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Magnetic field experiment for Voyagers 1 and 2The magnetic field experiments of the Voyager program involve studies of the planetary fields of Jupiter, Saturn, possibly Uranus, and several satellites; the solar wind and satellite interactions with the planetary fields, as well as large- and micro-scale features of the interplanetary magnetic field will also be investigated. Dual low field and high field magnetometer systems with dynamic ranges of + or - 0.5 G and + or - 20 G respectively provide high reliability for the missions and permit the separation of the spacecraft and ambient fields. Quantization uncertainty, rms noise levels and data compaction schemes of the magnetometer systems are also mentioned.
Document ID
19780037734
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Behannon, K. W.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Acuna, M. H.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Burlaga, L. F.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Lepping, R. P.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Ness, N. F.
(NASA Goddard Space Flight Center Laboratory for Extraterrestrial Physics, Greenbelt, Md., United States)
Neubauer, F. M.
(Braunschweig, Technische Universitaet Braunschweig, Germany)
Date Acquired
August 9, 2013
Publication Date
December 1, 1977
Publication Information
Publication: Space Science Reviews
Volume: 21
Subject Category
Lunar And Planetary Exploration
Accession Number
78A21643
Distribution Limits
Public
Copyright
Other

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