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arxiv: 1407.4048 · v2 · pith:JHDXOFOPnew · submitted 2014-07-15 · ⚛️ physics.flu-dyn · astro-ph.CO· astro-ph.GA

3D morphology of a random field from its 2D cross-section

classification ⚛️ physics.flu-dyn astro-ph.COastro-ph.GA
keywords distributionaspectcross-sectionellipsoidsprobabilityratiosfieldrandom
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We show that both aspect ratios of randomly oriented triaxial ellipsoids (representing isosurfaces of an isotropic 3D random field) can be determined from a single 2D cross-section of their sample using the probability distribution of the filamentarity F of the structures seen in the cross-section (F=0 for a circle and F=1 for a line). The probability distribution of F has a robust form with a sharp maximum and truncation that are sensitive to the ellipsoids' aspect ratios. We show that the aspect ratios of triaxial ellipsoids with randomly distributed dimensions can still be recovered from the probability distribution of F. This method is applicable to many shape recognition and classification problems, here illustrated with neutral hydrogen density in the turbulent interstellar medium of the Milky Way. The gas distribution is shown to be filamentary with the mean axis ratio 1:2:20.

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