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...
Main Authors: | , , , , , , |
---|---|
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 |
id |
doaj-4a1614c525dc4a0b9c449206682f1ed4 |
---|---|
record_format |
Article |
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 |
work_keys_str_mv |
AT enochkrotichkipnoo meerkattimeandfrequencyreferenceopticalnetworkpreliminarydesignanalysis AT romeorggamatham meerkattimeandfrequencyreferenceopticalnetworkpreliminarydesignanalysis AT andrewwrleitch meerkattimeandfrequencyreferenceopticalnetworkpreliminarydesignanalysis AT timothybgibbon meerkattimeandfrequencyreferenceopticalnetworkpreliminarydesignanalysis AT siasmalan meerkattimeandfrequencyreferenceopticalnetworkpreliminarydesignanalysis AT hennokriel meerkattimeandfrequencyreferenceopticalnetworkpreliminarydesignanalysis AT francoiskapp meerkattimeandfrequencyreferenceopticalnetworkpreliminarydesignanalysis |
_version_ |
1725601382649561088 |