospace engineering, bayesian neural networks, machine learning, light curves, artificial intelligence, anzsrc-for: 4001 Aerospace engineering

  • BIP!
    Impact byBIP!
    selected citations
    These citations are derived from selected sources.
    This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
    0
    popularity
    This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
    Average
    influence
    This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
    Average
    impulse
    This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
    Average
Powered by OpenAIRE graph
Found an issue? Give us feedback
selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
0
Average
Average
Average
Green