Another technique, time microscopy, also exists, and was used by the laboratory Physique des lasers, atomes et molécules (CNRS / Université de Lille) to study instabilities similar to those observed
in turbulent fluids.
Not exact matches
Nick Clegg is examine the «
fluid and unpredictable state» of the UK's
turbulent political scene
in...
Even the researchers who created this image had a tough time interpreting its complex representation how of
turbulent fluids flow
in three dimensions.
4 For example, the Navier - Stokes equations are used all the time to approximate
turbulent fluid flows around aircraft and
in the bloodstream, but the math behind them still isn't understood.
In fluid dynamics, a
turbulent flow is a swirling
fluid with faster or slower areas and higher or lower pressure.
Wouter Bos at the École Centrale de Lyon
in France and his colleagues have now tracked a
turbulent fluid's motion by picking one point and following it as the
fluid tosses it about.
More than 130 years ago, British physicist and engineer Osborne Reynolds described
fluid flowing at low speeds as «laminar,» meaning it flows smoothly
in a single direction, and
fluid flowing at high speeds as «
turbulent,» meaning it experiences chaotic changes
in pressure and energy.
The opposite of this is a
turbulent flow which is characterized by vortices and chaotic changes
in pressure and velocity within the
fluid.
In 1998, his previous fundamental work in turbulent combustion at the University of Colorado at Boulder led Dr. Mahalingam to do NSF - sponsored field research in Alaska comparing the properties of prescribed permafrost burns to help develop models describing the chemistry and fluid dynamics of fire
In 1998, his previous fundamental work
in turbulent combustion at the University of Colorado at Boulder led Dr. Mahalingam to do NSF - sponsored field research in Alaska comparing the properties of prescribed permafrost burns to help develop models describing the chemistry and fluid dynamics of fire
in turbulent combustion at the University of Colorado at Boulder led Dr. Mahalingam to do NSF - sponsored field research
in Alaska comparing the properties of prescribed permafrost burns to help develop models describing the chemistry and fluid dynamics of fire
in Alaska comparing the properties of prescribed permafrost burns to help develop models describing the chemistry and
fluid dynamics of fires.
The Southampton research team, led by Richard Sandberg, Professor of
Fluid Dynamics and Aeroacoustics, and including Dr Andrew Wheeler and Professor Neil Sandham, has identified that Direct Numerical Simulations (DNS), a model - free approach based on first principles (no assumptions or modelling are used) can help to develop an improved understanding of the role of
turbulent phenomena
in the flow - field and determine the validity of current turbulence modelling.
«People have seen these patterns
in turbulent flows for centuries, but we're finding ways to relate the patterns to mathematical equations describing
fluid flows,» Grigoriev said.
To the researchers» surprise, their calculations showed that
turbulent flows of a class of superfluids on a flat surface behave not like those of ordinary
fluids in 2 - D, but more like 3 - D
fluids, which morph from relatively uniform, large structures to smaller and smaller structures.
Using further 3 - D dynamo simulations, which model the generation of magnetic field by
turbulent fluid motions, Driscoll looked more carefully at the expected changes
in the magnetic field over this period.
In research featured on the cover of Journal of
Fluid Mechanics, an interdisciplinary Los Alamos team took a series of first - time measurements of
turbulent mixing, providing new insights for turbulence modelers.
The team directly measured terms
in turbulence model equations, providing insights into the global nature of the mixing (e.g., faster mixing near the edges of the
turbulent fluid layer when compared with the core) and identifying the dominant mechanisms governing the flow evolution.
The researchers took high - resolution mean and fluctuating velocity and density field measurements
in an RM flow, which was shocked and reshocked, to understand production and dissipation
in a two -
fluid, developing
turbulent flow field.
Violence issues center around dark, blood - like
fluids, bodies submersed
in water and
turbulent flashbacks.
That is to say, the transport of energy is (over some range of wavelengths) from shorter to longer wavelengths, the opposite of what is typically seen
in a
fluid, where energy is dissipated by the small - scale
turbulent structures.
Instead, it is a dynamically active, essentially
turbulent fluid,
in which large - scale tracer patterns arise from active turbulence and do not necessarily imply domination of the physics and climate system by large - scale flow fields....»
To improve the heat transfer between
fluid boundaries you can increase the
turbulent flow, which increases both the molecular contact rate and the rate of diffusion
in the
fluid.
The current thinking
in fluid dynamics, for which there is ample theoretical and computational evidence is that the Navier - Stokes equation if solved accurately are very accurate for a wide range of flows including
turbulent flows.
Now, Leif, the cause of the
turbulent field or natural convection is the suitable flow of energy from the solar core against gravity towards the surface, and the laws of
fluid dynamics under conditions
in which the convective cell has rotational and orbital components of angular momentum as determined by the path of the sun the planets force it to follow.
We demonstrate the energy with a very simple model
in which two
fluid elements of equal mass exchange positions, calling to mind a
turbulent field or natural convection.
Yet making progress is challenging,
in part because their dynamics involve three - dimensional,
turbulent fluid motions on the scale of a few meters, the nonlinear interaction of turbulence with the formation of cloud droplets, and the interaction of these cloud droplets with radiation (e.g. Wood (2012)-RRB-.