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| Titel |
Anisotropy of intermittency inspace plasmas turbulence |
| VerfasserIn |
L. Sorriso-Valvo, E. Yordanova, S. Perri, V. Carbone, R. Bruno, M. André, P. Veltri |
| Konferenz |
EGU General Assembly 2009
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| Medientyp |
Artikel
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| Sprache |
Englisch
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| Digitales Dokument |
PDF |
| Erschienen |
In: GRA - Volume 11 (2009) |
| Datensatznummer |
250020199
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| Zusammenfassung |
| The presence of a background magnetic field induces anisotropy in hydromagnetic
turbulence. Understanding properties of anisotropy is important to
characterize turbulence power spectrum. This work presents a statistical study of anisotropy of intermittent properties, by using in three different regions of the heliosphere, namely in the solar wind, and in the Earth's foreshock and magnetosheath behind a quasi parallel bow shock. The whole two-points structure function tensor is studied to point out the anisotropic effects on intermittency intensity in the different datasets. The results are discussed. |
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