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Two-way coherent Doppler error due to solar coronaTwo-way coherent Doppler errors resulting from phase scintillations induced on the uplink by the solar corona are considered. It is shown that this error can be estimated by taking statistics on the differential Doppler measurements. Typical estimates for the error are given for four Sun-Earth-probe angles and for integration times ranging from 1 second to 1 minute. These results are based on data collected during the 1985 Voyager 2 conjunction.
Document ID
19890010961
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Kinman, P. W. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Asmar, S. W. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Date Acquired
September 5, 2013
Publication Date
November 15, 1988
Publication Information
Publication: The Telecommunications and Data Acquisition Report
Subject Category
Communications And Radar
Accession Number
89N20332
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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