Fibre-optic delivery of time and frequency to VLBI station

The quality of Very Long Baseline Interferometry (VLBI) radio observations predominantly relies on precise and ultra-stable time and frequency (T&F) standards, usually hydrogen masers (HM), maintained locally at each VLBI station. Here, we present an operational solution in which the VLBI observ...

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Veröffentlicht in:Astronomy and astrophysics (Berlin) 2017-07, Vol.603, p.A48
Hauptverfasser: Krehlik, P., Buczek, Ł., Kołodziej, J., Lipiński, M., Śliwczyński, Ł., Nawrocki, J., Nogaś, P., Marecki, A., Pazderski, E., Ablewski, P., Bober, M., Ciuryło, R., Cygan, A., Lisak, D., Masłowski, P., Morzyński, P., Zawada, M., Campbell, R. M., Pieczerak, J., Binczewski, A., Turza, K.
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Sprache:eng
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Zusammenfassung:The quality of Very Long Baseline Interferometry (VLBI) radio observations predominantly relies on precise and ultra-stable time and frequency (T&F) standards, usually hydrogen masers (HM), maintained locally at each VLBI station. Here, we present an operational solution in which the VLBI observations are routinely carried out without use of a local HM, but using remote synchronization via a stabilized, long-distance fibre-optic link. The T&F reference signals, traceable to international atomic timescale (TAI), are delivered to the VLBI station from a dedicated timekeeping laboratory. Moreover, we describe a proof-of-concept experiment where the VLBI station is synchronized to a remote strontium optical lattice clock during the observation.
ISSN:0004-6361
1432-0746
DOI:10.1051/0004-6361/201730615