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The Pioneer Venus Orbiter Plasma Wave Investigation
The Pioneer Venus plasma wave instrument has a selfcontained balanced electric dipole (effective length = 0.75 m) and a 4-channel spectrum analyzer (30-percent bandwidth filters with center frequencies at 100 Hz, 730 Hz, 5.4 kHz, and 30 kHz). The channels are continuously active and the highest Orbi...
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Published in: | IEEE transactions on geoscience and remote sensing 1980-01, Vol.GE-18 (1), p.36-38 |
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Main Authors: | , , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | The Pioneer Venus plasma wave instrument has a selfcontained balanced electric dipole (effective length = 0.75 m) and a 4-channel spectrum analyzer (30-percent bandwidth filters with center frequencies at 100 Hz, 730 Hz, 5.4 kHz, and 30 kHz). The channels are continuously active and the highest Orbiter telemetry rate (2048 bps) yields 4 spectral scans/s. 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. |
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ISSN: | 0196-2892 1558-0644 |
DOI: | 10.1109/TGRS.1980.350257 |