Prior, C. and MacTaggart, D. (2019) 'Interpreting magnetic helicity flux in solar flux emergence.', Journal of plasma physics., 85 (2). p. 75850201.
Magnetic helicity flux gives information about the topology of a magnetic field passing through a boundary. In solar physics applications, this boundary is the photosphere and magnetic helicity flux has become an important quantity in analysing magnetic fields emerging into the solar atmosphere. In this work we investigate the evolution of magnetic helicity flux in magnetohydrodynamic (MHD) simulations of solar flux emergence. We consider emerging magnetic fields with different topologies and investigate how the magnetic helicity flux patterns correspond to the dynamics of emergence. To investigate how the helicity input is connected to the emergence process, we consider two forms of the helicity flux. The first is the standard form giving topological information weighted by magnetic flux. The second form represents the net winding and can be interpreted as the standard helicity flux less the magnetic flux. Both quantities provide important and distinct information about the structure of the emerging field and these quantities differ significantly for mixed sign helicity fields. A novel aspect of this study is that we account for the varying morphology of the photosphere due to the motion of the dense plasma lifted into the chromosphere. Our results will prove useful for the interpretation of magnetic helicity flux maps in solar observations.
|Full text:||(AM) Accepted Manuscript|
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|Publisher Web site:||https://doi.org/10.1017/S0022377819000229|
|Publisher statement:||This article has been published in a revised form in Journal of plasma physics https://doi.org/10.1017/S0022377819000229. This version is free to view and download for private research and study only. Not for re-distribution, re-sale or use in derivative works. © Cambridge University Press 2019.|
|Date accepted:||06 February 2019|
|Date deposited:||21 February 2019|
|Date of first online publication:||18 March 2019|
|Date first made open access:||19 September 2019|
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