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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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| Publicado no: | Geophys Res Lett |
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| Main Authors: | , , , , |
| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
BlackWell Publishing Ltd
2014
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| Assuntos: | |
| Acesso em linha: | https://ncbi.nlm.nih.gov/pmc/articles/PMC4459186/ https://ncbi.nlm.nih.gov/pubmed/26074642 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1002/2014GL062009 |
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