Abstract
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 (η) and moderate values of the turbulent power (∈), the reconnection rate is found to have a much weaker dependence on η than the Sweet-Parker scaling of η1/2 and is even consistent with an η independent value. For a given value of η, the dependence of the reconnection rate on the turbulent power exhibits a critical threshold in ∈ above which the reconnection rate is significantly enhanced.
Original language | English (US) |
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Pages (from-to) | L146-L150 |
Journal | Monthly Notices of the Royal Astronomical Society: Letters |
Volume | 399 |
Issue number | 1 |
DOIs | |
State | Published - Oct 2009 |
Externally published | Yes |
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
- Space and Planetary Science
Keywords
- Instabilities
- MHD
- Plasmas
- Turbulence