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Fiber Optic Reference Frequency Distribution to Remote Beam Waveguide Antennas

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dc.contributor.author Calhoun, M. en_US
dc.contributor.author Kuhnle, P. en_US
dc.contributor.author Law, J. en_US
dc.date.accessioned 2004-10-05T06:14:55Z
dc.date.available 2004-10-05T06:14:55Z
dc.date.issued 1994-12-05 en_US
dc.identifier.citation Precise Time and Time Interval Planning en_US
dc.identifier.citation reston, Virginia, USA en_US
dc.identifier.clearanceno 94-1399 en_US
dc.identifier.uri http://hdl.handle.net/2014/33490
dc.description.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. en_US
dc.format.extent 22826 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other deep space network very long-base interferometry low phase noise radio science fiber optics beam waveguide en_US
dc.title Fiber Optic Reference Frequency Distribution to Remote Beam Waveguide Antennas en_US


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