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11.
Eric G. Blackman George B. Field 《Monthly notices of the Royal Astronomical Society》2008,386(3):1481-1486
The magnetic Reynolds number, R M , is defined as the product of a characteristic scale and associated flow speed divided by the microphysical magnetic diffusivity. For laminar flows, R M also approximates the ratio of advective to dissipative terms in the total magnetic energy equation, but for turbulent flows this latter ratio depends on the energy spectra and approaches unity in a steady state. To generalize for flows of arbitrary spectra we define an effective magnetic dissipation number, R M,e , as the ratio of the advection to microphysical dissipation terms in the total magnetic energy equation, incorporating the full spectrum of scales, arbitrary magnetic Prandtl numbers, and distinct pairs of inner and outer scales for magnetic and kinetic spectra. As expected, for a substantial parameter range R M,e ∼ O (1) ≪ R M . We also distinguish R M,e from where the latter is an effective magnetic Reynolds number for the mean magnetic field equation when a turbulent diffusivity is explicitly imposed as a closure. That R M,e and approach unity even if R M ≫ 1 highlights that, just as in hydrodynamic turbulence, energy dissipation of large-scale structures in turbulent flows via a cascade can be much faster than the dissipation of large-scale structures in laminar flows. This illustrates that the rate of energy dissipation by magnetic reconnection is much faster in turbulent flows, and much less sensitive to microphysical reconnection rates compared to laminar flows. 相似文献
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Large-scale structures within a rough-wall boundary layer generated over a cube array have recently been linked to small-scale fluctuations close to the roughness through a dynamical mechanism similar to amplitude modulation. Demonstrating the existence of this mechanism for different roughness types is a crucial step towards the development of a generic model for wind fluctuations in the urban canopy. Here the influence of the upstream roughness geometry (two-dimensional (2D) and three-dimensional (3D)) and planform packing density (\( \lambda_{p} \)) and street-canyon aspect ratio on the non-linear interactions between large-scale momentum regions and the small scales induced by the presence of the roughness is studied within a wind tunnel using combined particle-image velocimetry and hot-wire anemometry. A multi-time delay linear stochastic estimation is used to decompose the flow into large scales that participate in modulation and the remaining small scales. Using three different upstream roughness configurations composed of either 3D cubes or 2D rectangular blocks it is shown that the upstream roughness configuration has an influence on the non-linear interactions in the rough-wall boundary layer. Analysis of the turbulence skewness decomposition shows a change in the location of the maximum of the term \( \overline{{u_{L}^{\prime} u_{S}^{\prime 2}}} \), which represents the influence of the large-scale momentum regions on the small scales, whilst the temporal correlation shows a modification of the interaction located closer to the roughness with a change from 3D to 2D roughness. Furthermore, a two-point spatio–temporal correlation demonstrates that the non-linear relationship is significantly modified in the wake-interference-flow regime compared to the skimming-flow regime. Through skewness decomposition and temporal correlations the canyon aspect ratio is shown to have no influence on the non-linear interactions, indicating that the mechanism depends only on the flow developing upstream. Finally, although the upstream roughness configuration is shown to influence the non-linear interactions, the nature of the mechanism remains the same in all configurations. 相似文献
15.
D. J. Ampleford S. V. Lebedev A. Ciardi S. N. Bland S. C. Bott G. N. Hall N. Naz C. A. Jennings M. Sherlock J. P. Chittenden A. Frank E. Blackman 《Astrophysics and Space Science》2007,307(1-3):51-56
Collimated flows ejected from young stars are believed to play a vital role in the star formation process by extracting angular
momentum from the accretion disk. We discuss the first experiments to simulate rotating radiatively cooled, hypersonic jets
in the laboratory. A modification of the conical wire array $z$-pinch is used to introduce angular momentum into convergent
flows of plasma, a jet-forming standing shock and into the jet itself. The rotation of the jet is evident in laser imaging
through the presence of discrete filaments which trace the rotational history of the jet. The presence of angular momentum
results in a hollow density profile in both the standing conical shock and the jet. 相似文献
16.
Eric G. Blackman 《Astrophysics and Space Science》2007,307(1-3):7-10
The absence of other viable momentum sources for collimated flows leads to the likelihood that magnetic fields play a fundamental
role in jet launch and/or collimation in astrophysical jets. To best understand the physics of jets, it is useful to distinguish
between the launch region where the jet is accelerated and the larger scales where the jet propagates as a collimated structure.
Observations presently resolve jet propagation, but not the launch region. Simulations typically probe the launch and propagation
regions separately, but not both together. Here, I IDentify some of the physics of jet launch vs. propagation and what laboratory
jet experiments to date have probed. Reproducing an astrophysical jet in the lab is unrealistic, so maximizing the benefit
of the experiments requires clarifying the astrophysical connection. 相似文献
17.
The fate and effects of the spill of Eleni V heavy fuel oil in May 1978 have been followed at two sites; one a heavily-polluted area subject to mechanical clean-up and one an undisturbed site where oil remains. At the first site the mechanized clean-up, and re-sorting of beach material by winter storms, has left the area visually clean of oil. However, near-shore and interstitial waters still contain high concentrations of Eleni V hydrocarbons 12 months after the spill. At the undisturbed site there has been very little change in the appearance and chemical composition of the oil during this period. 相似文献
18.
Under the Dumping at Sea Act 1974 the use of oil slick dispersants requres a licence from the Ministry of Agriculture, Fisheries and Food in England and Wales. These licences are issued or refused on the basis of tests to assess the toxicity of the dispersant when used at sea or on beaches. This paper describes the rationale behind the development of the two toxicity tests used, together with the test methods adopted and the results of the tests. 相似文献
19.
R.A.A. Blackman 《Marine pollution bulletin》1974,5(8):116-118
It may be necessary to immobilize an oil spill of more than 10,000 tons in European waters by sinking with sand. The possibility of damage to marine organisms from the sinking agents used has been investigated and it is concluded that toxic effects are unlikely to result. 相似文献
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