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The theory predicts a clear pattern in the density variations of the early universe, a feature measured by what is called the "spectral index".
These flux density variations could be due to changes in the circumstellar and interstellar medium in which the shocks travel.
Nevertheless, the individual states can still be clearly recognized in the density variations over the ribbons, and are in good agreement with the results from theory.
Such density variations were difficult to reconcile with the isotropy required by observations of the 3 K radiation.
This pattern is shown to be little sensitive to lower crust density variations.
Induced bone micro-structure (e.g. trabecular number, cortical thickness, porosity) and density variations can be quantified.
Existing analytical models ignore density variations either for the whole channel or across the channel gap.
Those advantages can enhance efficiency and are immune to drive current density variations.
High density variations in radial and axial directions, cause velocity gradients and increase fluid friction irreversibility.
Flux density variations, in the long (1981 to 2010), medium (2002 to 2010) and short (2009 to 2010) term are investigated.
In comparison to triangular and diamond tips, a bevel tip causes more needle bending and is more easily affected by tissue density variations.
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Justyna Jupowicz-Kozak
CEO of Professional Science Editing for Scientists @ prosciediting.com