NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Dynamic magnetic reconnection at an X-type neutral pointThe relaxation of a two-dimensional 'X-type' neutral point magnetic field disturbed from equilibrium is considered. Perturbations are shown to possess well-defined azimuthal modes which allow an exact determination of the magnetic annihilation rate. Free magnetic energy is dissipated by oscillatory reconnection which couples resistive diffusion at the neutral point to global advection of the outer field. The decay of azimuthally symmetric (m = 0) modes - the only modes associated with topological reconnection - is limited by the dissipation time scale of the 'fundamental' (n = 0) mode with no radial nodes. This mode decays over typically 100 Alfven times. An analytic treatment shows that the oscillation and decay time scales couple according to a given law.
Document ID
19910048329
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Craig, I. J. D.
(Waikato, University Hamilton, New Zealand)
Mcclymont, A. N.
(Hawaii, University Honolulu, United States)
Date Acquired
August 14, 2013
Publication Date
April 10, 1991
Publication Information
Publication: Astrophysical Journal, Part 2 - Letters
Volume: 371
ISSN: 0004-637X
Subject Category
Solar Physics
Accession Number
91A32952
Funding Number(s)
CONTRACT_GRANT: NAGW-864
CONTRACT_GRANT: NSF ATM-88-22366
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.
No Preview Available