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On the three-dimensional magnetic structure of the plasmoid created in the magnetotail at substorm onsetThe magnetic field in the plasmoid which is created by the reconnection of magnetic field lines at a neutral line formed in the near-earth region of the plasma sheet at substorm onset, and which flows out of the magnetotail into the magnetosphere's wake, displays a strong positive or negative Y(SM) component that has been difficult to reconcile with the standard, two-dimensional reconnection geometry. It is shown that this deviation of the magnetic field is a manifestation of the newly-reconnected field line loop's draping toward the tail's central or midnight meridian, and that the draping is a consequence of the three-dimensional plasma flow associated with the reconnection process.
Document ID
19820043480
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Hones, E. W., Jr.
(Los Alamos Scientific Lab. NM, United States)
Bame, S. J.
(Los Alamos National Laboratory Los Alamos, NM, United States)
Birn, J.
(Bochum, Ruhr-Universitaet Bochum, Germany)
Paschmann, G.
(Max-Planck-Institut fuer Physik und Astrophysik Garching, Germany)
Russell, C. T.
(California, University Los Angeles, CA, United States)
Date Acquired
August 10, 2013
Publication Date
March 1, 1982
Publication Information
Publication: Geophysical Research Letters
Volume: 9
Subject Category
Geophysics
Accession Number
82A27015
Funding Number(s)
CONTRACT_GRANT: W-7405-ENG-36
CONTRACT_GRANT: NAS5-25772
CONTRACT_GRANT: NASA ORDER S-50864
Distribution Limits
Public
Copyright
Other

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