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NASA NTRS · 20210004259

Fiber Optic Reference Frequency Distribution to Remote Beam Waveguide Antennas

Law, J.·Kuhnle, P.·Calhoun, M.
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Abstract

In the NASA/JPL Deep Space Network (DSN), radio science experiments (probing outer planet atmospheres, rings, etc.) and very long-base interferometry (VLBI) require ultra-stable, low phase noise reference frequency signals at the user locations.

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deepspacenetworkverylong-baseinterferometrylowphasenoiseradiosciencefiberopticsbeamwaveguide

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Law, J., Kuhnle, P., Calhoun, M.. 1994-12-05. Fiber Optic Reference Frequency Distribution to Remote Beam Waveguide Antennas. https://ntrs.nasa.gov/citations/20210004259

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