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Fiber Optic Reference Frequency Distribution to Remote Beam Waveguide AntennasIn 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.
Document ID
20210004259
Acquisition Source
Jet Propulsion Laboratory
Document Type
Other
External Source(s)
hdl:2014/33490
Authors
Law, J.
Kuhnle, P.
Calhoun, M.
Date Acquired
December 5, 1994
Publication Date
December 5, 1994
Publication Information
Publisher: UNKNOWN
Distribution Limits
Public
Copyright
Other
Technical Review
Keywords
deep
space
network
very
long-base
interferometry
low
phase
noise
radio
science
fiber
optics
beam
waveguide

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