MeerKAT time and frequency reference optical network: Preliminary design analysis

The MeerKAT telescope is a precursor to the Square Kilometre Array, which will rely on optical fibres to link the telescope receivers to a central processor point. The main aspects to consider for the fibre transport are astronomical data transmission as well as timing, monitoring and control. The a...

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Main Authors: Enoch K. Rotich Kipnoo, Romeo R.G. Gamatham, Andrew W.R. Leitch, Timothy B. Gibbon, Sias Malan, Henno Kriel, Francois Kapp
Format: Article
Language:English
Published: Academy of Science of South Africa 2017-05-01
Series:South African Journal of Science
Subjects:
Online Access:https://www.sajs.co.za/article/view/3830
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spelling doaj-4a1614c525dc4a0b9c449206682f1ed42020-11-24T23:12:20ZengAcademy of Science of South AfricaSouth African Journal of Science1996-74892017-05-011135/64410.17159/sajs.2017/201602383830MeerKAT time and frequency reference optical network: Preliminary design analysisEnoch K. Rotich Kipnoo0Romeo R.G. Gamatham1Andrew W.R. Leitch2Timothy B. Gibbon3Sias Malan4Henno Kriel5Francois Kapp61 Optical Fibre Research Unit, Department of Physics, Nelson Mandela University, Port Elizabeth, South Africa 2 Physical Science Department, University of Kabianga, Kericho, KenyaSquare Kilometre Array, MeerKAT Engineering Office, Cape Town, South AfricaFaculty of Science, Nelson Mandela University, Port Elizabeth, South AfricaOptical Fibre Research Unit, Department of Physics, Nelson Mandela University, Port Elizabeth, South AfricaSquare Kilometre Array, MeerKAT Engineering Office, Cape Town, South AfricaSquare Kilometre Array, MeerKAT Engineering Office, Cape Town, South AfricaSquare Kilometre Array, MeerKAT Engineering Office, Cape Town, South AfricaThe MeerKAT telescope is a precursor to the Square Kilometre Array, which will rely on optical fibres to link the telescope receivers to a central processor point. The main aspects to consider for the fibre transport are astronomical data transmission as well as timing, monitoring and control. The astronomical data streams from individual dishes to a central building, while the clock signal is distributed from a central point to remote dishes in the telescope array. The MeerKAT telescope, for instance, demands highly accurate and stable clock distribution over up to 12 km of optical fibre to remote dishes. The clock distribution is required for digitisation of astronomical signals. Phase stability is thus critical both for short-term and long-term requirements. In this work, we focused on the short-term stability. Phase noise measurements were performed on optical transmitters used to distribute the clock signals so as to ascertain their contribution to the overall clock jitter of the system. A maximum jitter requirement of 130 fs for a 1.712-GHz clock signal for MeerKAT time and reference is achieved using a distributed feedback laser. We found that with optimised modulation depth, additional passive optical components in the link do not significantly degrade the phase noise response. A distributed feedback laser was proven to be a suitable optical source that will meet the performance and link budget requirements for the MeerKAT telescope. Significance:  • A distributed feedback laser is recommended for the design of the MeerKAT time and reference system as it is a suitable optical source that will meet the performance and link budget requirements.https://www.sajs.co.za/article/view/3830telescopeoptical fibre networktiming signalsphase noiseprecursor
collection DOAJ
language English
format Article
sources DOAJ
author Enoch K. Rotich Kipnoo
Romeo R.G. Gamatham
Andrew W.R. Leitch
Timothy B. Gibbon
Sias Malan
Henno Kriel
Francois Kapp
spellingShingle Enoch K. Rotich Kipnoo
Romeo R.G. Gamatham
Andrew W.R. Leitch
Timothy B. Gibbon
Sias Malan
Henno Kriel
Francois Kapp
MeerKAT time and frequency reference optical network: Preliminary design analysis
South African Journal of Science
telescope
optical fibre network
timing signals
phase noise
precursor
author_facet Enoch K. Rotich Kipnoo
Romeo R.G. Gamatham
Andrew W.R. Leitch
Timothy B. Gibbon
Sias Malan
Henno Kriel
Francois Kapp
author_sort Enoch K. Rotich Kipnoo
title MeerKAT time and frequency reference optical network: Preliminary design analysis
title_short MeerKAT time and frequency reference optical network: Preliminary design analysis
title_full MeerKAT time and frequency reference optical network: Preliminary design analysis
title_fullStr MeerKAT time and frequency reference optical network: Preliminary design analysis
title_full_unstemmed MeerKAT time and frequency reference optical network: Preliminary design analysis
title_sort meerkat time and frequency reference optical network: preliminary design analysis
publisher Academy of Science of South Africa
series South African Journal of Science
issn 1996-7489
publishDate 2017-05-01
description The MeerKAT telescope is a precursor to the Square Kilometre Array, which will rely on optical fibres to link the telescope receivers to a central processor point. The main aspects to consider for the fibre transport are astronomical data transmission as well as timing, monitoring and control. The astronomical data streams from individual dishes to a central building, while the clock signal is distributed from a central point to remote dishes in the telescope array. The MeerKAT telescope, for instance, demands highly accurate and stable clock distribution over up to 12 km of optical fibre to remote dishes. The clock distribution is required for digitisation of astronomical signals. Phase stability is thus critical both for short-term and long-term requirements. In this work, we focused on the short-term stability. Phase noise measurements were performed on optical transmitters used to distribute the clock signals so as to ascertain their contribution to the overall clock jitter of the system. A maximum jitter requirement of 130 fs for a 1.712-GHz clock signal for MeerKAT time and reference is achieved using a distributed feedback laser. We found that with optimised modulation depth, additional passive optical components in the link do not significantly degrade the phase noise response. A distributed feedback laser was proven to be a suitable optical source that will meet the performance and link budget requirements for the MeerKAT telescope. Significance:  • A distributed feedback laser is recommended for the design of the MeerKAT time and reference system as it is a suitable optical source that will meet the performance and link budget requirements.
topic telescope
optical fibre network
timing signals
phase noise
precursor
url https://www.sajs.co.za/article/view/3830
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