Yeates, A. R. (2017) 'Sparse reconstruction of electric fields from radial magnetic data.', Astrophysical journal., 836 (1). p. 131.
Accurate estimates of the horizontal electric field on the Sun's visible surface are important not only for estimating the Poynting flux of magnetic energy into the corona but also for driving time-dependent magnetohydrodynamic models of the corona. In this paper, a method is developed for estimating the horizontal electric field from a sequence of radial-component magnetic field maps. This problem of inverting Faraday's law has no unique solution. Unfortunately, the simplest solution (a divergence-free electric field) is not realistically localized in regions of non-zero magnetic field, as would be expected from Ohm's law. Our new method generates instead a localized solution, using a basis pursuit algorithm to find a sparse solution for the electric field. The method is shown to perform well on test cases where the input magnetic maps are flux balanced, in both Cartesian and spherical geometries. However, we show that if the input maps have a significant imbalance of flux - usually arising from data assimilation - then it is not possible to find a localized, realistic, electric field solution. This is the main obstacle to driving coronal models from time sequences of solar surface magnetic maps.
|Full text:||(AM) Accepted Manuscript|
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|Publisher Web site:||https://doi.org/10.3847/1538-4357/aa5c84|
|Publisher statement:||© 2017. The American Astronomical Society. All rights reserved.|
|Date accepted:||27 January 2017|
|Date deposited:||27 January 2017|
|Date of first online publication:||14 February 2017|
|Date first made open access:||No date available|
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