Understanding Large-scale Dynamos In Unstratified Rotating Shear Flows: Revision history

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28 November 2025

  • curprev 17:1517:15, 28 November 2025 VirgilioVandegri talk contribs 4,016 bytes +4,016 Created page with "<br>We mix simulations with new analyses that overcome earlier pitfalls to explicate how nonhelical imply-field dynamos grow and saturate in unstratified, magnetorotationally driven turbulence. Shear of the imply radial magnetic field amplifies the azimuthal part. Radial fields are regenerated by velocity fluctuations that induce shear of radial magnetic fluctuations, adopted by Lorentz and [https://www.xn--jj0bn3viuefqbv6k.com/bbs/board.php?bo_table=free&wr_id=7630861..."
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