Adapting a Cryogenic Sapphire Oscillator for Very Long Baseline Interferometry

Details Adapting a Cryogenic Sapphire Oscillator for Very Long Baseline Interferometry Adapting a Cryogenic Sapphire Oscillator for Very Long Baseline Interferometry

2011-05-31

arxiv.org/abs/1106.0021v1

PASP, v. 123, p. 582, 2011

Astronomy and Astrophysics

Astrophysics

Instrumentation and Methods for Astrophysics

24 pages, 15 figures

Scientific paper

10.1086/660156

Extension of very long baseline interferometry (VLBI) to observing wavelengths shorter than 1.3mm provides exceptional angular resolution (~20 micro arcsec) and access to new spectral regimes for the study of astrophysical phenomena. To maintain phase coherence across a global VLBI array at these wavelengths requires that ultrastable frequency references be used for the heterodyne receivers at all participating telescopes. Hydrogen masers have traditionally been used as VLBI references, but atmospheric turbulence typically limits (sub) millimeter VLBI coherence times to ~1-30 s. Cryogenic Sapphire Oscillators (CSO) have better stability than Hydrogen masers on these time scale and are potential alternatives to masers as VLBI references. Here, We describe the design, implementation and tests of a system to produce a 10 MHz VLBI frequency standard from the microwave (11.2 GHz) output of a CSO. To improve long-term stability of the new reference, the CSO was locked to the timing signal from the Global Positioning System satellites and corrected for the oscillator aging. The long-term performance of the CSO was measured by comparison against a hydrogen maser in the same laboratory. The superb short-term performance, along with the improved long-term performance achieved by conditioning, makes the CSO a suitable reference for VLBI at wavelengths less than 1.3mm.

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