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An analysis of the turbulence in the central region of the Orion Nebula (M42) -- II. homogeneity and power-spectrum analyses

Anorve-Zeferino, G. A.
arXiv (All) · Papers
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astrophysics-of-galaxiescosmology-and-nongalactic-astrophysicsfluid-dynamics
In this second communication we continue our analysis of the turbulence in the Huygens Region of the Orion Nebula (M 42). We calculate the associated transverse structure functions up to order 8-th and find that the higher-order transverse structure functions are almost proportional to the second-or
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