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.
Even the researchers who created this image had a tough time interpreting its complex representation how of
turbulent fluids flow in three dimensions.
Not exact matches
In
fluid dynamics, a
turbulent flow is a swirling
fluid with faster or slower areas and higher or lower pressure.
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.
Fluid flows can take one of two forms: well - ordered «laminar» or highly disordered «
turbulent» motion.
The opposite of this is a
turbulent flow which is characterized by vortices and chaotic changes in pressure and velocity within the
fluid.
For such
flow profiles the processes that sustain and create
turbulent eddies fail and the
fluid gradually returns to smooth laminar motion and it remained laminar until it reached the end of the pipe.
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.
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.
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....»
I am an engineer (naval architect actually) so systems with feedbacks from resonance to damping,
fluid flow,
turbulent flow etc etc are a daily norm.
It is like
fluid flows — they are not always
turbulent.
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.
The
fluid flows are 3 - dimensional and
turbulent.