Current sheets formed in magnetic reconnection events are found to be unstable to high-wavenumber perturbations. The instability is very fast: its maximum growth rate scales as , where is the length of the sheet, the Alfvén speed, and the Lundquist number. As a result, a chain of plasmoids (secondary islands) is formed, whose number scales as .
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Going to the next order in our outer solution results in an additional subdominant contribution to comparable to the second term in Eq. (15). Note that while the contribution of the second term in Eq. (13) to is negligible, the term itself cannot be dropped because it ensures that the solution has a finite value at . Note also that there exists an unstable solution that is entirely confined inside the current sheet, so that . For this solution, in Eq. (11) and to the lowest order in , is given just by the second term in Eq. (15). Solving Eq. (10) to the next order in , we find . The growth rate then is obtained from Eq. (18) in the limit . The result is , whence and . We will not consider this solution because it grows slower than the unconfined mode and its validity hinges on the numerical smallness of .