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Exit of boundary layer plasma from the distant magnetotailIt is pointed out that the boundary layer plasma must somehow leave the magnetospheric system. It is proposed that the boundary layers on the dawn and dusk flanks are continued into the far magnetotail, becoming joined together far downstream, still on closed magnetic field lines. Within the combined layer there would be a dusk to dawn electric field for antisunward convection (as is the case for the boundary layers on the dawn and dusk flanks nearer to the earth). It is suggested that the boundary layer flow is so massive that the flow itself can generate the right electric field for continued flow. Most of the plasma in the mantle over the polar caps would also be convected out in a similar manner, rather feeding the plasma sheet. There would be a stagnation point inside the magnetotail, with any boundary or mantle plasma diffusing earthward of this point becoming the plasma sheet. It is deduced that no steady state solution is possible.
Document ID
19830043124
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Heikkila, W. J.
(Texas, University Richardson, TX, United States)
Date Acquired
August 11, 2013
Publication Date
March 1, 1983
Publication Information
Publication: Geophysical Research Letters
Volume: 10
Subject Category
Geophysics
Accession Number
83A24342
Funding Number(s)
CONTRACT_GRANT: NSF ATM-80-25194
CONTRACT_GRANT: NAGW-53
Distribution Limits
Public
Copyright
Other

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