Magnetosheath and solar wind turbulence processes features identification

A different kind of analysis should be applied to a turbulent process, than that applied to a nondisturbed medium. In this work we present the result of extended self-similarity analysis (ESS) by comparing between different turbulent models: Kolmogorov K41 model, She-Leveque (isotropic log-Poisson m...

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Bibliographic Details
Date:2015
Main Authors: Prokhorenkov, A.S., Kozak, L.V., Lui, A.T.Y.
Format: Article
Language:English
Published: Головна астрономічна обсерваторія НАН України 2015
Series:Advances in Astronomy and Space Physics
Online Access:http://dspace.nbuv.gov.ua/handle/123456789/119934
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Journal Title:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Cite this:Magnetosheath and solar wind turbulence processes features identification / A.S. Prokhorenkov, L.V. Kozak, A.T.Y. Lui // Advances in Astronomy and Space Physics. — 2015. — Т. 5., вип. 2. — С. 93-98. — Бібліогр.: 14 назв. — англ.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine