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Correlation of Doppler noise during solar conjunctions with fluctuations in solar activityDeviations betweeb observed Doppler noise and the noise model during solar conjunction were analyzed. It is tentatively concluded that these deviations are due to short-term fluctuations in solar activity as seen along the signal path, and not to solar/antenna structure effects or system noise temperature.
Document ID
19760008122
Acquisition Source
Legacy CDMS
Document Type
Other
Authors
Berman, A. L. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Rockwell, S. T. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Date Acquired
August 8, 2013
Publication Date
December 15, 1975
Publication Information
Publication: The Deep Space Network
Subject Category
Solar Physics
Accession Number
76N15210
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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