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

Jump to navigation Jump to search

Diff selection: Mark the radio buttons of the revisions to compare and hit enter or the button at the bottom.
Legend: (cur) = difference with latest revision, (prev) = difference with preceding revision, m = minor edit.

13 October 2025

5 October 2025

  • curprev 20:5920:59, 5 October 2025MaryellenF87 talk contribs 7,096 bytes +7,096 Created page with "<br>We mix simulations with new analyses that overcome earlier pitfalls to explicate how nonhelical mean-area dynamos develop and saturate in unstratified, magnetorotationally driven turbulence. Shear of the imply radial magnetic area amplifies the azimuthal part. Radial fields are regenerated by velocity fluctuations that induce shear of radial magnetic fluctuations, adopted by Lorentz and Coriolis forces that source a unfavourable off-diagonal part within the turbulent..."