"Ideal" tearing and the transition to fast reconnection in the weakly collisional MHD and EMHD regimes. Issue 3 (25th March 2016)

• Record Type: Journal Article
• Authors: Del Sarto, Daniele; Pucci, Fulvia; Tenerani, Anna; Velli, Marco
• Is Part Of: Journal of geophysical research. Volume 121:Issue 3(2016:Mar.)
• Page Start: 1857
• Page End: 1873
• Publication Date: 2016-03-25
• Subjects: magnetic reconnection -- ideal tearing -- tearing mode -- plasmoid instability; Magnetospheric physics -- Periodicals; Space environment -- Periodicals; Cosmic physics -- Periodicals; Planets -- Atmospheres -- Periodicals; Heliosphere (Astrophysics) -- Periodicals; Geophysics -- Periodicals; 523.01
• DOI: 10.1002/2015JA021975
• Languages: English
• ISSNs: 2169-9380

Abstract

Abstract: This paper discusses the transition to fast growth of the tearing instability in thin current sheets in the collisionless limit where electron inertia drives the reconnection process. It has been previously suggested that in resistive MHD there is a natural maximum aspect ratio (ratio of sheet length and breadth to thickness) which may be reached for current sheets with a macroscopic length L, the limit being provided by the fact that the tearing mode growth time becomes of the same order as the Alfvén time calculated on the macroscopic scale. For current sheets with a smaller aspect ratio than critical the normalized growth rate tends to zero with increasing Lundquist number S, while for current sheets with an aspect ratio greater than critical the growth rate diverges with S . Here we carry out a similar analysis but with electron inertia as the term violating magnetic flux conservation: previously found scalings of critical current sheet aspect ratios with the Lundquist number are generalized to include the dependence on the ratio d e 2 / L 2, where d e is the electron skin depth, and it is shown that there are limiting scalings which, as in the resistive case, result in reconnecting modes growing on ideal time scales. Finite Larmor radius effects are then included, and the rescaling argument at the basis of "ideal" reconnection is proposed to explain secondary fast reconnection regimes naturally appearing in numerical simulations of current sheet evolution. Key Points: The critical scalings of the ideal tearing are generalized in the inertia‐driven regime FLR effects reduce the critical aspect ratio for the transition to the ideal tearing The ideal tearing model may explain a nonlinear reconnection rate increase of primary tearing modes