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Ion-scale spectral break of solar wind turbulence at high and low beta

The power spectrum of magnetic fluctuations in the solar wind at 1 AU displays a break between two power laws in the range of spacecraft-frame frequencies 0.1 to 1 Hz. These frequencies correspond to spatial scales in the plasma frame near the proton gyroradius ρ(i) and proton inertial length d(i)....

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Detalles Bibliográficos
Autores principales:	Chen, C H K, Leung, L, Boldyrev, S, Maruca, B A, Bale, S D
Formato:	Online Artículo Texto
Lenguaje:	English
Publicado:	BlackWell Publishing Ltd 2014
Materias:	Research Letters
Acceso en línea:	https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4459186/ https://www.ncbi.nlm.nih.gov/pubmed/26074642 http://dx.doi.org/10.1002/2014GL062009

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