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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/3919

Title: Sweet–Parker current slab in a partially ionized plasma
Authors: Krishan, Vinod
Keywords: Magnetic fields
MDH plasmas
Issue Date: 29-Oct-2009
Publisher: Wiley Interscience for the RAS
Citation: Monthly Notices of the Royal Astronomical Society, 2009, Vol.400, p2200
Abstract: The formation of the Sweet–Parker current sheet, in fact a slab, is studied for a partially ionized plasma. The effects arising from the ion–neutral drag, the ambipolar diffusion, the resistivity resulting from electron–neutral and electron–ion collisions, and the Hall electric field are important for determining the dimensions of the current slab as well as the magnetic reconnection rate. It is the Hall effect that transforms the sheet into a slab. Along with the slab configuration, the out-of-plane plasma flow generated jointly by the Hall and the ambipolar effects is an important signature result. Although the ambipolar effect enhances and the Hall effect depletes the reconnection rate, its quantitative estimate may, at best, be considered only a pointer, owing to the lack of information on the precise physical conditions near the reconnection region in astrophysical settings.
Description: Restricted Access.
URI: http://hdl.handle.net/2289/3919
ISSN: 1365-2966 (Online)
0035-8711
Alternative Location: http://adsabs.harvard.edu/abs/2009MNRAS.400.2200K
http://dx.doi.org/10.1111/j.1365-2966.2009.15623.x
Copyright: 2009 Wiley Interscience for the RAS
Appears in Collections:Research Papers (A&A)

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