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The Origin of the Slow-to-Alfvén Wave Cascade Power Ratio and its Implications for Particle Heating in Accretion Flows

Fuente: arXiv

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Dettagli Bibliografici
Autori principali:	Satapathy, Kaushik, Psaltis, Dimitrios, Özel, Feryal
Natura:	Preprint
Pubblicazione:	2024
Soggetti:	High Energy Astrophysical Phenomena Plasma Physics
Accesso online:	Acceder al recurso
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