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Quasi-two-dimensionality of three-dimensional, magnetically dominated, decaying turbulence · DOI 10.33232/001c.122855

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Magnetic Prandtl number dependence of plasmoid-mediated reconnection

physics.plasm-ph · 2026-05-18 · unverdicted · novelty 5.0

In the fully plasmoid-mediated regime the reconnection rate becomes nearly independent of the magnetic Prandtl number.

Small-scale Magnetic Fields in the Milky Way and Nearby Galaxies

astro-ph.GA · 2026-06-23 · unverdicted · novelty 1.0

Review chapter summarizing the importance of small-scale galactic magnetic fields and proposing SKA observation strategies.

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Magnetic Prandtl number dependence of plasmoid-mediated reconnection physics.plasm-ph · 2026-05-18 · unverdicted · none · ref 33
In the fully plasmoid-mediated regime the reconnection rate becomes nearly independent of the magnetic Prandtl number.
Small-scale Magnetic Fields in the Milky Way and Nearby Galaxies astro-ph.GA · 2026-06-23 · unverdicted · none · ref 26
Review chapter summarizing the importance of small-scale galactic magnetic fields and proposing SKA observation strategies.

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