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Magnetic field of Jupiter and its interaction with the solar windJupiter's magnetic field and its interaction with the magnetized solar wind were observed with the Pioneer 10 vector helium magnetometer. The magnetic dipole is directed opposite to that of the earth with an inclination of 15 deg lying in a system III meridian of 230 deg. The dipole is offset about 0.1 Jupiter radius north of the equatorial plane and about 0.2 Jupiter radius toward longitude 170 deg. There is severe stretching of the planetary field parallel to the equator throughout the outer magnetosphere, accompanied by a systematic departure from meridian planes. The field configuration implies substantial plasma effects inside the magnetosphere, such as thermal pressure, centrifugal forces, and differential rotation.
Document ID
19740035859
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Smith, E. J.
(California Institute of Technology, Jet Propulsion Laboratory, Pasadena Calif., United States)
Davis, L., Jr.
(California Institute of Technology Pasadena, Calif., United States)
Jones, D. E.
(Brigham Young University Provo, Utah, United States)
Colburn, D. S.
Dyal, P.
(NASA Ames Research Center Moffett Field, Calif., United States)
Coleman, P. J., Jr.
(California, University Los Angeles, Calif., United States)
Sonett, C. P.
(Arizona, University Tucson, Ariz., United States)
Date Acquired
August 7, 2013
Publication Date
January 25, 1974
Publication Information
Publication: Science
Volume: 183
Subject Category
Space Sciences
Accession Number
74A18609
Funding Number(s)
CONTRACT_GRANT: NAS7-100
Distribution Limits
Public
Copyright
Other

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