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Theoretical models of magnetic field line merging. I

Journal Article · · Rev. Geophys. Space Phys., v. 13, no. 1, pp. 303-336
Models of magnetic field line merging that consider processes in a limited region around the magnetic X line, within which the external magnetic fields are roughly uniform and antiparallel, are reviewed. Part I describes the concept of magnetic merging and then considers the models based on a hydromagnetic approach. The models developed by Sweet and Parker, by Petschek, and by Sonnerup and Yeh and Axford are shown to be fundamentally consistent, representing different aspects of the same problem. The model of Sweet and Parker describes the small region around the neutral line where magnetic field diffusion is the dominant process. The inclusion of inertial as well as finite resistivity effects allows an extension of their model to collisionless plasmas. Petschek's model represents a system with a boundary condition of uniform field at the sides; it has been extended and formulated in a mathematically precise manner. The nonsingular model of Sonnerup and of Yeh and Axford has special boundary conditions at the sides producing localized slow mode MHD expansion fans in the external flow; the singular models and the compressible similarity models are physically unrealizable. The maximum merging rate corresponds to flow into the diffusion region of the local Alfven speed, which, however, can be made arbitrarily large by slow mode MHD expansion if suitable boundary conditions are present. (auth)
Research Organization:
Massachusetts Inst. of Tech., Cambridge
Sponsoring Organization:
USDOE
NSA Number:
NSA-33-001709
OSTI ID:
4141021
Journal Information:
Rev. Geophys. Space Phys., v. 13, no. 1, pp. 303-336, Journal Name: Rev. Geophys. Space Phys., v. 13, no. 1, pp. 303-336; ISSN RGPSB
Country of Publication:
United States
Language:
English

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