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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| Published in: | Advances in Astronomy and Space Physics |
|---|---|
| Date: | 2015 |
| Main Authors: | , , |
| Format: | Article |
| Language: | English |
| Published: |
Головна астрономічна обсерваторія НАН України
2015
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| Online Access: | https://nasplib.isofts.kiev.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. |