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Nonlinear Interactions in Spherically Polarized Alfvénic Turbulence

Turbulent magnetic field fluctuations observed in the solar wind often maintain a constant-magnitude magnetic field accompanied by spherically polarized velocity fluctuations; these signatures are characteristic of large-amplitude Alfvén waves. Nonlinear energy transfer in Alfvénic turbulence is typ...

Täydet tiedot

Tallennettuna:
Päätekijät: Trevor A. Bowen, Corina I. Dunn, Alfred Mallet, Jonathan Squire, Samuel T. Badman, Stuart D. Bale, Thierry Dudok de Wit, Timothy S. Horbury, Kristopher G. Klein, Davin Larson, Lorenzo Matteini, Michael D. McManus, Nikos Sioulas
Aineistotyyppi: Artigo
Kieli:Inglês
Julkaistu: IOP Publishing 2025-01-01
Sarja:The Astrophysical Journal
Aiheet:
Alfvén waves
Space plasmas
Magnetohydrodynamics
Interplanetary turbulence
Interstellar plasma
Solar wind
Linkit:https://doi.org/10.3847/1538-4357/adc569
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