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Plasma and magnetic field characteristics of magnetic flux transfer eventsPlasma and magnetic field data from ISEE 1 and 2 are examined for 5 passes of the magnetopause region at 20 and 40 deg northern latitudes, and are presented in terms of moments of the distribution function, calculated from two-dimensional or three-dimensional data. Flux transfer events are characterized by a mixture of magnetosheath and magnetospheric particles, which supports the hypothesis that flux transfer events represent encounters of reconnected flux tubes. An excess pressure appears to be balanced by the tension of the ambient magnetic field lines as they are draped around the reconnected flux tube, and the different observed magnetic field signatures are consistent with expectations for encounters of the flux tubes at different relative locations. It is suggested that increased flow speeds are caused by continued reconnection at the low-latitude boundaries of the flux tubes.
Document ID
19820047460
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Paschmann, G.
(Max-Planck-Inst. fuer Physik und Astrophysik Garching, Germany)
Haerendel, G.
(Max-Planck-Inst. fuer Physik und Astrophysik Garching, Germany)
Papamastorakis, I.
(Max-Planck-Inst. fuer Physik und Astrophysik Garching, Germany)
Sckopke, N.
(Max-Planck-Institut fuer Physik und Astrophysik Garching, Germany)
Bame, S. J.
(Max-Planck-Inst. fuer Physik und Astrophysik Garching, Germany)
Gosling, J. T.
(Los Alamos National Laboratory Los Alamos, NM, United States)
Russell, C. T.
(California, University Los Angeles, CA, United States)
Date Acquired
August 10, 2013
Publication Date
April 1, 1982
Subject Category
Geophysics
Accession Number
82A30995
Funding Number(s)
CONTRACT_GRANT: NAS5-20064
CONTRACT_GRANT: NASA ORDER S-50864-A
CONTRACT_GRANT: BMFT-01-01-0-27-ZA/WF/WRK-2754
Distribution Limits
Public
Copyright
Other

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