Some of the Galileo spectra display a low-frequency turnover at frequencies ∼0.1 mHz that might be evidence of the density turbulence outer scale in the inner slow solar wind.
This expression is valid only if outer scales of turbulence are or the same order of magnitude as the dimensions of the radar volume (see, e.g., White et al. 1999).
The results show that the optimum beam size for FSO uplink depends upon Fried parameter and outer scale of the turbulence.
This collapsed the wedge shaped grooves in the outer initiator shell and created turbulence that rapidly mixed the plutonium and beryllium of the inner and outer spheres together.
The turbulence in the outer interface region is shown to be dominated by incompressible Alfvén waves both for cases of quasiparallel and quasiperpendicular shocks.
Estimates of the outer scale of solar wind turbulence at different heliocentric distances are found from a comparison of Doppler scintillations from near and distant spacecraft.
But the distance of the sun's surface from its center depends on several factors other than its gravitational field, he notes, including the sun's inner rotation; the convection and turbulence in its outer layers; and magnetic forces, particularly those around sunspots.
The corrugated outer surface acted as micro-turbulence promoters mitigating the temperature polarization effect and enhanced the external effective surface area for condensation.
The turbulences at the outer edges of the plasma are generated due to the interactions between incoming nitrogen gas flow and the outgoing plasma species.
This architecture manifested its suitability during repeated oxidation limiting the effect of oxygen attack to some microns thickness, due to diffused Mo which prevented turbulence and bursting phenomena on the outer glass.
