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Optical subnet concepts for the deep space networkThis article describes potential enhancements to the Deep Space Network, based on a subnet of receiving stations that will utilize optical communications technology in the post-2010 era. Two optical subnet concepts are presented that provide full line-of-sight coverage of the ecliptic, 24 hours a day, with high weather availability. The technical characteristics of the optical station and the user terminal are presented, as well as the effects of cloud cover, transmittance through the atmosphere, and background noise during daytime or nighttime operation on the communications link. In addition, this article identifies candidate geographic sites for the two network concepts and includes a link design for a hypothetical Pluto mission in 2015.
Document ID
19940018796
Acquisition Source
Legacy CDMS
Document Type
Other
Authors
Shaik, K.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Wonica, D.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Wilhelm, M.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Date Acquired
September 6, 2013
Publication Date
November 15, 1993
Publication Information
Publication: The Telecommunications and Data Acquisition Report
Subject Category
Communications And Radar
Accession Number
94N23269
Funding Number(s)
PROJECT: RTOP 315-91-30-20-03
CONTRACT_GRANT: JPL-958733
CONTRACT_GRANT: JPL-958734
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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