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Magnetic field studies at Jupiter by Voyager 2 - Preliminary resultsThe Voyager 2 magnetic field experiment, for which the instrumentation is identical to that on Voyager 1, operated flawlessly throughout the second Jupiter encounter. The paper presents a brief overview of the results obtained to date on the Jovian magnetosphere, the bow shock, the magnetopause, and the extended magnetic tail. The results and the magnetic field geometry confirm the earlier conclusion from Voyager 1 that Jupiter has an enormous magnetic tail, approximately 300-400 Jupiter radii in diameter, trailing behind the planet with respect to the supersonic flow of the solar wind. Additional observations of the distortion of the inner magnetosphere by a concentrated plasma show a spatial merging of the equatorial magnetodisk current with the current sheet in the magnetic tail. Disturbances near Ganymede are discussed.
Document ID
19800028676
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Ness, N. F.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Acuna, M. H.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Lepping, R. P.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Burlaga, L. F.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Behannon, K. W.
(NASA Goddard Space Flight Center Greenbelt, Md., United States)
Neubauer, F. M.
(Braunschweig, Technische Universitaet Braunschweig, Germany)
Date Acquired
August 10, 2013
Publication Date
November 23, 1979
Publication Information
Publication: Science
Volume: 206
Subject Category
Lunar And Planetary Exploration
Accession Number
80A12846
Distribution Limits
Public
Copyright
Other

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