Intermittent Character of Fast Reconnection and its Role in Self-Regulation of a Marginally Collisionless Corona.

Physics

Scientific paper

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2723 Magnetic Reconnection (7526, 7835), 2772 Plasma Waves And Instabilities (2471), 2788 Magnetic Storms And Substorms (7954), 7526 Magnetic Reconnection (2723, 7835), 7845 Particle Acceleration

Scientific paper

I will review the current status of our understanding of magnetic reconnection, with a specific emphasis on the problem of onset of fast reconnection, i.e., on the transition between the slow resistive-MHD regime in collisional plasmas to the fast collisionless regime. I will formulate the condition for this transition and explain its critical role in various magnetically self-organized systems. As my main example, I will focus on solar coronal heating and will demonstrate how the highly intermittent nature of reconnection results in a dynamic self-regulation of this process to maintain the corona at about marginal collisionality.

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