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The Pioneer Venus Orbiter plasma wave investigationThe Pioneer Venus plasma wave instrument has a self-contained balanced electric dipole (effective length = 0.75 m) and a 4-channel spectrum analyzer (30% bandwidth filters with center frequencies at 100 Hz, 730 Hz, and 30 kHz). The channels are continuously active and the highest Orbiter telemetry rate (2048 bits/sec) yields 4 spectral scans/sec. The total mass of 0.55 kg includes the electronics, the antenna, and the antenna deployment mechanism. This report contains a brief description of the instrument design and a discussion of the in-flight performance.
Document ID
19800046665
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Scarf, F. L.
(TRW Defense and Space Systems Group Redondo Beach, CA, United States)
Taylor, W. W. L.
(TRW Defense and Space Systems Group Redondo Beach, CA, United States)
Virobik, P. F.
(TRW Defense and Space Systems Group Redondo Beach, Calif., United States)
Date Acquired
August 10, 2013
Publication Date
January 1, 1980
Publication Information
Publication: IEEE Transactions on Geoscience and Remote Sensing
Volume: GE-18
Subject Category
Spacecraft Instrumentation
Accession Number
80A30835
Funding Number(s)
PROJECT: PROJECT PIONEER
CONTRACT_GRANT: NAS2-9842
CONTRACT_GRANT: NAS2-8809
Distribution Limits
Public
Copyright
Other

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