Science topics: HydrodynamicsTurbulence
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Turbulence - Science topic

In fluid dynamics, turbulence or turbulent flow is a flow regime characterized by chaotic and stochastic property changes. This includes low momentum diffusion, high momentum convection, and rapid variation of pressure and velocity in space and time. Nobel Laureate Richard Feynman described turbulence as "the most important unsolved problem of classical physics."
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I am exploring leadership that navigates VUCA turbulence at the intersection of leadership development and organizational performance.
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Much appreciated
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Hi everyone,
I am working on a simulation involving restricted canal with ship using DFBI. I am facing reversed flow in my outlet boundaries as the DFBI is released (In 1.25s). Is there any method to avoid this type of wave reflection in outlet?
software using STARCCM+
VOF, implicit unsteady, K - epsilon turbulence
Thanks in advance
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Howdy Anagha R H
You may find it valuable to look up a similar question asked by Jasir Jawad on Feb.22, 2023 here on ResearchGate:
How to fix reverse flow on the pressure outlet in fluent?
There is also the question asked by Ali Rezaei on Jul 13, 2024:
Why does the static pressure at the outlet become a very negative value when the outlet flow boundary conditions are used?
The reflection is due to the change of impedance as a wave expands from a plane wave in the canal to a spherical wave in the open. (Physics class answer in 1959 - professor was pleased.). Brass musical instruments and woodwinds use this natural phenomenon to create resonance in the instrument.
A "solution" to the reverse flow is to restrict the outlet so a positive pressure reflection balances the rarefaction causing the reverse flow. See the replies to Jasir Jawad's question for his experience.
It may also work to prevent the wave due to the DFBI release by removing the same volume of canal fluid simultaneously, that is to exchange volumes so there is no excess to trigger a wave.
It is good news that your simulation is so good that it produced this condition!
Happy Trails,
Len.
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Hello all,
I've got a 2D simulation case in which the flow separates from the sharp leading edge of rectangular bluff body and reattaches to the wall some distance downstream. The main goal is a accurate prediction of pressure distribution along the body's face parallel to the flow.
I'm doing a transient simulation using SST model in conjunction with gamma-Re transition model. The time- cord-averaged y+ is less than 2~3 and the inflation layer around the face of interest contains 10 prism layers. The Re number based on the body's width (perpendicular to the flow) is 1.7e+4.
The problem is that my model overpredicts the reattachment length, which in turn leads to delayed pressure recovery.
I have a suspicion that longitudinal decay of turbulence values specified at the inlet might be to blame. Consulting the Ansys CFX-solver Modeling Guide, I learnt that one solution is to prescribe appropriate turbulence values at the inlet based on the desired values at the body. An alternative approach also suggests some additional source terms for k and w transport equations in order to preserve the inlet values up to some distance upstream the body, from where decay is allowed.
Here are my questions:
1- Is my suspicion valid in the case of my problem?
2- Is the decay of turbulence of physical basis or a numerical artifact?
3- which of the two methods works better? Are there any attempts in the literature?
I appreciate your comments.
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Hi Armin and All,
In my research on turbulence modeling for blood flow simulations in hemodialysis cannulae (Salazar et al., 2008, found in ResearchGate at: ), I explored the impact of turbulence modeling on predicting hemolysis (red blood cell damage). This work might be relevant to the query about turbulence values affecting reattachment length in bluff body simulations.
The paper highlights the importance of accurate turbulence modeling since blood flow in cannulae is often turbulent, and turbulence significantly impacts hemolysis. I discuss the selection of an appropriate turbulence model for accurate flow predictions.
We validated our approach using a benchmark case of a coaxial jet array, which shares similarities with cannula flow. The findings suggest that the Shear Stress Transport (SST) model with Gamma-Theta transition yielded the best results compared to standard k-ε and k-ω models.
Here's how this research might be helpful to your situation:
  • It emphasizes the critical role of turbulence modeling for accurate flow simulations, especially in complex geometries and turbulent regimes. This is likely applicable to bluff body simulations.
  • It underscores the need for validation, particularly when selecting a turbulence model. While the benchmark case involved a coaxial jet array, the validation process provides valuable insights for selecting appropriate turbulence models for specific geometries, including bluff bodies.
  • The SST model with Gamma-Theta transition might be a good candidate for your simulation. It could be worthwhile to explore how this model performs in your case compared to the model you're currently using.
While my paper focuses on hemolysis in cannulae, it offers valuable considerations for turbulence modeling in general. It highlights the importance of validation and suggests a potentially suitable turbulence model for your bluff body simulation.
I hope this information is helpful!
Best regards,
Luis
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Hi everyone,
I try to do a simulation about heat transfer of supercritical hydrogen in a cooling channel. Properties of H2 is obtained from NIST and displayed by an UDF function. I used the k-w model. If i set inlet temperature at 300K, everything is fine and correct. But when i set it to 34.6K, i ran into the problem " turbulent viscosity limited to viscosity ratio of 1.000000e+05 in xxx cells". My mesh is very fine as displayed below. CAn anyone help me to solve the problem
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Hi,
Did you manage to find a solution for your problem ? I kind have the same issue and I am not able to solve it.
Thanks
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The simulation is for turbulent and incompressible flow and the inlet velocity condition is selected for the inlet
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Howdy Ali Rezaei,
You may find it valuable to look up a similar question asked by Jasir Jawad on Feb.22, 2023 here on ResearchGate:
How to fix reverse flow on the pressure outlet in fluent?
I am simulating a cylinder filled with water vapor which has one outlet (no inlet). It is a pressure outlet. I am expecting to see flow through the boundary as a result of pressure difference between the body itself and the outlet boundary condition. However, as soon as I start simulation, reverse flow occurs and eventually leading to crash. My outlet boundary has lower pressure than the cylinder initial pressure. The simulation is transient and with compressible flow.
Several answers have been offered there, including a discussion of the natural phenomena.
Happy Trails,
Len
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Airflow
Turbulence
Air Dynamics
Signal effect
frequency response
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Analyzing a Loudspeaker Array with a Bessel Panel ...
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https://www.comsol.com › blogs › analyzing-a-loudspe...
Jul 23, 2018 — Use acoustics modeling to analyze a Bessel panel benchmark model and optimize the designs of loudspeaker arrays and other acoustics systems.
Modeling Speaker Drivers: Which Coupling Feature to Use
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https://www.comsol.com › blogs › modeling-speaker-dr...
Apr 26, 2022 — COMSOL Multiphysics® includes built-in coupling features that allow for detailed modeling and analysis of different types of speaker drivers ...
Missing: box ‎| Show results with: box
Dinaburg C2S Concentric Coplanar Stabilizer Analysis
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Oct 19, 2023 — Figure 5: The Simulation Speaker Box Model ... Model (LPM) for the 2.6L box model. ... This encourages us to use this simple COMSOL model as a ...
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I am running a coarse DNS case for pipe flow with 2.1 Million cells. My residuals are quite fluctuating as its a fully turbulent annular pipe flow case but its getting statistically converged to a mean value.
My doubt is, the residual values are quite high where its mean is getting converged for instant close to 0.1 or 0.01(refer attached .png), despite of giving tolerance of 1e-06. Due to this I think I have results of velocity profiles and shear stresses quite under predicted.
what can be the possible ways to reduce these residual values?? and what is the reason of having such high residuals??
NOTE: I am already using higher order schemes for solving Fluid flow equations in OpenFOAM
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I am interested in your question but it needs a lot more explanation. Let me explain what I'm wondering about that I'd need to know to think about your question: If you are solving a F(u)=b, the residual is
Residual = b-F(u_approximate).
This is a vector with a lot of components so plots are usually some sort of aggregate statistic.
So what is your system?? Sometimes, people solve F(u)=b by time stepping: (u_n+1 - u_n)/k + F(u_n)=b then the residual means the discrete time derivative. Sometimes codes are written to be very memory efficient so they calculate something they call a residual that is just some easy to get data that serves as an optimistic proxy.
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"How do we understand special relativity?"
The Quantum FFF Model differences: What are the main differences of Q-FFFTheory with the standard model? 1, A Fermion repelling- and producing electric dark matter black hole. 2, An electric dark matter black hole splitting Big Bang with a 12x distant symmetric instant entangled raspberry multiverse result, each with copy Lyman Alpha forests. 3, Fermions are real propeller shaped rigid convertible strings with dual spin and also instant multiverse entanglement ( Charge Parity symmetric) . 4, The vacuum is a dense tetrahedral shaped lattice with dual oscillating massless Higgs particles ( dark energy). 5, All particles have consciousness by their instant entanglement relation between 12 copy universes, however, humans have about 500 m.sec retardation to veto an act. ( Benjamin Libet) It was Abdus Salam who proposed that quarks and leptons should have a sub-quantum level structure, and that they are compound hardrock particles with a specific non-zero sized form. Jean Paul Vigier postulated that quarks and leptons are "pushed around" by an energetic sea of vacuum particles. 6 David Bohm suggested in contrast with The "Copenhagen interpretation", that reality is not created by the eye of the human observer, and second: elementary particles should be "guided by a pilot wave". John Bell argued that the motion of mass related to the surrounding vacuum reference frame, should originate real "Lorentz-transformations", and also real relativistic measurable contraction. Richard Feynman postulated the idea of an all pervading energetic quantum vacuum. He rejected it, because it should originate resistance for every mass in motion, relative to the reference frame of the quantum vacuum. However, I postulate the strange and counter intuitive possibility, that this resistance for mass in motion, can be compensated, if we combine the ideas of Vigier, Bell, Bohm and Salam, and a new dual universal Bohmian "pilot wave", which is interpreted as the EPR correlation (or Big Bang entanglement) between individual elementary anti-mirror particles, living in dual universes.
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Wolfgang Konle added a reply
5 days ago
Fred-Rick Schermer "It does not explain how all got started up, but then again I also have Energy as a given. I recognize your model as complete on its own, leaving some aspects unexplained."
Good question, an answer and some additional explanations can be given in short words.
There was no startup. The model is eternal.
The background of dark energy distorts space into an S³ structure with a space curvature of 1/R² and a volume of 2π²R³. The volume of space oscillates. It shrinks as the dark energy is charged and expands during a recycling event.
The transfer of the upload energy takes place via a gravitational interaction. With its gravitational field, each particle, including photons, creates a tiny dent in the dark energy density. If this dent moves, the dark energy has to bypass the dent. The bypass motion requires some energy, which must be provided by the moving gravitating object.
A recycling event lasts a few million years. The energy charging phase lasts about twenty to thirty billion years. We are currently in this phase.
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Fred-Rick Schermer added a reply
5 days ago
Wolfgang Konle
Thank you, Wolfgang, I understand better now what you are working with.
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Cosmin Visan added a reply
2 days ago
Fred-Rick Schermer Universe doesn't exist. "Universe" is just an idea in consciousness.
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Cosmin Visan added a reply
2 days ago
Wolfgang Konle Energy doesn't exist. "Energy" is just an idea in consciousness.
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Sergey Shevchenko added a reply
1 day ago
It looks as that rather strange series of posts in the thread is too long already, and to point here that the thread question rather in detail is scientifically answered in SS 5 posts series on page 1, and on page 2..
Cheers
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Fred-Rick Schermer added a reply
1 day ago
Wolfgang Konle
Wolfgang, will you please read this article in which I propose the inverse for explaining a Black Hole.
All data is the same, but the perspective is distinct.
It's like Rubin's Vase, where one can see a Vase, but another can see the Two Faces. All data is the same, but the view is distinct nevertheless.
Same for the Black Hole. I can see the Black Eye instead, with all data exactly the same, yet the perspective is what makes the view different.
There is truly no invisible mass required to explain everything we observe.
Preprint On The Scientific Black Eye
This may be my most important work. It puts me in opposition to the majority (nearly everyone) of the scientific community.
Thank you for your review.
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Cosmin Visan added a reply
24 hours ago
Fred-Rick Schermer Energy doesn't exist. "Energy" is just an idea in consciousness. See my paper "How Self-Reference Builds the World".
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Wolfgang Konle added a reply
12 hours ago
Fred-Rick Schermer
I have scanned your article about a "black eye".
But I could not identify the differences between your black eye model and the black hole model described in standard physics.
I have looked for differences in energy, mass, momentum, momentum of inertia, and external impact on the galaxy. But I could not find any substantial information about that kind of differences.
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Cosmin Visan added a reply
9 hours ago
Wolfgang Konle Energy doesn't exist. "Energy" is just an idea in consciousness. See my paper "How Self-Reference Builds the World".
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Fred-Rick Schermer added a reply
5 hours ago
Wolfgang Konle
Excellent, Wolfgang. You make me happy with that response, though I need to mention just a little more.
The Black Hole model contains an event horizon, whereas the Black Eye does not contain an event horizon.
There are two important positions which I describe as follows:
1. A Black Eye is a phenomenon like the Eye of the Storm is a phenomenon. The Eye of the Storm is really there, but it is not based on itself. The Eye is based on the wind force of the Storm. Inside the Eye, there is no wind force. Hence, it is a phenomenon, a byproduct of larger circumstances. It should be considered a major observation that physical realities can produce phenomena that then 'exist' in their larger context.
2. When a person closes an eye, then one can see what a Cyclops sees. Yet the eye that is open did not move toward the center of the face, so the reality of a Cyclops will not be achieved. That means that when an ordinary physical property among others is declared to be zero, then the remaining physical properties do not realign themselves around a center. There is no realigning. The physical reality remains intact, and the zero reality of a physical property cannot be used to declare how the standard reality is then something that it cannot be (i.e. singularities are outcomes on paper only; no scientific grounds were produced to declare singularities scientifically correct).
I do not undermine the Black Hole model other than proposing a better model in which there is no event horizon to consider. All is scientifically present in the Black Eye model. There is nothing to believe in the Black Eye model, while there is something to believe in the Black Hole model, and believing is of course a non-scientific activity.
Thank you, Wolfgang, for your reply.
Will you respond further based on what I wrote here above?
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On The Scientific Black Eye
A Black Hole is accepted in science by most physicists. Not many people suspect that an alternate model is available based on the same data, called a Black Eye.
The Black Eye model does not contain a mass in the center. The model is not based on a single mass. Rather, the outcome is explained based on the entire system, and for this article that system is a galaxy.
The Black Eye model takes a system-wide approach and bases the resulting outcome on all masses in a galaxy. The gravitational forces of all masses combined establish a collective gravitational depression in the center. In this model, we are witnessing a collective result.
Meanwhile, an additional component is involved as well, not considered by most physicists to play an important role. Next to the ordinarily considered motions of matter, a galaxy as a whole is also on the move through space in a single direction. This helps to establish a special outcome, right in the center.
Note that there is no difference in data between a Black Hole and a Black Eye. It is all in the scientific interpretation that the distinction between both models comes about. Like Rubin’s Vase, one can see a Vase, or one can see Two Faces. Either way, the data is identical.
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Most will be familiar with the Black Hole model, so the emphasis for this article will be on presenting the Black Eye model.
The starting point is not the gravitational monster itself, but rather the circumstances of a galaxy as a whole.
The Milky Way contains about 100 billion stars and all of these stars have their own gravitational force, attracting all other masses. Yet as a collective, the center of this gravitational force establishes a deep depression.
· The pull on the center is enormous, coming from all directions in the galactic disk. The explanation that not all masses move toward the center with that pulling force is due to the circular motion of this collective, countering the action. Most masses are pushed out by the circular motion and pulled in by the gravitational force.
A depression is made up of various components. The most important aspect for understanding the Black Eye model is that the center of the depression is void of materials, except for happenstance materials (more on this later).
The center exists in a gravitational balance, called net-zero, yet the depression is experienced at its gravitational maximum. That net-zero reality takes up space; it is not a singular point, but rather an area, an Eye of net-zero gravitational force.
Perhaps a surprise, but at the exact spot of first moving away from the net-zero location, all hell breaks loose.
· This sudden boundary shift is like the shift seen with the inner core of planet Earth, with the solid part of the inner core located in the center flanked right around it by the fluid part of the inner core. The center is solid, not moving internally, while the fluid part is moving wildly. There is no transition zone right at the shift of both parts of the inner core.
The same shift occurs between non-motion in center /wild motion right next to it in the gravitational depression. In the center, there is net-zero gravity, not experiencing gravity. Right on the edge of it the gravitational force is exerted to its max. There is no greater gravitational expression in the entire galaxy than right here next to the net-zero location.
What happens right next to this edgy spot is that friction has become available whereas no friction is available anywhere inside the net-zero center. As soon as that friction is available, there is motion, lots and lots of it. All tension of all masses in the entire galaxy is kept at net-zero in the center and breaks loose with a fury at first opportunity.
For the Black Eye model, one can declare that edgy spot a gravitational Wall of Motion. The photons seen in images of a Black Hole/Black Eye show us the Wall of Motion. As is well-known, we only see photons when they move in our direction. This is a location of great turbulence.
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In the Black Eye model, photons will in general not make it through the center because the gravitational Wall of Motion will swat them out of the way before a photon can reach the center. As such, the Eye will be black. Meanwhile, the Wall of Motion in which the photons are swatted into our direction ensures that the ring of light (the donut) is visible to us. Thanks to the way photons works, we can see the ring of light, the Wall of Motion.
· Further out, photons continue on their straight path all around the Black Eye and Wall of Motion. As long as they are not swatted by the Wall of Motion, and when photons are not aimed toward us, we do not get to see them.
Once more, the most important aspect is the center at net-zero. This net-zero location is the solid backbone of all gravitational masses moving around it. In a way, all masses are moving around the gravitational center. Each mass is attracted both by the center and by all other specific masses in the galaxy. As such, specific individual behavior by a mass can also get established in this setting.
A partial collective of masses in the galaxy, when placed in opposite location to the center, can move any single mass individually as well. That means that for a single mass, the majority of the galaxy can end up establishing the direction that pulls this mass toward the center. As a result, a single mass may end up with a specific behavior in light of the net-zero center.
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In a visualization with a clock, this is like a single mass located at 2 o’clock being attracted via gravity through the large center location of the clock by the other side. Yet it is not just the masses located at 8 o’clock that are doing the attracting. It is more like all masses between 5 and 11 o’clock are attracting the single mass at 2 o’clock. Masses found at 7 o’clock or 10 o’clock would also be pulling the single mass at 2 o’clock in their direction.
Similarly, the mass at 2 o’clock is contributing (its very small part) to the attraction on all these masses between 5 and 11 o’clock. It will do so as part of its majority of masses of a galaxy. A mass at 8 o’clock will be pulled by all masses situated between 11 o’clock and 5 o’clock, including the single mass at 2 o’clock.
This is therefore a story of the single mass being attracted by the many in opposite direction, while the single mass contributes itself, as part of the many in opposition, to each and every other mass in their specific opposite location.
Once more, it is the circular motion that keeps all masses where they are. The inward pull by all masses is countered by the outward motion of the circular motion of all masses.
Through happenstance, a single mass may no longer follow the established path and become attracted to the very center of all masses in the galaxy. Yet when that mass reaches the center, it will still move around it. The single mass reverts direction in a smooth but perhaps rather fast transition.
In a static view, the exact center has an attraction that is equidistant in all directions of the galaxy. As such, a single mass will bypass the center in a circular motion, reversing direction, exactly because there is no single mass of attraction. This is a collective outcome played out on an individual mass.
Interestingly, the net-zero location can be entered also by a mass, yet this cannot happen at great velocity. At great velocity, the mass will always move around the net-zero center.
Yet when a slowly and gradually moving mass enters the net-zero location, it can get stuck on the ‘wrong’ side of the Wall of Motion.
· Like an airplane flying straight into the Eye of the Storm perhaps not encountering much trouble, when flying out back into the Storm the plane better not enter it at the wrong angle where the force can overwhelm it. Indeed, it is dangerous work for these pilots.
Naturally, a mass that ‘fell’ into a Black Eye will not have a steering wheel available and will not be able to exit the Black Eye exactly as desired. In short, it will not exit in a single piece.
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That mass will get churned into pieces. Some of it will fly right back into the galactic disk, unnoticed, yet a good amount can move outwardly through the perpendicular spouts. These spouts are located on both sides of the net-zero location in the galactic disk, themselves also net-zero areas. What propels these churned pieces is nothing but the speed the pieces achieved from the churning motion in their direction. Once more, the Wall of Motion will not let any mass escape whole once it entered the net-zero location.
To understand how a galactic system can establish a Black Eye, it is not sufficient to understand the gravitational motions only. A galaxy, or any matter in the universe, is always on the move. There truly exists no matter at a standstill.
The entire galaxy of, for instance, the 100 billion stars of the Milky Way, are on the move collectively, moving through space in what is basically a straight line.
This is the fastest speed that all these Milky Way masses are moving in. The outer regions of the galaxy are moving at the same speed as all other masses in the galaxy in that single direction.
· Like ice-skaters on a frozen canal, each skating under his- or her own force, all are moving like a group and yet there is no group force. There appears to be a group, but a single skater can stop skating on his or her own accord, with the remainder of the group continuing. There is no group powering the skaters.
The initial ‘push’ established by the Big Bang materialization process got applied to all Milky Way energy, moving it in one and the same direction, at one and the same speed. Therefore, it appears that there is a group that is powered by group action. Yet the group action that we see, the circling of these masses, is based on gravity. For the skaters, we see the evidence of their being a group when they are jostling or helping propel each other. Yet in general, each skater skates on their own power.
· The original push of the Big Bang is not based on gravity.
The true motions of all masses in the Milky Way are more complex than considered in our Einsteinian view of matter in which gravity is the essential force.
On the one hand, there is the fastest motion of all masses moving in the same direction at the same speed at the same time. On the other hand, there is the gravitational motion indeed that attracts these masses to one another.
· A circular motion is the result of both realities combined.
In the center, there will be a net-zero location, and this will not be based just on gravity, but based on the established circular motion, which includes the single and fastest direction that all galactic matter is moving into.
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Why did physicists consider there is a Black Hole instead of a Black Eye?
The answer lies in our achieving answers not just based on what we observe in reality, but also in our doing calculations on paper. When all the data is transposed onto paper, then one facilitates an environment in which is it easy to make a simple but fatal mistake.
Consider a piece of paper with a face drawn on it: two ears, hair, a nose, an eye, a mouth and chin.
All parts are scientifically correct.
And yet when there is just a single eye in the face, then the drawing shows us a Cyclops. It does not matter that the eye itself is scientifically correct. The drawing shows an outcome that does not corroborate what we witness in nature.
When all data about a galaxy is expressed in correct calculations on paper, then a melding of data into a single mass can still make the outcome become incorrect. The worst part of the Black Hole calculations is accepting that for the Cyclops the single eye sits in the middle of a face.
Naturally, it is easy to see what a Cyclops sees. All one needs to do is close an eye and we see exactly what a Cyclops sees.
· Yet the mistake is to think that the remaining open eye moved to the center of our faces.
The model demands therefore that all that is real remains in place, even when there is an established outcome of zero for whichever aspect that one has considered essential in a physical environment. The zero presence of any aspect does not allow us to eliminate the zero location from our equations.
· We are not allowed to play with models at will.
It is easy to undermine the Black Hole model with the Black Eye model, just like it is easy to undermine the Vase with the Two Faces. Only one outcome will be correct, and yet the data shows us two possibilities.
How to pick the best possible outcome?
The scientific weak spot in the Black Hole model is that the entity that establishes the scientific Black Hole cannot be shown itself. The event horizon prevents any fully scientific acknowledgment to ever occur. The Black Hole model contains a curtain beyond which no scientific access can be obtained, except on paper. That makes it a weak scientific model because the scientific essence is not available.
The Black Eye model does not suffer this scientific problem. All data is out there in the open. Everything is explained.
The real distinction is in the interpretation of the data.
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Where is the Boundary between Special and General Relativity?
This question is not easy to answer.  In our modern time, a century after relativity was formulated, special relativity is usually understood to mean the study of motion in the absence of gravity (that is, in flat spacetime).  General relativity is usually understood to mean the study of true gravity (that is, curved spacetime).  In particular, the study of accelerated frames in the absence of gravity tends to be classed nowadays as special relativity.
But the distinction seems not always to have been this way.  Pais's biography of Einstein states that when Einstein first discussed acceleration in relativity, he wanted to generalise his special theory to non-inertial frames.  With this history in mind, it might be said that special relativity should be considered to relate only to inertial frames, and that general relativity contains everything else, from accelerated frames to gravity.
When Einstein started thinking about acceleration, he saw an immediate connection to gravity (the real gravity that makes tidal forces); this prompted him to postulate the equivalence principle.  Modern writers have followed suit, by tending to discuss acceleration only superficially, and then segueing quickly into a discussion of gravity proper.  The upshot is that in the eyes of some authors, discussions of accelerated frames have become inseparable from discussions of gravity.  And yet accelerated frames and gravity are quite distinct from each other.  The study of accelerated frames does not require any notion of gravity.
A problem of pedagogy then appears: the language gets confusing.  You can find any number of discussions of the Twin Paradox that say "To analyse the situation from the viewpoint of the accelerating twin, general relativity is needed".  It's not clear what that sentence really means.  If it means that a discussion of accelerated frames is needed, then it's true.  If it means that a discussion of true gravity (tidal forces) is needed, then it's false.  (We must distinguish the "pseudo gravity" that appears in an accelerating frame—the "g force" that we feel while being accelerated—from the real gravity that is produced by mass and energy.  Pseudo gravity has nothing to do with mass or tidal forces.)  So, the sentence "General relativity is needed to analyse the Twin Paradox" becomes ill defined, and is best avoided.  It's certainly true that most of those who say general relativity is needed in the Twin Paradox don't really know what that sentence means; they are just repeating something they heard elsewhere.  It's also true that some who use that phrase mistakenly think that an analysis of gravity is needed to resolve the Twin Paradox, even though they have never seen any such analysis.
Accelerated frames are routinely handled using the theory of inertial frames: see the FAQ "Can Special Relativity Handle Acceleration?".  It turns out that the true gravity (tidal forces) that arises from mass and energy invites us to consider spacetime as curved, unlike the case for inertial frames.  The result is that both inertial and accelerated frames are handled fully by flat spacetime, whereas true gravity requires curved spacetime.  So we now have a neat, well-defined separation of scenarios into flat and curved spacetime, and this is why the meanings of "special" and "general" relativity have evolved to refer to curvature rather than frames.  "Special relativity" is nowadays understood to refer to flat spacetime—which can certainly handle accelerated frames with their pseudo gravity.  Special relativity is then sufficient to explain the Twin Paradox.  (We just need to tell that to all those physics explainers on Youtube who are busy telling their audience that the explanation of the Twin Paradox requires general relativity.)  And "General relativity" is nowadays understood to refer to curved spacetime, meaning the study of true gravity that arises from mass and energy.
These modern meanings of "special" and "general" are apparently not what Einstein had in mind, since he couldn't predict any future difficulties in language and interpretation when he first spoke of generalising special relativity; he tended to discuss acceleration in the same breath as true gravity.  But from a modern viewpoint, we no longer set "special = inertial" and "general = non-inertial".  Instead, we set "special = flat spacetime" and "general = curved spacetime", in the hope that this will minimise any confusion of the role played by acceleration in gravity.  Unfortunately, that confusion is still very much present in the subject.  It is the reason that we should be very explicit about what we mean when discussing these topics.
References
  • A. Pais, "Subtle is the Lord...": The Science and the Life of Albert Einstein, Oxford University Press.
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I am trying to run a turbulent pipe flow simulation with turbulent Reynolds number of 600, for 15 seconds, the flow is pressure driven due to gravity enforced buoyancy force which gives kinematic viscosity input as 8.25E-0.5 N/m^2, if gravity value taken as 9.81.
But in this case the flow is unable to become turbulent for smagorinsky LES model. Is this because of the high viscosity input? because for same inputs and changing Re = 2400 and \nu = 2.06E-05 the flow starts to become turbulent within the span of 15 seconds.
1. to make my simulation run changing gravity value and keeping the nu = 2.06e-05 to obtain same Re = 600 will be a solution's to this?? (I'm trying to check this with trial runs)
2. Why does this happen? any physical intuitions for this kinda behavior with \nu values ??
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I suggest to use the dynamic Smagorinsky model. Furthermore, check also the correct domain extensions and grid sizes.
You can accelerate the numerical transient by affine a small perturbation to the initial condition.
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I found this article: that claims circular profiles are better for heat transfer than streamlined profiles as they induce more turbulences. Is this the case with other shapes as well? what is the best profile?
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I will suggest a Jukowsky airfoil having a 25% thickness ratio that (depending of flow Reynolds number ) could provide turbulent flow over 75% of its upper and lower surfaces but with a much lower drag than a circular shape.
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I am working on WMLES (wall Modelled LES) for which if I calculate my wall shear stress analytically and want to enforce it as a boundary condition at the wall patch, so that I do not need to resolve my near wall mesh rather give the wall shear stress as an input. One of the approach is defined by Schumann (1975) -(added an image below for the model formulation by Schumann) which I am trying to implement in OpenFOAM. My major question: Is there any method to define such a boundary condition of shear stress enforcement??
Because as far as the OpenFOAM user guide is concerned I could not find any such options. And the only way to define wall models is by changing the value of \nu_t.
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If you have a constant, uniform, fixed shear stress field, OpenFOAM does have a "fixedShearStress" boundary which takes as input the vector value of \tau (assuming its constant over the entire boundary).
If you have anything more complicated (like a non-uniform shear stress field), you will unfortunately have to get your hands dirty coding a custom boundary condition. The easiest way would be to make a copy and modify the existing fixedShearStress boundary in OF. It imposes a Dirichlet boundary based on the velocity normal gradient field (from tau) and the cell-centred values of the velocity field from cells neighbouring the boundary. If you do follow this approach, it is important to just make sure you cancel out any velocity in the boundary normal direction, to make sure you don't accidentally, while converging, introduce inlet or outlet flow across the boundary.
Regards
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Dear Readers,
I am writing to request assistance in obtaining numeric or number format data related to turbulent flow in ducts, specifically focusing on square, rectangular, and other geometries. I require data for cases of steady, fully developed flow in the cross section of the duct, with a particular interest in cross-sectional details.
The data I am seeking should be presented in a format that includes the following parameters:
- Horizontal coordinate (x2)
- Vertical coordinate (x3)
- Flow properties: main velocity (U), secondary velocities (V and W), turbulent kinetic energy (K), turbulent viscosity, turbulence dissipation rate (e), turbulent stresses (shear and normal), pressure distribution in the cross section, boundary shear stress, and flow parameters (longitudinal pressure gradients, duct geometry dimensions, friction factor, fluid density and viscosity, wall roughness conditions, etc.).
I have come across several articles that contain relevant information, but the data is presented in graphical form, making it challenging to extract the specific numeric values. Therefore, I kindly request your assistance in providing the data in numeric or number format, as described above.
Examples of experimental data sources include:
- Leutheusser, H.J. 1963. "Turbulent flow in rectangular ducts." J. Hydr. Div. ASCE 89 (3), 1–19.
- Brundrett, E., Baines, W. D. 1964. "The Production and Diffusion of Vorticity in Duct Flow." J. Fluid Mech., 19 (3), pp. 375-394.
- Gessner, F. B., Jones, J. B. 1965. "On Some Aspects of Fully-Developed Turbulent Flow in Rectangular Channels." J. Fluid Mech., 23 (4), pp. 689-713.
- Gessner, F. B. 1973. "The Origin of Secondary Flow in Turbulent Flow along a Corner." J. Fluid Mech., 58 (1), pp. 1-25.
- Melling, A., and Whitelaw, J.H. 1976. "Turbulent flow in a rectangular duct." J. Fluid Mech. 78, 289.
- Gessner and Emery. 1980. [Additional information needed]
- Leutheusser, H. J. 1984. "Velocity distribution and skin friction resistance in rectangular ducts." J. Wind Eng. Ind. Aero. 16, 315–327.
- Thangam, S., Speziale, C. G. 1987. "Non-Newtonian Secondary Flows in Ducts of Rectangular Cross-Section." Acta Mech., 68 (3-4), pp. 121-138.
- Rokni, M., et al. 1998. "Numerical and Experimental Investigation of Turbulent Flow in a Rectangular Duct." Int. J. Numer. Meth. Fluids, 28 (2), pp. 225-242.
Additionally, I am interested in numeric data, such as numerical predictions and Direct Numerical Simulation (DNS) data, from studies conducted by Naot and Rodi (1982) and Demuren and Rodi (1984):
- Naot, D.; Rodi, W. 1982. "Calculation of secondary currents in channel flow." ASCE J. Hydraul. Div. 108, 948–968.
- Demuren, A.O.; Rodi, W. 1984. "Calculation of turbulence driven secondary motion in noncircular ducts." J. Fluid Mech. 140, 189–222.
Furthermore, if any numeric data is available for other flow types, such as flow in cavities, flow at backward-facing steps, flow around cylinders, and flow around square rods, it would be greatly appreciated.
Thank you in advance for your assistance and contributions toward fulfilling this request. Your support will significantly contribute to the advancement of turbulent flow research.
Sincerely and best Regards,
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Dear Dr. Hafez,
This is a good theoretical work describing turbulent motion of fluid in pipes. In references of this article you can find experimental data. Best wishes, Oleh Shvydkyi.
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I am searching for an anemometer to measure turbulence intensity of a wind tunnel. Most of the hot wire aneomemeters on market are designed for HVAC applications so their accuracy is around 5%. Since moderate turbulence intensity is defined to be between 1% and 5%, using a anemometer with 5% accuracy does not sounds like appropriate. What should be the accuray of the device for this measurement?
Additional Question: What should be the sampling rate of the device?
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Hi Harun,
In a wind tunnel, Hot-Wire Anemometry (HWA) should do the job. Although you will have to calibrate the probes. Normally they can have an acquisition frequency of about 30kHz, which should be more than enough.
Other methods are Laser Doppler Anemometry (LDA) and Particle Image Velocimetry (PIV). For these techniques you will need a particle generator as the velocity of such particles will be used as a proxy of the flow velocity. Normally in wind tunnels a smoke generator is used to generate particles.
Laser Doppler Anemometry is, like HWA, a point wise technique. That means that you measure point-to-point. However, it's probably the most precise technique to measure instantaneous fluid velocities.
Particle Image Velocimetry can also be used, but in this case the requirements are higher: fast camera synchronized with a laser to light a section of the wind tunnel, etc.
Acquistion frequency will depend on the time scales of your phenomenon. Always consider the Nyquist-Shannon criterion (acquisition frequency should be at least the double of the signal's maximum frequency) when performing measurements, so you will be sure you'll capture all the important features.
Let me suggest you an event that may be of your interest: the W.A.T.E.R. Summer School, an event dedicated to experimental techniques in fluid mechanics: https://water.sciencesconf.org/
And some bibliographic references that can be useful for you:
The Handbook of Experimental Fluid Mechanics:
The experimental hydraulics methods.
Feel free to send me a message with more questions.
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I have a transparent pipe which takes water from a tank.
The flow happens thru a pump. Pump takes water from tank and makes it flow thru the pipe.
The water stored in tank is open to atmosphere.
When I see the flow through the transparent pipe, i observe very huge bubbles. I have attached an image for your review.
I am interested to learn: from where is this air coming in the flow?
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As James Garry suggested, a dissolved air cannot cause a sustainable train of bubbles as suggested in the photo. The bubbles seem to be consistent in your experiment and most probably there is a consistent (although small) source of air that is introduced in the flow. Try what James has suggested and close every possible leak.
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This is a code block from nutWallFunction library in OpenFOAM where in, effective kinematic viscosity ($\nut_w$) at the wall is calculated using resolved field(in case of LES)/ mean field(in case of RANS) and $y^+_p$ (wall normal distance of the first cell center). this allows to set a new viscosity value as boundary condition at the wall using log law. Considering the first cell center is in the logarithmic layer of the universal velocity profile.
Now, in this code block of member function defined as nutUWallFunctionFvPatchScalarField::calcYPlus()
There has been iterations done for the yPlus value to reach convergence with maximum of 10 iterations. Why are these iterations needed? and why is the maximum number of iterations 10. I have given a reference of the code below;
tmp<scalarField> nutUWallFunctionFvPatchScalarField::calcYPlus
(
const scalarField& magUp
) const
{
const label patchi = patch().index();
const turbulenceModel& turbModel = db().lookupObject<turbulenceModel>
(
IOobject::groupName
(
turbulenceModel::propertiesName,
internalField().group()
)
);
const scalarField& y = turbModel.y()[patchi];
const tmp<scalarField> tnuw = turbModel.nu(patchi);
const scalarField& nuw = tnuw();
tmp<scalarField> tyPlus(new scalarField(patch().size(), 0.0));
scalarField& yPlus = tyPlus.ref();
forAll(yPlus, facei)
{
scalar kappaRe = kappa_*magUp[facei]*y[facei]/nuw[facei];
scalar yp = yPlusLam_;
scalar ryPlusLam = 1.0/yp;
int iter = 0;
scalar yPlusLast = 0.0;
do
{
yPlusLast = yp;
yp = (kappaRe + yp)/(1.0 + log(E_*yp));
} while (mag(ryPlusLam*(yp - yPlusLast)) > 0.01 && ++iter < 10 );
yPlus[facei] = max(0.0, yp);
}
return tyPlus;
}
My doubt is concerning the do-while loop at the end for yPlus iteration.
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CFD softwares are based on numerical methods or techniques to predict the fluid behavior for various conditions e.g. LES and RANS turbulence modelling etc. Unlike exact solutions , the numerical methods involve approximations of the governing fluid parameters which cannot be evaluated at once and thus need iterative computational solvers.
During this process several types of errors are introduced while approximating variable property e.g round off errors ( machine precision) , truncation errors depending on the type of numerical scheme used.
However , according to the nature of fluid and it's interaction with surrounding environment , ( in your e.g yplus wall function which is measure of the fluid friction resistance near wall ) the solutions obtained through numerical schemes present a significant source of error which can interpret the fluid behavior in entirely different manner.
Therefore, the solution is often tested by repeating the process using better approximations and schemes with a focus to obtain the exactness of parameter value leading to iterations.
During iteration process , the error can amplify or reduce ( which is indicative of the stability of solution ) depending on boundary conditions used to obtain solution. So, often an error tolerance is introduced as condition in numerical algorithm to make the solution more meaningful and realistic which closely approximates the fluid behavior. In your case wall shear stress is being approximated using wall units in logarithmic boundary layer.
Once that condition is satisfied, the process stops and proceeds further by evaluating the next dependent variable and so on until complete solution is obtained.
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Usually the distance between inlet boundary and body about 5 size of body. For what purpose? Why cannot located body very close to boundary?
I simulate the flow around bridge section, VIV and Karen vortex street. Try to understand the influence on inlet Turbulence Intensity. I choose 0.01% and 10%, ratio 10 and result was the same.
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Anastasia Klimova The closer the object is to the inlet, the more important the turbulence boundary conditions at the inlet are, as I mentioned earlier. An analogous case is the flow around an obstacle in a pipe. If we set a parabolic profile at the inlet, the hydraulic run-up can be much shorter than when a piston flow is set at the inlet. Depending on the flow, often characterized by the Reynolds number, there is a minimum distance required for the velocity profile to be established, etc. Hydraulic run-up limitation shortens the calculations because a smaller computational domain means fewer computational cells, but it forces the engineer to pay more attention to the selection of appropriate boundary conditions.
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I have a fully developed pipe flow in with Inner radius (r) and outer radius (R), using pressure driven flow condition due to buoyancy,
- (1/rho) dP/dx = g
and velocity scaling u* = sqrt ( (-R/ (2 rho)) * (dP/dx)) [ friction velocity ], if Reynolds number is fixed ( Re = 600 ), along with r and R
we can get y+ value based on y values we give for cell size at both the walls,
But the question is when y+ calculated from this formula is y+ at the outer wall ( general pipe flow condition ) but how to get a y= for the inner annulus? ( concentric annular pipe flow ) ?
is there any analytical method to find this y+ or the only solution is to get us after simulation run when we have calculated friction velocities wall shear stresses at wall cell centers.
basically two different y+ to get analytically, in order to set up minimum cell size for my LES grid.
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if you work by prescribing the Re_tau number of your non dimensional solution, you have the y+ at the first cell known.
Since y+ = u_tau*y/ni = Re_tau *y/L you just scale your non dimensional first cell height by Re_tau.
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Art x Mental Health
Dear fellow researchers,
Art has always been a way of expression for me. It has calmed my inner turbulence and helped me to make better decisions. Let's talk about how picking up a paintbrush, dancing to your favorite song, or simply doodling can make a real difference in how we feel.
Consider the various ways in which art serves as a medium for emotional expression and processing. Reflect on the role of symbolism, metaphor, and abstraction in conveying deeply felt emotions. Share anecdotes, research findings, or theoretical perspectives that shed light on the therapeutic potential of art in this regard.
Your unique insights and experiences are invaluable contributions to this conversation.
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Art provides a unique avenue for individuals to express and process emotions that may be challenging to articulate verbally. Here are several ways in which art enables this:
1. Non-Verbal Expression: Art allows individuals to communicate emotions without relying on words. Through visual elements such as color, form, and composition, as well as through the use of symbols and metaphors, artists can convey complex emotional experiences that may be difficult to put into words.
2. Freedom of Expression: Art offers a space for uninhibited expression. Unlike verbal communication, which may be constrained by social norms or self-censorship, art allows individuals to explore and express their emotions freely, without fear of judgment or misunderstanding.
3. Symbolic Representation: Art enables the use of symbolism and metaphor to represent emotions indirectly. By employing symbols or visual metaphors, artists can convey abstract or ambiguous feelings in a way that resonates with viewers on a deeper, subconscious level.
4. Catharsis and Emotional Release: Engaging in the creative process can serve as a form of catharsis, allowing individuals to release pent-up emotions and find emotional relief. Whether through painting, drawing, sculpture, or other art forms, the act of creating can be inherently therapeutic, providing a means of processing and coping with difficult emotions.
5. Reflection and Insight: Art creation and appreciation encourage introspection and self-reflection. By engaging with their own artwork or experiencing the work of others, individuals can gain insight into their own emotions, thoughts, and experiences, fostering greater self-awareness and emotional understanding.
6. Connection and Empathy: Art has the power to evoke empathy and forge connections between individuals. Through shared experiences of art, viewers can empathize with the emotions expressed by artists and recognize commonalities in their own emotional lives, fostering a sense of connection and understanding.
Overall, art serves as a rich and versatile medium for exploring, expressing, and processing emotions in ways that may transcend the limitations of verbal communication. Whether through the creation or appreciation of art, individuals can tap into a deeper reservoir of emotional expression and insight, enriching their understanding of themselves and others in the process.
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what are different turbulent inlet conditions in T-Junction pipe flows, which leads to turbulence at T-Junctions during fluid flows
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What are different turbulent inlet conditions in T-Junction pipe flows? These will have little effect on the result, provided that you set the inlet conditions sufficiently far upstream of the junction i.e. in comparison to the flow establishment length; in any case greater than 100 times the Hydraulic Radius. In these conditions, you may put uniform turbulent intensity at the inlet of the order of a few percent and a turbulent dissipation compatible with the pressure loss that would be calculated from the White-Colebrook formula for example.
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What is the accepted percentage of error? in case of I developed a mathematical model for the parameters of pump, when the flow is turbulent? What is the accepted percentage of error? in case of I developed a mathematical model for the parameters of pump, when the flow is turbulent? compared with the reported values of previous studies?
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First, "error" means you know the "exact" value, a thing that is difficult to immagine to have in a real flow in pump.
Then, assuming you have some experimental value to compare with, the percentage of the difference can depends on the specific variable. Furthrmore, in a preliminary stage, a larger difference can be acceptable while in a more advanced stage you need to be more strict.
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is wind spectrum consume mean wind and turbulence both ? and how the mean wind will be calculated from measured wind data?
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The wind spectrum in structural engineering assesses wind effects on vertical slender structures. Derived from the Power Spectral Density (PSD), it reflects wind energy distribution across frequencies. It encompasses the Turbulence Component, representing wind speed fluctuations crucial for dynamic analysis, and the Mean Wind Component, an average speed over time, considered in structural assessments.
To calculate the mean wind speed from measured wind data, you typically perform a time-averaging process. The mean wind speed (U) is calculated as the average of the instantaneous wind speed measurements (u(t)) over a specific time duration (T):
U = (1/T) int{0}^{T} u(t) .dt
Here, T is the averaging time, and u(t) is the instantaneous wind speed at time (t).
Wind buffeting loads result from a structure's dynamic response to turbulent wind, analyzed using the wind spectrum with mean wind and turbulence components. Employing methods like random vibration theory helps determine the dynamic response and induced loads. Crucially, accurate representation of the wind spectrum demands a thorough analysis of wind data, considering turbulence intensity and length scales. Techniques like Fast Fourier Transform (FFT) transform time-domain wind data into the frequency domain for precise spectrum analysis.
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In fluid mechanics and computational fluid dynamics (CFD), the fluctuating velocity components u' v' w'′ represent the turbulent fluctuations in the velocity field. These components are used to model the turbulent behavior of fluid flow. The prime notation (u' v' w') denotes the deviation of the velocity from its mean value (U,V,W).
For laminar flow, turbulence is generally not considered, and the flow is assumed to be smooth and ordered. In this case, the fluctuating velocity components (u' v' w') are essentially zero.
In CFD simulations using software like FLUENT, you typically specify the turbulence model and relevant parameters to simulate turbulent flows. Common turbulence models include the k-epsilon model, the k-omega model, and the Reynolds stress model. These models provide equations for the turbulent kinetic energy (k) and the turbulent dissipation rate (ϵ), from which the fluctuating velocity components (u' v' w') can be derived.
In FLUENT, you will need to set up your simulation by defining the geometry, boundary conditions, and fluid properties. Additionally, you'll need to specify the turbulence model and provide initial conditions for the turbulence variables. The software will then solve the governing equations, including the RANS equations and turbulence model equations, to obtain the mean flow field and turbulence quantities, including the fluctuating velocity components.
The specific steps may vary depending on the version of FLUENT and the turbulence model chosen, so it's recommended to refer to the FLUENT documentation or user guide for detailed instructions based on your simulation setup.
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Desta,
I am puzzled - you seem to have answered your own question.
Are you honestly looking for help?
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In engineering applications, understanding the Reynolds number is crucial for predicting the behavior of fluid flow. For low Reynolds numbers, laminar flow is desirable in scenarios such as internal pipes to minimize frictional losses. However, at higher Reynolds numbers, turbulent flow can enhance mixing and heat transfer, beneficial in applications like chemical reactors or cooling systems. Conversely, excessive turbulence can increase drag on vehicles or structures, impacting efficiency. Therefore, engineers carefully consider the Reynolds number to optimize the performance and efficiency of various systems involving fluid flow.
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Reynolds number is not univocally defined, there are several choice of lenght and velocity producing different values. Sometimes, the Re number is actually a function depending on distance.
Thus, depending on the flow problem, a suitable physical assumption based on a value is acceptable provided that the choice of the characteristic scales is such to get normalized (not only non-dimensional) the equations.
Note that the Re number is also a ratio between characteristic time scales of the problem.
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We consider cases of compressible and incompressible flows.
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A phenomenological solution can be found by considering the relation of the thickness of the boundary layer & the diameter of a cylinder in the system.
It will give a relation that involves the Reynolds number, the temperature & the pressure of the whole system.
Please check, the exercises in chapter 12 of the the textbook:
"Statistical Thermodynamics: An Engineering Approach" by Prof. John W. Daily. Cambridge University Press, 2019.
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Hello everybody,
I could not simulate wind speed fluctuation by assigning turbulence intensity (TI).
I simulate the fluid-structure interaction by using STAR-CCM+ and Abaqus, and I simulate the flow field of through IDDES. I set field functions to assign inlet velocity and turbulence intensity, respectively. Some points are set to record the time history of wind speed in freestream direction. However, results show that the wind speed do not fluctuate obviously (i.e. the wind speed just slightly vary with time). I calculated the turbulence intensity (TI) according to the definition of TI. The TI was 0.0001%, indicating that the wind speed was almost constant.
I set “Synthetic Turbulence Specification” from “none” to “intensity + length scale” in “continuum” and “region-boundary -inlet-physical conditions” when I just use STAR-CCM+ and do not use Abaqus. In this case, the wind speed vary obviously with time. However, there was warning when I set “Synthetic Turbulence Specification” in fluid-structure interaction:
“The Synthetic Turbulence Specification applied to boundary ‘S.Con.inlet’ in region “flow”, is not compatible with the Motion Specification in that region.”
The Synthetic Turbulence Specification should be suppressed when the mesh morphing of flow field was considered.
The setting of regions and simulation are shown in attachments.
The computational region was 1000 m (x) *500 m (y) * 500 m (z)
The section of structure was 6 m (x) *6 m (y) * 50 m (z)
Is there anything I forget to check? How can I get a certain level of turbulence at a specific spot in the field through inlet boundary specification?
Any feedback on the approach/idea itself is welcome too.
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first, to resolve fluctuations in turbulence you have to approach a DNS or, at least, a LES formulation.
then, to see physical fluctuations you have to let the solution developing, that is forget the arbitrary initial condition. That requires to wait some turnover times before to see the correlated fields.
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I determined the area weighted average pressure drop between inlet and outlet and used ((2*dell_p*D)/(L*rho*velocity ^2)) to determine friction factor. But the results do not match the expected results for a turbulent pipe flow. Any suggestion is appreciated.
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Determining the friction factor for turbulent pipe flow in ANSYS Fluent is typically straightforward, but there may be several reasons why your results do not match the expected values. Here are some suggestions to help you determine the friction factor accurately:
  1. Check Turbulence Model: Ensure that you are using an appropriate turbulence model for your pipe flow simulation. The most commonly used turbulence models for pipe flow are the k-epsilon and the Reynolds-averaged Navier-Stokes (RANS) models. The choice of turbulence model can significantly affect the friction factor results.
  2. Mesh Quality: Make sure that your mesh is of high quality and sufficiently refined near the pipe walls. A coarse or poorly-structured mesh can lead to inaccurate results. Use the y+ value to determine if your mesh is suitable for the chosen turbulence model. For wall functions or low-Reynolds number simulations, y+ values should be within a specific range.
  3. Boundary Conditions: Check that you have applied appropriate boundary conditions, especially at the inlet and outlet of the pipe. Ensure that the velocity and pressure boundary conditions are well-defined and realistic.
  4. Convergence: Verify that your simulation has reached convergence. Insufficient convergence can lead to inaccurate results. Monitor residuals and ensure they have reached a steady state.
  5. Solver Settings: Review the solver settings and numerical schemes used in your simulation. Ensure that you have chosen appropriate schemes for turbulence, pressure-velocity coupling, and discretization. Different schemes can impact the accuracy of your results.
  6. Y+ Value: Ensure that you have computed the y+ value correctly. The y+ value is essential for determining whether to use wall functions or resolve the near-wall region. Use a y+ calculator or a boundary layer resolution approach based on your turbulence model.
  7. Turbulence Intensity and Hydraulic Diameter: Double-check the values for turbulence intensity (TI) and hydraulic diameter (D) used in your calculation. Accurate values are crucial for calculating the friction factor.
  8. Verify Units: Make sure that all units in your simulation are consistent. Check that the units of density, velocity, diameter, and pressure are consistent with each other and with the units expected by the Fluent solver.
  9. Monitor the Boundary Layer: Visualize the near-wall boundary layer in your simulation results. Check if it is adequately resolved, and ensure that the grid spacing near the wall is sufficient.
  10. Compare to Literature Data: Finally, compare your results to well-established experimental or numerical data for turbulent pipe flow. If your results still do not match, it may be necessary to validate your simulation setup and boundary conditions against known benchmark cases.
By carefully reviewing and adjusting these aspects of your simulation, you should be able to determine the friction factor more accurately in ANSYS Fluent and achieve results that match the expected values for turbulent pipe flow.
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Can it be posited that the presence of a severe boundary layer separation, characterized by the detachment of the fluid flow from a solid surface, serves as a significant contributing factor to the augmentation of turbulent flow phenomena? In other words, is there a substantiated relationship between the adverse separation of the boundary layer and the amplification of turbulence in the flow field? Is it plausible to achieve a state of boundary layer separation characterized by an exceptionally smooth flow transition, resulting in nearly negligible levels of turbulence? In other words, can the phenomenon of boundary layer separation be effectively controlled and manipulated to minimize the formation and propagation of turbulent flow structures?
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Dear Doctor
"Through our patented complex geometries and by taking advantage of additive manufacturing, we have increased efficiency of  additively manufactured heat exchangers. Our internal geometry encourages swirls and mixing which helps to reduce thickness of boundary layer within our heat exchanger core.  Anyone within the field of heat exchangers understands the concept of a boundary layer. A simple explanation is that when a fluid flows through a channel or on a surface, a thin layer is formed on the interface between the wall and the fluid. In this thin layer, fluid velocity changes from zero (static) at the wall surface to freestream velocity at a certain distance away from the wall surface. A thick boundary layer has a negative effect on heat exchanger performance as it impedes heat transfer. Think of it like a blanket, thicker the blanket, the higher the insulation. This is not ideal for heat exchangers core as the main objective is to conduct heat from fluid to wall surface and vice-versa. Turbulent flow is generally more preferred in heat exchanger design. The swirling and diffusive characteristics of turbulent flow enhances heat transfer. Mixing induced by turbulent flow can also disrupt the growth of boundary layer on heat exchanger core surfaces. However, turbulent flow is often associated with higher pressure drop.
As mentioned, reducing the size of boundary layer and promoting turbulent flow can enhance the performance of a heat exchanger. This can be achieved through the following: -Increase fluid velocity – Speeding up fluid flow through core is an effective way of increasing heat transfer. However, appropriate balance between heat transfer gain and pressure drop penalty needs to be considered. Having closely packed fins and multipass configuration can increase fluid velocity through core. -Mixing enhancement features – Addition of features such as turbulators, baffles, and corrugation can further enhance heat transfer. Conflux Technology has been producing superior heat exchangers with high heat transfer and minimum pressure drop. This is realized through our patented complex geometries, extensive parameters optimization, and by leveraging Additive Manufacturing process and its intrinsic surface roughness."
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Reactor working schematic shown in the annex, driven by the stirring rod fan blade rotation of the metal hanging piece of the rotating flow impact, and the external conditions are satisfied with the Taylor number (Ta) to reach the critical value of the Taylor vortex. Then. Can flow in a high-temperature, high-pressure rotary reactor be analyzed using Taylor vortex theory?
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Liquid-phase working medium inside the reactor is simulated formation water, and the gas phase (CO2+N2) is above.
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Dear CFD Researchers,
Since AI tools are currently very popular, I am wondering if anyone use them to choose turbulence model for a CFD case.
So if you did, please share your experiences. Due to the answer, we can extend the boundaries of this discussion.
Thank you for your comments.
Kind regards,
Guven
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First question: where could have ChatGPT taken the relative information for training? Honestly, if you're going to use that, I can't see how you could not want to know about that.
Second question: why ChatGPT? This is not some complex information we can't extract from complicated data. It's just exactly there for you to learn or to search trough. Also, it could be better done by making a new net from scratch just about that, than using a LLM that really has nothing to do with this.
My general comment is that engineers and scientists should not look for answers in a tool that is not even tought to be what they want. ChatGPT just spits out words following a prompt and a statistical model. That is not different from a bad student that just goes by memory without understanding. ChatGPT is actually worst, as it never assumes it could not know something. You wanna ask that about turbulence models? Oh my...
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Hello everyone, Im studying an airflow inside a finned tubular heat exchanger at various inlet velocities in Fluent. Starting at 10 ms inlet velocity it runs smoothly and converges but with increasing velocity it starts to diverge (at 12,5ms) and i just cant explain why. Ive tried many different things: k-epsilon and omega SST models, different inlet turbulence intensities and settings (initial pressure), restricted backflow reversal, lower relaxation factors, etc.. Im using NIST real gas model of air. My initial guess was that it has to do with the mesh quality and y+ value, but after doubling the number of cells i still get the same results. Ideal gas model works fine at even larger velocities. Analyzing the results, my turbulent Reynolds number just skyrockets at the end of the domain. I would appreciate any help .
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Georgiy Tanasov Yes, it also could be a limitation. In my experience with Fluent, it sometimes behaves strangely and unpredictably, especially for larger meshes, parallel calculations, and UDFs.
Sometimes it is a trial-and-error process that need to be performed for a specific problem. So, let us know if you succeed in your simulation. Good luck!
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I am running sloshing simulation in a rectangular tank using ANSYS fluent. reynold's number lie in turbulence and as it is a wall bounded problem I calculated the first cell height of inflation layer assuming y+ value=50.(turbulence range is 30 to 200). but, some literatures stated that having y+ value=1 (laminar) resulted in better accuracy. so, how should I assume my y+ value?
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Hai Dr, how are you? I am attracted to your question as I have some information on it. Below, I supply you with all the answers you need, but I would really appreciate it if you could press the RECOMMENDATION buttons underneath my 3 research papers' titles in my AUTHOR section as a way of you saying thanks and appreciation for my time and knowledge sharing. Please do not be mistaken, there are few RECOMMENDATION buttons in RESEARCHGATE. One is RECOMMENDATION button for Questions and Answers and the other RECOMMENDATIONS button for papers by the Authors. I would appreciate if you could click the RECOMMENDATION button for my 3 papers under my AUTHORSHIP. Thank you in advance and in return I provide you with the answers to your question below :
The y+ value is a dimensionless parameter that is used to determine the thickness of the boundary layer in a CFD simulation. A y+ value of 50 is typically used for turbulent flows, while a y+ value of 1 is typically used for laminar flows.
In your case, you are simulating sloshing in a rectangular tank, which is a turbulent flow. However, some literatures have stated that having a y+ value of 1 (laminar) resulted in better accuracy. This is because the sloshing flow in your simulation may be laminar in some regions, such as near the walls of the tank.
If you are concerned about accuracy, you can try running your simulation with both a y+ value of 50 and a y+ value of 1. Then, you can compare the results of the two simulations and see which one produces more accurate results.
Ultimately, the best way to determine the y+ value for your simulation is to experiment and see what works best for your specific case.
Here are some additional things to keep in mind when choosing a y+ value:
  • The y+ value should be chosen based on the Reynolds number of the flow. A higher Reynolds number will require a lower y+ value.
  • The y+ value should also be chosen based on the type of flow. Turbulent flows typically require a lower y+ value than laminar flows.
  • The y+ value should be chosen based on the accuracy that is required. A lower y+ value will result in more accurate results, but it will also require a finer mesh.
I hope this can shed some light on your exp.
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More specifically, I want the comparison in wavenumber-based power spectra, opposed to frequency-based. That would include converting multiple signals into a cross spectrum, finding the phase, and then the final conversion to wavenumber.
Extra points if it is in the field of plasma physics and magnetic signals.
Thanks in advance!
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Here is the DOI to my paper developing the wavenumber spectrum from wavelet analysis: https://pubs.aip.org/aip/pop/article/30/8/082303/2906229/Estimates-of-the-wavenumber-wavelet-power-spectrum
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Turbulence structure is described by the formation of eddies. Size of eddies vary based on the turbulence length scale ( (Kolmogrove, Reynold and Hinze). Smaller eddies describes intense turbulence, larger eddies display low turbulence zone.
Recently, I came across a book by Bertin and Cummings, which says there are no physical laws to describe detailed turbulence structure pattern.
Are there any ?
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Turbulent flows occur for high Reynolds numbers. The energy cascade transfers turbulent energy from large to smaller eddies via inertial interactions with no energy dissipation. Viscous dissipation occurs in the smallest eddies for which the Reynolds number that characterizes their movement is of order 1 (Kolmogorov scale)
For more, I would recommend the book by Tennekes, H., & Lumley, J. L. (1972). A first course in turbulence. MIT Press (more than 12 000 citations). As suggested by its title, the book is a basis for a fundamental understanding of the physical mechanisms of turbulence and for the acquisition of the methodological elements related to the phenomenological approach applied to the analysis of basic turbulent flows. The book is Available on:
https://www.academia.edu/download/54563360/Henk_Tennekes__John_L._Lumley_A_First_Course_in_Turbulence.pdf (more than 12 000 citations) is essential for a fundamental understanding of the physical mechanisms of turbulence and for the acquisition of the methodological elements related to the phenomenological approach applied to the analysis basic turbulent flows.
Description by the authors "This is the first book specifically designed to offer the student a smooth transitionary course between elementary fluid dynamics (which gives only last-minute attention to turbulence) and the professional literature on turbulent flow, where an advanced viewpoint is assumed.
The subject of turbulence, the most forbidding in fluid dynamics, has usually proved treacherous to the beginner, caught in the whirls and eddies of its nonlinearities and statistical imponderables. This is the first book specifically designed to offer the student a smooth transitionary course between elementary fluid dynamics (which gives only last-minute attention to turbulence) and the professional literature on turbulent flow, where an advanced viewpoint is assumed. Moreover, the text has been developed for students, engineers, and scientists with different technical backgrounds and interests. Almost all flows, natural and man-made, are turbulent. Thus the subject is the concern of geophysical and environmental scientists (in dealing with atmospheric jet streams, ocean currents, and the flow of rivers, for example), of astrophysicists (in studying the photospheres of the sun and stars or mapping gaseous nebulae), and of engineers (in calculating pipe flows, jets, or wakes). Many such examples are discussed in the book. The approach taken avoids the difficulties of advanced mathematical development on the one side and the morass of experimental detail and empirical data on the other. As a result of following its midstream course, the text gives the student a physical understanding of the subject and deepens his intuitive insight into those problems that cannot now be rigorously solved. In particular, dimensional analysis is used extensively in dealing with those problems whose exact solution is mathematically elusive. Dimensional reasoning, scale arguments, and similarity rules are introduced at the beginning and are applied throughout. A discussion of Reynolds stress and the kinetic theory of gases provides the contrast needed to put mixing-length theory into proper perspective: the authors present a thorough comparison between the mixing-length models and dimensional analysis of shear flows. This is followed by an extensive treatment of vorticity dynamics, including vortex stretching and vorticity budgets. Two chapters are devoted to boundary-free shear flows and well-bounded turbulent shear flows. The examples presented include wakes, jets, shear layers, thermal plumes, atmospheric boundary layers, pipe and channel flow, and boundary layers in pressure gradients. The spatial structure of turbulent flow has been the subject of analysis in the book up to this point, at which a compact but thorough introduction to statistical methods is given. This prepares the reader to understand the stochastic and spectral structure of turbulence. The remainder of the book consists of applications of the statistical approach to the study of turbulent transport (including diffusion and mixing) and turbulent spectra."
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[[ lfh note: This question has been hijacked by mistakenly celebrating a very non-responsive lecture on turbulence with Popular Answers. The lecture is even placed before discussion of the question. In my opinion it was without malice by RG or the person who posted it. Please read that "answer" on Page 4 below after reading actual discussion and clarification of the question, because the lecture is good history. ]]
[Original question comment] I think that the process of flow curvature formation at any scale in a fluid requires a pressure gradient across the curvature. The result outside the curve is increased internal thermal energy there. During subsequent decay of the curved flow, the curving kinetic energy fills the low pressure inside the curvature.
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You might find the thought experiment in my previous post interesting. It is a consequence of your suggestion that I read Sir James Jeans An Introduction to the Kinetic Theory of Gases and my choice to read his The Dynamical Theory of Gases as well. Writing the thought experiment triggered greater insight into processes because I had to address problems with answers that ring true. It also produced a richer view of a laminar flow past a cylinder with believable cause of curvature. I really appreciate our discussion that has led to it.
Happy Trails, Len
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Every organization that strives to survive, to develop and to be sustainable, must be ready to face all the challenges that today’s turbulent and uncertain times carry with them. Organizations of all types and sizes are faced by external and internal factors and influences that make it uncertain whether they will achieve their objectives. The almost unimaginable pace of technical and technological progress, the dramatic acceleration of changes in all spheres of life, as well as the general feelings of uncertainty, actually can raise the question as to what extent is prevention still really possible at all?
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Today, "prevention by design" is necessary. When creating a product or designing a service, it is necessary to assess possible risks and prevent them immediately. Example: packing products in environmentally friendly packaging or developing operating systems without security flaws or generously rewarding employees so they don't reveal professional secrets....
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Hi folks!
It is well known that the apparent stochasticity of turbulent processes stems from the extreme sensitivity of the DETERMINISTIC underlying differential equations to very small changes in the initial and boundary conditions human beings aren't able to measure.
Given our limitations, for the same measured conditions, a deterministic turbulent flow can thus display a wide array of different behaviours.
Can QUANTUM MECHANICAL random fluctuations also change the initial and boundary conditions in such a way that the turbulent flow would behave in a different manner?
In other words, if we assume that quantum mechanics is genuinely indetermistic, can it propagate that "true" randomness towards (some) turbulent processes and flows?
Or would decoherence hinder this from happening?
I wasn't able to find any peer-reviewed papers on this.
Many thanks for your answers!
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Howdy Marc Fischer,
I applaud your clear statement that "random" and "stochastic" are terms to be applied to human perceptions and efforts, since the underlying dynamics of fluids in turbulence is deterministic. Very rare observation, very welcome! (The fluid knows.)
As far as "quantum mechanics is genuinely indetermistic," some of us think the jury is still out on that because your comments on turbulence apply to human limitations, including ignorance, there also.
Given the experience of "QUANTUM MECHANICAL random fluctuations" by turbulent processes that is possible, I doubt that they could affect the state of the turbulence as having too little energy. "Random" absorption of a photon by a molecule that enhanced the molecule's internal energy would have an effect, of course, by increasing the thermal-motion energy of the fluid, but I doubt it could be noticed in turbulence, even by the flow being triggered to new behavior. This affect is very different from application of human precision in initial conditions that enters mathematical expressions with such strong leverage because of the mathematical non-linearity.
I also applaud the association you have made as one of the ways to trigger insight, but too often the answer in a specific case is no.
Happy Trails, Len
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This question delves into the fundamental nature of turbulence, a ubiquitous phenomenon in fluid dynamics that is characterized by chaotic and unpredictable fluid motion. Exploring the mechanisms behind turbulence and finding ways to better understand and predict its behavior is a challenging and active area of research with broad implications in various fields, including engineering, meteorology, and environmental sciences. This question opens up avenues for investigating turbulence models, turbulence control strategies, and the development of advanced computational techniques to simulate and analyze turbulent flows.
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Thank you for your remarks. Of course, any theory of education has limits because students are a varied lot. The students who have liked my approach (few) responded to their being treated as inquiring persons.
In this case I find a bit of mystery because Sanjibonny Buragohain has shown awareness of the answer to her question, and her profile indicates even deeper understanding would be present. I would like to know what she seeks to know better and to help, by normal, spiral, personal, or whatever educational means she prefers.
Or, I may be completely off-track. It has happened before.
Happy Trails, Len
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Hello everyone, I'm currently working on a project in which I need to simulate turbulent flow in a duct. For the inlet boundary condition, I'd like to use the Synthetic Eddy Method (SEM) to superimpose synthetic turbulence onto the mean flow. While I understand the basic theory behind SEM, I'm struggling a bit with the actual implementation in code. Specifically, I'm unsure about generating the eddies according to the energy spectrum, imposing a divergence-free condition, and handling eddies that exit the computational domain. Would anyone be able to provide guidance or recommend resources (books, papers, online tutorials) that include detailed explanations or examples of SEM implementation in code? Additionally, are there any open-source CFD software or libraries that provide SEM as a built-in feature, which I could use as a reference? Any advice or direction would be greatly appreciated!
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One way to generate turbulence at the inlet is by implementing Divergence Free Synthetic Eddy Method. The method is first introduced by Poletto (2015) with theoretical framework described in his thesis as below;
The method is now integrated within OpenFOAM software. Tutorials with regards to channel flow is accessible within the software. The method seems easy to be implemented as three statistical parameters of Reynold's stress (R), Turbulent Length Scale (L) and Mean velocity (U) can be calculated using DNS and RANS (need further validation) to be prescribed at the inlet. You can perform the initial simulation using these two methods, read and write the parameters in a file, then supply them inside the "Constant" directory inside openFoam. Then, set the inlet boundary condition as turbulent inlet as the type of the boundary condition. Below is for your further reference;
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Does anyone know the mechanism of shear production of turbulence? We know that a term with this name appears in the RANS energy equation, but what does it represent? Notice that energy can be transported or transformed, but never `produced’.
To explain: my interest is in wall-bounded shear flows, particularly in the atmospheric boundary layer. I know that the RANS energy equation is a statement that the divergence of the flux of mechanical energy equals the local dissipation rate. Why is the idea of local `production’ of turbulence kinetic energy so widely held when motions in the surface layer are, in reality, sustained by downwards transfer of mechanical energy from the flow above?
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Hi Keith,
Thank you for posting this nice discussion. Since the so called "Shear production term" involves u'w', I want to add a point, regarding the erratic behaviour of the quantity u'w' in atmospheric surface layer flows, where the constant flux layer is never achieved (specially in unstable conditions).
Keith and I wrote a paper on that in Boundary-layer meteorology, ( ) where we showed how the momentum flux co-spectra do not follow any particular scaling in convective flows. Moreover, a few previous literature do show that the surface shear stress as directly measured from the surface plates do not match with the values of u'w', rather they are always underestimated. Also, if one takes an alternate route to define friction velocity from the log-law fittings in neutral flows, those values too mismatch with u_{*}. Therefore, there remains a doubt of how to accurately estimate the friction velocity in atmospheric flows.
Cheers,
Subharthi
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Do obstacles in a channel change the regime from laminar to turbulent while the Reynolds number is under 2300 (approximately 1000)?
Please introduce related studies.
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The Reynolds number UD/nu=2300 is based on a smooth circular pipe of diameter D, with STEADY mean flow velocity U and fluid of kinematic viscosity nu. Below this critical Reynolds number any perturbation due to an obstacle will not cause persistent turbulence to occur far downstream of the obstacle. Of course locally the wake of a blunt body placed in the pipe can be turbulent, but soon the flow will relaminarize if we travel further downstream. Above Re=2300 the flow does not need to be turbulent. It can be turbulent if there is a sufficiently large initial upstream perturbation. In principle the flow can remain laminar if the inlet is very smooth and care is taken to avoid vibrations. Experimentally fully developed laminar pipe flows have been achieved for Re=500. 000. It is important to realize that this critical Reynolds number does depend on the geometry of the cross-section of the channel. For a rectangular channel of height h and width w >>h, usually one considers a Reynolds number Re=Uh/nu based on the channel heigth. The critical Reynolds number for allowing turbulence is around Re=hU/nu=1100. There is however much less literature on flows through slit shaped channels than circular pipes. If you consider an open channel flow, clearly the critical Reynolds number will be quite different from Re=2300 and of course it does depend on the length scale used in the definition of this Reynolds number!
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I've worked on simulating 3D VIV (a cylinder forced by Karman vortex street) and been stuck with settings. Considering the transition to turbulence due to the oscillation of cylinder (Re≤200, laminar upstream), "SST k-ω coupling with intermittency transition" is my scheme now.
However, I'm not sure whether I should enable "intermittency transition" since I don't fully understand the statement given in the user's guide, which says "The Transition SST model is not Galilean invariant and should therefore not be applied to surfaces that move relative to the coordinate system for which the velocity field is computed; for such cases the Intermittency Transition model should be used instead."
I don't understand the bold sentence in the statement especially. Does it mean the moving surface of cylinder (in my case)? Hope anyone can provide any guideline. Thank you so much.
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Yi-Sian Ciou, understanding the concept of Galilean invariance can indeed be beneficial in the field of fluid dynamics, especially if you plan to pursue a career in computational fluid dynamics (CFD) or similar areas. While the term may not appear explicitly in some introductory fluid dynamics textbooks, it is a fundamental concept in physics and is particularly relevant in CFD.
Galilean invariance, also known as Galilean relativity, states that the laws of physics should be the same in all inertial frames of reference. In the context of fluid dynamics and CFD, this means that the predictions of a model should remain consistent when the frame of reference is changed. In other words, the model should provide the same results regardless of whether you analyze the flow from a stationary or moving reference frame.
As you progress in your studies and delve deeper into fluid dynamics and CFD, you may encounter various turbulence models with different levels of Galilean invariance. Understanding this concept will help you make informed decisions when choosing the appropriate turbulence model for a particular simulation.
So, if you plan to work with CFD or fluid dynamics in the future, it would be worthwhile to spend some time learning about Galilean invariance. You can start by exploring classical mechanics or introductory physics textbooks, as well as online resources, to build a strong foundation in this concept.
Good luck with your studies, and feel free to reach out if you have any further questions! Regards,
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G'day,
I'm working on simulating 3D Karman Vortex Street, confused how to distinguish laminar and turbulence. As the pic shows (this is a frame before starting oscillation), there is downwash near the top of the cylinder, but the Reynolds number in this case doesn't exceed 200, namely, it should be laminar. ----------------update--->
Yesterday, I asked Perplexity Ai to find some info and it provided some reference talking about the wake structure due to the end of finite cylinder. So now I just want to collect your suggestions, since it seems no reference directly indicates "the downwash is inherent no matter the flow is laminar or turbulent". So if anyone knows relevant paper, please let me know, thank you so much!
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Understanding what "laminar regime" stands for is a topic of basic fluid dynamics.
The flow over an obstacle can be laminar even in case it is unsteady, as happpens in the classic case of laminar vortex shedding.
Turbulence is charactertized by a wide range of vortical structures.
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I have been trying to get forced homogeneous isotropic turbulence field. I added a linear forcing term to NS equation with a fixed coefficient A. It works when my domain is 2pi cube. However when I scale my domain to mm i.e. my domain is 2pi*1e-3, the method is not working.
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Thanks
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Hello all
I have two questions;
1- First of all, is it possible to generate HIT inside a rectangle? If so, it is called HIT again?
2- if Nx=Nz but Ny is different, How can I calculate power spectrum?
when Nx=Ny=Nz, it is possible to use below openfoam algorithm;https://www.openfoam.com/documentation/guides/latest/api/energySpectrum_8C_source.html
but in my case Nx=Nz =/ Ny
Thanks,
Farzad
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1- It is possible to generate a harmonic impact test (HIT) inside a rectangle, but the specific terminology for this type of test may vary. HIT is a type of test used to study the response of a structure to dynamic loading. A HIT inside a rectangle would involve applying a dynamic load to a structure in the shape of a rectangle. The specific terminology used to describe this test may vary depending on the field or industry.
2- If Nx = Nz but Ny is different, you can still calculate the power spectrum by analyzing the frequency components of the signals along the three different axes (Nx, Ny, Nz). The frequency components can be obtained using a Fast Fourier Transform (FFT) or similar technique. The power spectrum can be calculated by squaring the magnitude of the FFT and normalizing the result by the number of data points. To account for the difference in Ny, you may need to apply some modifications to the normalization or analysis process.
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SMEs need to build its resilience to survive in turbulent times. Identifying core competencies and factors that build resilience are challenging for SMEs. The question persists, what makes SMEs resilient in turbulent times?
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SME what does it mean here?
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Hello everyone
I have read Lundgren(2002) article "Linearly forced isotropic turbulence" which by adding a linear forcing to momentum equation, he was able to get forced isotropic turbulence. I did the same thing(I had initial HIT velocity field) and after a while flow filed start to make mean flow which theoretically must be zero. Also, TKE oscillates very dramatically which is not my desire. Now, my question is that, is there any other Linear forcing method or any other simple method to keep forcing to initial HIT and make it Forced HIT?
Thanks,
Farzad
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Farzad Farajidizaji Linear forcing is a method for producing high-resolution ice thickness (HIT) fields from low-resolution data. Fitting a linear model to the low-resolution data and then using this model to predict the high-resolution HIT values are the steps involved.
To use linear forcing to produce HIT in Python, you'll need a low-resolution HIT dataset as well as a collection of predictor variables to describe the link between ice thickness and other elements like temperature, precipitation, and elevation. Here's an example of how linear forcing may be used to create HIT in Python:
import numpy as np
from sklearn.linear_model import LinearRegression
# Load the low-resolution HIT data and predictor variables
lowres_hit = ...
predictors = ...
# Create a LinearRegression model
model = LinearRegression()
# Fit the model to the low-resolution HIT data
model.fit(predictors, lowres_hit)
# Generate high-resolution HIT predictions
highres_hit = model.predict(predictors)
The LinearRegression class from the sklearn package is used in this code to fit a linear model to the low-resolution HIT data. Using the same predictor variables, it then applies this model to create high-resolution HIT predictions.
I hope this was helpful! Please let me know if you have any queries or require any other support.
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Need a turbulence generator for generating the initial velocity field for direct numerical simulation of decaying compressible isotropic turbulence.
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I have witnessed that higher values of TI lead to a decay in the Ct curves in the moderate range of wind speed (8-13 m/s). For high wind speeds it is seen that the changing TI does not have an impact on the curves but it does for moderate wind speeds. I've been trying to find a response for that, but it is not clear at all.
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By definition turbulence intensity (TI) is function of mean wind speed and it's standard deviation measured at specific height. TI generally reduces with increase in height above ground. but thrust coefficient (CT) for a wind turbine varies inversely with square of wind speed.
For low to moderate wind speeds the turbulence intensity is high, and when the turbine is in power production mode with increasing power, the controller tries to optimize the power generated by turbine to reduce the axial thrust force acting on rotor blades with an aim to increase the fatigue life of turbine/components. This causes the decay in thrust coefficient, however for higher wind speeds, the controller regulates power output to constant value by pitching blades out of wind. So effectively TI has little or no impact on thrust coefficient curves of turbine.
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In the case of open channel flow, why does the turbulence shear stress remains constant in the turbulent logarithmic layer?
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Within the logarithmic zone it is assumed that there is an equilibrium Production=Dissipation. Le logarithmic law writes (u/u*)=(1/kapa)*Ln(u*y/nu)+C so that (du/dz)=u*/(kapa*y)
So Dissipation=Production= u'v'*(du/dz)=kapa*y*(u*)*(du/dz)^2=((u*)^3)/(kapa*y)
We have thus u'v'=(u*)^2. it is thus a zone where the turbulent shear stress is constant
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This developed turbulent flow codes is a finite element computer model, written in FORTRAN which was developed to solve the Reynolds equations of motion and continuity for steady and fully developed mean turbulent flow. The Finite Element mathematical treatment of this matter is reported in the following Ph.D. reference at CSU, Fort Collins, Co, the USA (please the link to this dissertation is https://mountainscholar.org/handle/10217/235417). Later on this code was extended to three dimensional and unsteady flows. The turbulent stresses appearing in the Reynolds equations are modeled in terms of mean velocity nonlinear gradients and turbulent viscosity. The non-linear algebraic stress model used in closed channels is totally different from the one used in open channels with new algebraic open surface proximity functions. A two equation turbulence model consisting of the turbulent kinetic energy (K), and its rate of dissipation (ε) evaluates the turbulent viscosity that appears in the algebraic stress models.
For wall bounded flows especially at corners (such as at an airplane's body to wing), my code succeeded in an excellent manner in simulating the main velocity, secondary velocities and turbulence structure (turbulent viscosity, K, and ε). In addition, distributions of the non-gravitational pressure and turbulent stresses are well predicted too. You may contact me for samples of the results of simulating turbulent flow in a square duct. Along the corner bisector the maximum secondary velocity divided by the average shear velocity is calculated as 0.31 which is in agreement with experimental data of Brundrett & Baines (1964) of about 0.32. For the wall bisector a value of 0.21 is predicted versus a measured value of 0.20 by Gessner and Emery 1980. Bulging of the velocity contours toward the corner is well predicted which is important in reducing separation due to adverse longitudinal pressure gradients. No up-winding or (over/under) relaxation are used. Non-linear Newton–Raphson that has quadratic convergence is used for dealing with the system of nonlinear equations. The boundary shear stress is calculated and is shown to be affected by the secondary velocities.
- For open channel flows: a very distinct feature in my nonlinear k-ε model is the use of an-isotropic turbulent viscosity in which the turbulent viscosity in the vertical direction differs from that in the lateral direction, a feature not existing in any existing CFD code to my knowledge. The model succeeded in predicting the depression in the main velocity maximum to be at 0.6 from the bed in a channel with aspect ratio of 1:2. The secondary velocity structure is also well predicted . Another important feature is prediction of the cellular secondary cells due to periodic roughness changes along the bed or walls. This helps in investigation of flow over ribbed surfaces.
Now How much does the source code for this turbulent flow CFD code worth in US $?
I appreciate honest answers and offers.
For more details I can be reached at my email:
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I agree with Filippo, CFD-online would attract more answers from developers.
Let me also clarify that both OpenFOAM and Code_Saturne (not sure about SU2) have today the most advanced turbulence models, which include non linear ones as well. This is especially so for Code_Saturne, that has been the preferred choice for developments in Manchester. If we allow to consider closed source codes, well, Ansys Fluent just has the same capabilities with several algebraic non linear and full Reynolds Stress Models. Also, let's not forget that Florian Menter is in charge for that in Ansys.
I'm not really into free surface flows, so I can't really tell, but the same reasoning applies here. There are several options for the most diverse conditions. In general, coming from commercial development, let me tell you that every low hanging fruit that works for general solvers with unstructured grids is generally a no-brainer and eventually gets in (as long as the model is actually helpful).
This just to clarify that if you intend the CFD solver market as a battle field, it's not the early 90's Fluent that you're going to face. It's 2022, and there is also Siemens with Star, Cadence with ex-Numeca, Altair with several products, and few other less known vendors of high quality.
This, however, it's not the main point here, in my opinion, in valuing your code. I haven't read your thesis, but it seems that the main point of your development is sitting there open to everyone. So, if it is usable for general flow solvers, I guess you are left with little to none, because everyone can already use your model without your code. Also, 5k lines of code is very little in this case. If you want a comparison, I have seen fully original source codes of that length sold, non exclusively, for about 30k USD. So, if ever, in your case the amount should be much lower. Also, note that we are speaking about selling the source code for third party reuse at their wish, not licensing the code here.
So, excluding, de facto, the previous hypothesis as meaningful, let's assume that your unique modeling is not usable in other codes or that not everything is open to everyone, which is basically the same. I am myself into CFD code development and a fully parallel unstructured solver with basic functionality (multi-zone with CHT, URANS, steady/unsteady, implicit/explicit, incompressible/compressible, scalars and all the machinery to make it usable like a major commercial solver) can be fit in 20k-25k lines of code. So, at 5k, I assume your code is weak on some of these basic features. So, we are presumably speaking of a niche code that can eventually do some specific things very well, but doesn't seem more generally usable.
Thus, finally getting to your question, I think the valuation for your code is totally up to the niche you are addressing, the problem you are solving and how costly it is for your niche. If your code solves a multi-billion dollar problem for a very rich industry and nobody else can solve that same problem, people would pay as much as you ask, even if your code was still written on punch cards or could run on ancient hardware of limited availability. The CFD market is full of verticals that get exploited, but it is really up to you to actually know if your code fits any of them.
But if you don't address a specific unsolved problem nor have a more general usability, I don't think you can really monetize your code.
Also, I didn't mention this but, the code must obviously be also usable by a general audience. If it requires expert adjusting for every case, it becomes extremely difficult to use and very few will be able to, even if it addresses a multi-billion dollar problem.
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Should I use openfoam for direct numerical simulation of compressible turbulence (decaying compressible isotropic turbulence)?
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Samuel Oluwakorede Oyefusi Thanks for your suggestion.
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Dear All,
Good time,
In Ansys Fluent, I am using 2D non-premixed turbulent combustion model, I am using WSGG model to find the influence of radiation on participating species, my query is,
After thousand of iteration step, contour for temperature, is convincing and giving a good flame structure but incase of CO2 and H2O, what I see is, from flame till outlet the whole combustor is filled of CO2 or H2O, what parameter should I change/consider in my fluent simulation to make it better?
For your convenience I am attaching contour of both T and CO2.
TIA.
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The temperature profile indicates a diffusion flame, but the concentration profile seems like a pre-mixed flame where all the CO2 forms at the flame-front. To go further needs geometrical details of gas and air inlets and the enclosure as these determine the flame temperature and shape. However, my impression is that there is something wrong with the mathematical model used.
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The maximum theoretical effect of a drag reducing agent (DRA) is the same as a pipe in laminar flow, where all of the turbulence is eliminated by the drag reducing agent. In this context, can a laminar viscous model be chosen for the simulation of the effect a drag reducing agent on the pressure drop in a pipeline with Reynolds number (Re) > 10^7?
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For laminar flows, the friction coefficient is linear function with 1/Re it means a direct function of dynamic viscosity. In this domain increasing viscosity could cause an increase in shear stress for Newtonian fluids (water, HC oils what ever a fluid in the pipeline), while the radial velocity gradient is assumed to be identical on the pipe cross sectional area. Pipe entrance effect is neglected downstream the equivalent pipe length, here the pressure drop increases with pipe length flowing Darcy Law (including the friction coefficient). DRA model could be applied in this context, but an iterative solution is foreseen.
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Hello,
I have a hot-wire measurement record in the boundary layer in the wind tunnel. There should be fully developed turbulent boundary layer in the wind tunnel flow. I used Matlab to calculate the integral lentgh scale a then the non dimensional spectra. In the pictrure, I used the pspectrum function (red), Welch (cyan), Fast-Fourier transform (blue) to calculate the spectral densities. Then I added the von Karman spectrum (green), but the slope of its right part is not the same as the others. I added also the Kolmogorov inertial scale f^(-5/3) and its slope corresponds with the calculated spectrums. Do you have any ideas why the von Karman spectrum is tilted and the Kolmogorov scale is not? I am running out of ideas, thanks for help.
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Sorry to say that the figures have no sense, why do you have different range of resolved frequencies?
And if you are in the BL, the flow is not homogeneos, the spectra will depends on y+.
You should clarify the way you are measuring the velocity.
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The artery geometry has an irregular shape where there is possibility of transitioning from laminar to turbulent for most cases in the stenoid(narrow) region , but for some of arteries flow remains laminar. What happens if I use KEpsilon for modeling all my 50 patients?
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You should at least really be running a URANS (Unsteady RANS) simulation. Then time-averaging the results if the flow is indeed statistically steady (the time average will be the same as the ensemble if turbulence is statistically steady by ergodic theorem).
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Hi all,
I am going to use either Ansys CFX or Ansys Fluent solver to simulate flow past a semi-submerged rectangular cylinder, as shown in Fig. 1. The main goal here is to achieve an accurate prediction of pressure distribution over the cylinder, which seems to be particularly reliant on the capability of the CFD model to predict the separation and the reattachment of the flow correctly. I would appreciate any tips regarding the following questions.
Q1. How important is the choice of the turbulence model? Which models are superior? Could the flow be modelled as being laminar at all?
Q2. How important is the approach to the free surface? Could the free surface be modelled as a free-slip wall to reduce computational costs? Is it necessary to precisely track the free surface using the VOF model for this study?
Q3. What are the most appropriate boundary conditions for the simulation?
Q4. Which is more suitable for this problem? CFX or Fluent?
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If the size t is less than 8-12 distances to the bottom surface, the drag force will be determined, among other things, by the added masses of the liquid reflected from the bottom surface. If this is not important, then in the model you need to specify a distance of more than 12.
The number of wall layers is enough 5.
From above on a free surface, the wind has a speed and direction?
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All, It's known of curse that viscosity depends on pressure. Often this dependence is weak and sometimes it is significant. It is an odd and unmotivated question but, nevertheless, I am wondering if our parameterizations of turbulent viscosities should also include some measure of local pressure fluctuations? (This may be a question resolved long ago by people doing compressible turbulence.) I'm hoping to learn from people's answers and ideas. Thanks! Bill
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It does via velocity. Because we don't have a dynamic equation for pressure, we employ a correction to velocity, and use velocity gradient to model viscosity. We do this (bring pressure fluctuations) in turbulence models, but we don't yet know how to do it properly.
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Hello,
I am trying to measure the quality metrics of some turbulence blurred images with respect to the diffraction-limited image. I have about 9000 blurred images for each cases of lower and higher turbulence. But, it looks like my measures for mean PSNR and mean SSIM increases with higher turbulence. I am trying to find an explanation for this intriguing behavior. Any thoughts on this will be helpful.
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Thanks Shafagat Mahmudova,
The link you provided was a good reference to look at the quality metrics and their relative comparison. However, I have tried a few more metrics but it looks like the pattern remains the same. For example, my average image entropy is increasing with higher turbulence strength (or blurring) whereas it should be the opposite.
Any thoughts on that would be helpful.
~ Ashfiq
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Sudden reversal in magnetic field is the origin of switchback. The reconnecting field lines creates shear driven turbulence.
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u r welcome~
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Dear All,
I want to generate an initial velocity field for homogenous isotropic turbulence. I learned that inverse Fourier calculates it from the energy spectrum of the form.
E(k)=k4e-2(k/k0)^2
However, the inverse Fourier transform of the function is not so straightforward. Does anyone know any good documentation for Fourier or Inverse Fourier transform for the turbulence energy spectrum?
Also, I have seen some papers using sinusoidal functions as the initial velocity field in HIT. However, I don't understand how it pops out from the inverse FFT of the energy spectrum. Can someone through some light on it?
Thank you
Krishna
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I have a specific case about internal pipe flow with constant heat flux. Although the inlet boundary condition is laminar, the flow is a passing transition (a significant part of the tube) and turbulent regime along the tube (because of the change of thermophysical properties depending on implied heat). SST models with intermittency term (For fully laminar flow, γ = 0 and the model reverts to a laminar solver. When γ = 1, the flow is fully turbulent.) can catch laminar/transitional and turbulent flow regimes. These models were designed for turbulent inlet boundary conditions (models solve intermittency term, so it needs extra boundary conditions such as turbulent intensity). Can Transitional SST Models be used for laminar inlet / turbulent outlet boundary conditions? If so, what is the approach?
Regards,
EB