Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 399, Issue 1, Pages L146-L150Publisher
OXFORD UNIV PRESS
DOI: 10.1111/j.1745-3933.2009.00742.x
Keywords
instabilities; MHD; plasmas; turbulence
Categories
Funding
- EPSRC
- European Commission under EURATOM
- European Commission under UKAEA
- NSF [PHY-0821899]
- STFC
- Engineering and Physical Sciences Research Council [EP/G003955/1] Funding Source: researchfish
- EPSRC [EP/G003955/1] Funding Source: UKRI
- STFC [ST/F002505/2] Funding Source: UKRI
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Two-dimensional numerical simulations of the effect of background turbulence on two-dimensional resistive magnetic reconnection are presented. For sufficiently small values of the resistivity (eta) and moderate values of the turbulent power (is an element of), the reconnection rate is found to have a much weaker dependence on eta than the Sweet-Parker scaling of eta(1/2) and is even consistent with an eta independent value. For a given value of eta, the dependence of the reconnection rate on the turbulent power exhibits a critical threshold in is an element of above which the reconnection rate is significantly enhanced.
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