| 11. | The notion of isotropy, for properties independent of direction, is not a consequence of homogeneity.
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| 12. | Under normal conditions, the diffraction pattern has circular symmetry, expressing the isotropy of the liquid.
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| 13. | Cosmic isotropy and homogeneity are important as they are the basis of the modern standard model of cosmology.
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| 14. | The rest is some vague, hard-to-follow stuff on isotropy in computer graphics and cosmology.
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| 15. | The isotropy / anisotropy of a two-dimensional window function is shared by its two-dimensional Fourier transform.
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| 16. | Conversely, symmetric spaces with compact isotropy group are Riemannian symmetric spaces, although not necessarily in a unique way.
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| 17. | Thus, large scale isotropy is due to quantum fluctuations produced during cosmic inflation that are pushed outside the horizon.
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| 18. | The existence of an isotropy scale is determined by the length scale at which the Back-reaction parameter vanishes.
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| 19. | A series of one-way measurements were undertaken, all of them confirming the isotropy of the speed of light.
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| 20. | For the space of stable maps is an orbifold, whose points of isotropy can contribute noninteger values to the invariant.
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