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Three-dimensional oscillatory magnetic reconnection View all abstracts by submitter

Jonathan Thurgood   Submitted: 2017-07-05 13:31

Here we detail the dynamic evolution of localised reconnection regions about three-dimensional (3D) magnetic null points by using numerical simulation. We demonstrate for the first time that reconnection triggered by the localised collapse of a 3D null point due to an external MHD wave involves a self-generated oscillation, whereby the current sheet and outflow jets undergo a reconnection reversal process during which back-pressure formation at the jet heads acts to prise open the collapsed field before overshooting the equilibrium into an opposite-polarity configuration. The discovery that reconnection at fully 3D nulls can proceed naturally in a time-dependent and periodic fashion is suggestive that oscillatory reconnection mechanisms may play a role in explaining periodicity in astrophysical phenomena associated with magnetic reconnection, such as the observed quasi-periodicity of solar and stellar flare emission. Furthermore, we find a consequence of oscillatory reconnection is the generation of a plethora of freely-propagating MHD waves which escape the vicinity of the reconnection region

Authors: J.O. Thurgood, D.I. Pontin, J.A. McLaughlin
Projects: None

Publication Status: Accepted for publication in ApJ.
Last Modified: 2017-07-06 10:45
Go to main E-Print page  Magnetic Flux Cancelation as the Origin of Solar Quiet Region Pre-Jet Minifilaments  Quasi-Periodic Radio Bursts Associated with Fast-mode Waves near a Magnetic Null Point  Edit Entry  Download Preprint  Delete Entry 

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