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Analysis of the ICE combiner for multiple antenna arrayingThe passage of the International Cometary Explorer (ICE) through the tail of comet Giacobini-Zinner took place on September 11, 1985, at approximately 11:04 GMT. The signal-to-noise ratio of the data received from the ICE spacecraft during the comet encounter was improved by arraying the 64-m antenna channels A and B (RCP and LCP) with the two 34-m antennas. Specially designed combiners were built to combine the signals received by the three antennas at the different DSN sites to ensure that the spacecraft's weak signal was received. Although the ICE spacecraft was built with a 5-W transmitter and with a small antenna designed to provide data from no farther than 1 million miles, these combiners provided enough signal margin during the encounter to receive the ICE transmitted data from within the tail of comet Giacobini-Zinner, 44 million miles from earth.
Document ID
19880003322
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Foster, C.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Marina, M.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Date Acquired
September 5, 2013
Publication Date
November 15, 1987
Publication Information
Publication: The Telecommunications and Data Acquisition Report
Subject Category
Communications And Radar
Accession Number
88N12704
Funding Number(s)
PROJECT: RTOP 314-40-50-28-22
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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