A novel (SO(3)) analysis of anisotropies in Solar Wind turbulence (Ulysses) shows the absence of a complete recovery of isotropy in magnetic field fluctuations at the smallest scales and persistence of intermittent, anisotropic contributions. Quantities mixing isotropic and anisotropic fluctuations, such as longitudinal structure functions, may thus be affected by uncontrolled errors.
Bigazzi, A., Biferale, L., Gama, S., Velli, M. (2007). Anisotropy and universality in solar wind turbulence. Ulysses spacecraft data. In ADVANCES IN TURBULENCE XI (pp.682-684).
Anisotropy and universality in solar wind turbulence. Ulysses spacecraft data
BIFERALE, LUCA;
2007-01-01
Abstract
A novel (SO(3)) analysis of anisotropies in Solar Wind turbulence (Ulysses) shows the absence of a complete recovery of isotropy in magnetic field fluctuations at the smallest scales and persistence of intermittent, anisotropic contributions. Quantities mixing isotropic and anisotropic fluctuations, such as longitudinal structure functions, may thus be affected by uncontrolled errors.File in questo prodotto:
Non ci sono file associati a questo prodotto.
I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
