LEO Satellites and Frequency Synchronization

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  • Using the parameters provided by the project Telesat LEO, this thesis addresses the Doppler frequency shift encountered when an earth terminal station receives signals from a LEO satellite. To achieve fast frequency synchronization, there is a necessity to construct a Costas loop to speed up the acquisition time. Based on the theoretical foundations of the PLL, this thesis reviews the theory of BPSK and QPSK Costas loops. Then the thesis creates a new way of achieving fast synchronization for a BPSK Costas loop by adding a quadri-correlator. An optimized way is then introduced, which guarantees both stability and rapidity of acquisition. The construction of a QPSK Costas loop is different from that of BPSK. The thesis then shows that the addition of a quadri-correlator cannot be used in a QPSK Costas loop, but that the synchronization time can still be reduced by changing the parameters in the loop filter.

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  • Copyright © 2021 the author(s). Theses may be used for non-commercial research, educational, or related academic purposes only. Such uses include personal study, research, scholarship, and teaching. Theses may only be shared by linking to Carleton University Institutional Repository and no part may be used without proper attribution to the author. No part may be used for commercial purposes directly or indirectly via a for-profit platform; no adaptation or derivative works are permitted without consent from the copyright owner.

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  • 2021

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