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The Jovian Magnetosphere And Magnetopause

Davis, Leverett, Jr. and Smith, E. J. (1976) The Jovian Magnetosphere And Magnetopause. In: Magnetospheric Particles and Fields. Astrophysics and Space Science Library. No.58. Springer , Dordrecht, pp. 301-310. ISBN 978-94-010-1505-9. https://resolver.caltech.edu/CaltechAUTHORS:20180830-095202831

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Abstract

It is convenient to divide the magnetosphere into three regions. The inner magnetosphere extends from the surface to about 25 R_J and is dominated by the basically dipolar field. The outer magnetosphere, on the sunward side, occupies a layer roughly 15 R_J thick just inside the magnetopause. Here the field direction was found by Pioneers 10 and 11 to have a strong southward component, 5 to 10 times as strong as expected if one scales the observations in the Earth’s magnetosphere. The middle magnetosphere is the remaining region. Its thickness, again on the sunward side, varies greatly as the magnetopause moves in and out. In this region the field direction turns as one goes outward from nearly dipolar to nearly radial but with a persistent southward component. The field is outward in the northern hemisphere, inward in the southern, separated by a thin (~1 or 2 R_J) warped current sheet in which the magnetic field appears to be very weak and mainly southward.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
https://doi.org/10.1007/978-94-010-1503-5_28DOIArticle
https://rdcu.be/b5PjtPublisherFree ReadCube access
Additional Information:© 1976 D. Reidel Publishing Company, Dorcht, Holland. We are greatly indebted to our coinvestigators on the Vector Helium Magnetometer Team, D.E. Jones, P.J. Coleman, Jr., D.S. Colburn, P. Dyal, and C.P. Sonett, as well as to the many others who worked on the project, for the efforts that yielded the data we have presented. We are indebted to colleagues in the scientific community for discussions and information that were invaluable in developing what understanding we have of Jupiter's magnetic field. We are indebted to NASA Grant NGR-05-002-160 (L.D.) and to NASA Contract NAS 7-100 (E.J.S.) for financial support that enabled us to carry out this research.
Funders:
Funding AgencyGrant Number
NASANGR-05-002-160
NASANAS 7-100
Subject Keywords:Solar Wind; Field Line; Current Sheet; Spherical Harmonic Expansion; Magnetometer Data
Series Name:Astrophysics and Space Science Library
Issue or Number:58
Record Number:CaltechAUTHORS:20180830-095202831
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20180830-095202831
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:89306
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:30 Aug 2018 17:05
Last Modified:24 Jul 2020 22:51

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