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Rising thermal bubble in adiabatic atmosphere |
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May 5, 2016, 13:07 |
Rising thermal bubble in adiabatic atmosphere
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#1 |
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Mihir Makwana
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I am trying to simulate a warm bubble(air) that rises in an adiabatic atmosphere using FVM.
The paper that i am reffering to is http://www.sciencedirect.com/science...21999107005384 The problem is defined in section 3.2) case 2 : Rising thermal bubble where it is mentioned that they are using no-flux B.C at all boundaries. Based on section 4.4.2 No-flux B.C, it is clear that no-flux B.C mean that velocity normal to boundary is zero along with gradient of tangential velocity being zero ( i.e free slip B.C at all boundaries) The kind of equations that i am solving are 1) continuity eqn 2) momentum eqn 3) pressure correction eqn Thus i need B.C for density, velocity and pressure correction at all boundaries Now, velocity B.C is obtained based on free slip. But what about the B.C for density and pressure correction ??? Based on the problem definition, what can be B.C for density and pressure correction ? Please help. Thanks in advance. |
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May 5, 2016, 14:11 |
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#2 |
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Filippo Maria Denaro
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I am not sure to understand you in what you wrote and now I cannot access the paper, I suppose pressure correction should imply the solving of the continuity equation.
What set of equations are you solving? |
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May 5, 2016, 14:46 |
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#3 | |
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Mihir Makwana
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Quote:
The continuity and momentum equations are http://i.imgur.com/2Kr1hxT.jpg The energy equation is converted to pressure equation and that is in turn converted to a pressure correction( dp(2) ) equation which is http://i.imgur.com/DvG7sBo.jpg In the pressure correction equation, terms on RHS are source terms Also, i have applied time integration to the pressure correction equation. The snippets from the paper which discuss the problem are 1) section 3.2 : case 2 : Rising thermal bubble http://i.imgur.com/RUZ307C.jpg 2) section 4.4.2 No-flux B.C http://i.imgur.com/OIzD8Fp.jpg In the paper the set of equations used are different from the one that i am using Also, based on my calculations Reynolds number for the flow is approx 10^7. Last edited by mihirmakwana6; May 5, 2016 at 16:18. Reason: images were not accessible |
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May 5, 2016, 16:02 |
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#4 |
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Filippo Maria Denaro
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the images are not available....
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May 5, 2016, 16:19 |
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#5 |
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Mihir Makwana
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May 5, 2016, 16:44 |
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#6 |
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Filippo Maria Denaro
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from the image of the energy equation, the field p_2 is a solution of an alliptic equation, right? Therefore the Neuman condition are derived from the Grad p_2 term in the momentum under projection along the normal direction to the boundary and using the condition u.n=0
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May 5, 2016, 16:52 |
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#7 | |
Member
Mihir Makwana
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Quote:
Due to no-flux B.C , u.n=0 thus grad_dp2 will be zero at the boundaries. This gives the B.C for pressure correction equation. but is this condition of grad_dp2 = 0 ,correct for the problem at hand. i.e can we apply it for this problem also, we need a B.C for density |
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May 5, 2016, 17:13 |
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#8 | |
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Mihir Makwana
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Quote:
1) grad_dp2 = 0 at all 4 boundaries 2) grad_density = 0 at all 4 boundaries ( i am not sure whether it is correct for the thermal bubble problem ) Based on the above B.C's along with free slip B.C for velocity, i ran the simulation. But the results are not matching I think there is some problem with the B.C that i am imposing |
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May 5, 2016, 17:31 |
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#9 |
Senior Member
Filippo Maria Denaro
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maybe you can find useful this recent paper and its references
http://eprints.eemcs.utwente.nl/2607...ukhvostova.pdf |
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May 5, 2016, 18:08 |
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#10 | |
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Mihir Makwana
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Quote:
I will have a look at it. |
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May 5, 2016, 18:50 |
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#11 |
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Filippo Maria Denaro
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As you can read, they set (1/rho) dp/dn = 0
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May 6, 2016, 02:44 |
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#12 |
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Mihir Makwana
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so, in my case it will be (1/rho) grad(dp2) = 0 i.e. grad(dp2) = 0 at all the boundaries.
Now, Density is obtained by solving continuity equations only for internal points i.e. I don't have values of density at the boundaries So, some B.C for density is needed Last edited by mihirmakwana6; May 6, 2016 at 02:48. Reason: needed to add something |
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May 6, 2016, 04:10 |
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#13 |
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Filippo Maria Denaro
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you can consider to solve the density equation in a FV around the node boundary...otherwise, an approximation such as d rho/dn = 0 (actually, the normal derivative should be expressed by the state equation)
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May 6, 2016, 05:24 |
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#14 |
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Mihir Makwana
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i did implement d rho/dn = 0 at all boundaries but it is not giving the expected result
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May 6, 2016, 05:26 |
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#15 |
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Filippo Maria Denaro
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May 6, 2016, 05:30 |
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#16 |
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Mihir Makwana
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May 6, 2016, 06:16 |
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#17 | |
Senior Member
Filippo Maria Denaro
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Quote:
I used that many years ago in a FV formulation on unstructured grid, unfortunaltely I don't remember those references. However, it is just a local integral formulation for a FV built around the node at the wall. |
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