Caricamento...

Dissipation and heating in solar wind turbulence: from the macro to the micro and back again

The past decade has seen a flurry of research activity focused on discerning the physics of kinetic scale turbulence in high-speed astrophysical plasma flows. By ‘kinetic’ we mean spatial scales on the order of or, in particular, smaller than the ion inertial length or the ion gyro-radius—the spatia...

Descrizione completa

Salvato in:
Dettagli Bibliografici
Pubblicato in:Philos Trans A Math Phys Eng Sci
Autori principali: Kiyani, Khurom H., Osman, Kareem T., Chapman, Sandra C.
Natura: Artigo
Lingua:Inglês
Pubblicazione: The Royal Society Publishing 2015
Soggetti:
Accesso online:https://ncbi.nlm.nih.gov/pmc/articles/PMC4394685/
https://ncbi.nlm.nih.gov/pubmed/25848077
https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1098/rsta.2014.0155
Tags: Aggiungi Tag
Nessun Tag, puoi essere il primo ad aggiungerne! !