Decaying columnar magnetic fields spontaneously isotropize and reproduce the expected helical and nonhelical MHD decay scalings, with the Hosking integral conserved for initially pointwise nonhelical fields.
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Inverse cascade from helical and nonhelical decaying columnar magnetic fields
Decaying columnar magnetic fields spontaneously isotropize and reproduce the expected helical and nonhelical MHD decay scalings, with the Hosking integral conserved for initially pointwise nonhelical fields.