INTERMITTENCY OF SOLAR WIND DENSITY FLUCTUATIONS FROM ION TO ELECTRON SCALES

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F14%3A10289642" target="_blank" >RIV/00216208:11320/14:10289642 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1088/2041-8205/789/1/L8" target="_blank" >http://dx.doi.org/10.1088/2041-8205/789/1/L8</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1088/2041-8205/789/1/L8" target="_blank" >10.1088/2041-8205/789/1/L8</a>

Result language
angličtina
Original language name
INTERMITTENCY OF SOLAR WIND DENSITY FLUCTUATIONS FROM ION TO ELECTRON SCALES
Original language description
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.
Czech name
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Czech description
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Type
J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)
CEP classification
BL - Plasma physics and discharge through gases
OECD FORD branch
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Project
<a href="/en/project/GAP209%2F12%2F1774" target="_blank" >GAP209/12/1774: Solar wind control of the processes at the magnetospheric boundaries</a><br>
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2014
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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