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

Internet

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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