Abstract
The paper deals with steady-state turbulent fountains in a homogeneous surrounding. A set of mono-dimensional conservation equations is first derived from the Navier–Stokes equations. In contrast with equations used for plumes or rising fountains, these equations reveal additional terms in order to account for the effect of the (annular) down-flow on the fountain up-flow. Large-eddy simulations are then performed and used to determine, from radial profiles, the values of the constants (associated with these additional terms) to be fitted in the model. With these constants, analytical solutions of the model for steady-state fountain are proposed and compared with previous experiments.
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Notes
The CFD code ISIS can be freely downloaded from the following website: https://gforge.irsn.fr/gf/project/isis/.
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Appendices
Appendix 1
This appendix details the formulation of ‘the-top hat’ confined model used in this study.
From the Navier–Stokes Eq. (2), (3) and (4) and after some algebra, Carazzo et al. [12] derived this new set of equations:
The main interest of these equations is that the vertical velocity w is involved in all the r-derivative terms. Then, these terms will vanish when integrated over the up-flow region since \(w(z,r=b)=0\). To integrate these three equations, they also introduced the so-called shape functions of velocity, of density deficit and of shear stress
Let us now introduce the following integrals which slightly differ from those given by Carazzo et al. [12]
where \( r' = r / b \) is the dimensionless radial coordinate.
By integrating Eq. (30), (31) and (32) with respect to \(r' \) from \(0\) to \(1\), we obtain the following set of equations:
These equations can be rewritten in a form similar to those given by Morton et al. [28], providing (5), (6) and (7), in which the parameters of the theoretical model are
The main steps of the calculations presented in this appendix are summarized in Fig. 11 in the form of a diagram.
Appendix 2
In order to obtain analytical expressions for the fountain height and in the same way as done by [11], it is convenient to treat separately the two regimes corresponding to weak (\(\varGamma _i \gg 1\)) or forced (\(\varGamma _i \ll 1\)) fountains.
In the case of weak fountains, we introduce the following relations
in (16), then we are led to
According to the fact that in the vicinity of the fountain height \(H_{ss}\), \(\varGamma \) tends towards \(\infty \) as \(\xi \rightarrow H_{ss}\varLambda _i\), the fountain function can be sought in this region in the form
where \(\epsilon (\xi )\) is a function which tends to zero when \(\xi \rightarrow H_{ss} \varLambda _i\).
By injecting (46) in (45) and by expanding this equation with respect to \(\epsilon \), we obtain at leading order
where \(H_{ss}\varLambda _i\) is the constant of integration. In order to determine this constant, we use the fact that \(\varGamma _i \gg 1\) which allows us to consider that the approximated solution remains accurate even at the vicinity of the source (\(\varGamma _{\mathrm{approx}}(\xi =0)\simeq \varGamma _i\)). This last step leads us to the following relation :
In the case of forced fountains, Eq. (17) can be split into two parts as follows
which finally leads us to the fountain height given by (24).
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Mehaddi, R., Vaux, S., Candelier, F. et al. On the modelling of steady turbulent fountains. Environ Fluid Mech 15, 1115–1134 (2015). https://doi.org/10.1007/s10652-015-9400-9
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DOI: https://doi.org/10.1007/s10652-015-9400-9