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Structure of Jupiter's magnetopause - Pioneer 10 and 11 observationsThe magnetic structure of Jupiter's magnetopause, as observed by the space probes Pioneer 10 and 11, is compared with terrestrial magnetopause structures from the OGO 5 mission. The Jovian magnetopause thickness, deduced from a rapid triple crossing, is found to lie in the range 3500-5200 km, while the adjoining plasma boundary layer was 5600-8400 km thick. Comparison with the terrestrial situation suggests that the dayside magnetopause thickness in both cases is a few times the ion gyroradius and that the dayside boundary layer is also of about the same width. The magnetopause normal vector and normal magnetic field component are determined for each crossing by use of minimum variance analysis. The results indicate a blunt and floppy magnetopause surface, for the most part with an insignificant normal magnetic field component. Only for three of the 14 crossings did this component exceed 1.5 times its error estimate. In two of these cases, the magnetic field tangential to the magnetopause displayed the characteristic features of a rotational discontinuity.
Document ID
19810050953
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Sonnerup, B. U. O.
(Dartmouth College Hanover, N.H., United States)
Smith, E. J.
(Dartmouth Coll. Hanover, NH, United States)
Tsurutani, B. T.
(California Institute of Technology, Jet Propulsion Laboratory, Pasadena Calif., United States)
Wolfe, J. H.
(NASA Ames Research Center Moffett Field, Calif., United States)
Date Acquired
August 11, 2013
Publication Date
May 1, 1981
Publication Information
Publication: Journal of Geophysical Research
Volume: 86
Subject Category
Lunar And Planetary Exploration
Accession Number
81A35357
Funding Number(s)
CONTRACT_GRANT: NSF ATM-79-20277
CONTRACT_GRANT: NAS7-100
CONTRACT_GRANT: NSG-7292
Distribution Limits
Public
Copyright
Other

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