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BIBTEX RIS

INTERMITTENCY OF SOLAR WIND DENSITY FLUCTUATIONS FROM ION TO ELECTRON SCALES

2014; IOP Publishing; Volume: 789; Issue: 1 Linguagem: Inglês

10.1088/2041-8205/789/1/l8

ISSN

2041-8213

Autores

C. H. K. Chen, L. Sorriso‐Valvo, Jana Šafránková, Zdeněk Němeček,

Tópico(s)

Ionosphere and magnetosphere dynamics

Resumo

The intermittency of density fluctuations in the solar wind at kinetic scales has been examined using high time resolution Faraday cup measurements from the Spektr-R spacecraft. It was found that the probability density functions (PDFs) of the fluctuations are highly non-Gaussian over this range, but do not show large changes in shape with scale. These properties are statistically similar to those of the magnetic fluctuations and are important to understanding the dynamics of small scale turbulence in the solar wind. Possible explanations for the behavior of the density and magnetic fluctuations are discussed.

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