4-8 July 2016
Kramer Law building
Africa/Johannesburg timezone
<a href="http://events.saip.org.za/internalPage.py?pageId=10&confId=86">The Proceedings of SAIP2016</a> published on 24 December 2017

Advantages of Free Space Optics over Optical Fibre for Clock Tone Distribution in a 2.5 GHz Transmission Link

6 Jul 2016, 16:10
1h 50m
Kramer Law building

Kramer Law building

UCT Middle Campus Cape Town
Board: F.243
Poster Presentation Track F - Applied Physics Poster Session (2)

Speaker

Mr Kagiso J Leburu (Nelson Mandela Metropolitan University)

Would you like to <br> submit a short paper <br> for the Conference <br> Proceedings (Yes / No)?

No

Level for award<br>&nbsp;(Hons, MSc, <br> &nbsp; PhD, N/A)?

MSc

Main supervisor (name and email)<br>and his / her institution

Prof Tim Gibbon, Tim.Gibbon@nmmu.ac.za, Nelson Mandela Metropolitan University

Please indicate whether<br>this abstract may be<br>published online<br>(Yes / No)

Yes

Apply to be<br> considered for a student <br> &nbsp; award (Yes / No)?

Yes

Abstract content <br> &nbsp; (Max 300 words)<br><a href="http://events.saip.org.za/getFile.py/access?resId=0&materialId=0&confId=34" target="_blank">Formatting &<br>Special chars</a>

The Square Kilometre Array is a big data project across Africa and Australia. When fully operational, SKA will host the world’s largest telescope with a combined signal collection surface area of about 1 km2, with distance up to 3000 km. The telescope rely on high clock tones to be distributed to each antenna and each clock signal is crucial for driving the digitizers, time stamping the data, and for monitoring and control functions. In addition to radio astronomy, other applications requiring high precision clock tones include banking systems, satellite navigation and metrology services. In the case of buried and aerial optical fibres, a complex interplay between numbers of factors adversely affect the stability in the light-wave clock tone as it propagates within an optical fibre. These factors include temperature fluctuations, component noise, polarisation instability, birefringence and others. Free Space Optics (FSO) presents some advantages over optical fibre – license free spectrum, quicker deployment and lower costs. However, the challenges experienced in FSO systems compared to optical fibre are atmospheric absorption and disturbances (fog, snow, rain), background light and requires line of sight. In this paper we present a detailed analysis of the advantages of FSO for clock distribution versus fibre transmission in the case of fluctuating temperature. The typical fibre has thermal coefficient of expansion of 7 ppm/°C. This means for 1 km length of fibre when the temperature changes by magnitude of 10 degree Celsius over a night/day cycle, the time of flight will change by 350 ps. This corresponds to a 19 degrees phase shift for a 2.5 GHz clock. The FSO system is far more immune to the temperature effects since the length of the medium remains unaffected.

Primary author

Mr Kagiso J Leburu (Nelson Mandela Metropolitan University)

Co-authors

Prof. Andrew Leitch (NMMU) Mr Duncan Boiyo (Nelson Mandela Metropolitan University) Mr George Isoe (Optical Fibre Research Unit,Nelson Mandela Metropolitan University) Dr Timothy Gibbon (NMMU Physics Department)

Presentation Materials

There are no materials yet.