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Radio frequency science considerationsUse of the 400 MHz telecommunications system to obtain scientific information, to provide backup information for the experiments flown, and to obtain measurements which aid in designing future probes is considered. Recommended objectives of such a program are summarized and include: measure 400 MHz amplitude to determine adsorption and perhaps scintillation (if data rate permits); measure noise strength near 400 MHz to reexamine 400 MHz choice and to observe thermal, cosmic, and local synchrotron noise trends; probe VSWR sensing to monitor integrity of system, icing, and possible plasma effects; after the probe is finished, have the bus radio occultation in the same region where the probe fell to evaluate the occultation.
Document ID
19750012326
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Croft, T. A.
(Stanford Univ. CA, United States)
Date Acquired
August 8, 2013
Publication Date
August 1, 1974
Publication Information
Publication: Dynatrend, Inc. Proc. of Outer Planet Probe Technol. Workshop, Sect. 1 through 11
Subject Category
Communications And Radar
Accession Number
75N20398
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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