| Matrix or Vector | Geometry | Shape Functions | Integration Points |
|---|---|---|---|
| Thermal Conductivity Matrix | Between nodes I and J | Equation 11–13 | None |
| Convection between nodes I and K and between nodes J and L (optional) | None | None | |
| Pressure Conductivity Matrix | Between nodes I and J | Equation 11–12 | None |
| Specific Heat Matrix and Heat Generation Load Vector | Equation 11–13 | None | |
Transient pressure and compressibility effects are also not included.
The thermal and pressure aspects of the problem have been combined into one element having two different types of working variables: temperatures and pressures. The equilibrium equations for one element have the form of:
(13–150) |
where:
| [Ct] = specific heat matrix for one channel |
| {T} = nodal temperature vector |
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| {P} = nodal pressure vector |
| [Kt] = thermal conductivity matrix for one channel (includes effects of convection and mass transport) |
| [Kp] = pressure conductivity matrix for one channel |
| {Q} = nodal heat flow vector (input as HEAT on F command) |
| {w} = nodal fluid flow vector (input as FLOW on F command) |
| {Qg} = internal heat generation vector for one channel |
| {H} = gravity and pumping effects vector for one channel |
| Nc = number of parallel flow channels (input as Nc on R command) |
Specific Heat Matrix
The specific heat matrix is a diagonal matrix with each term being the sum of the corresponding row of a consistent specific heat matrix:
(13–151) |
where:
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| ρ = mass density (input as DENS on MP command |
| P = pressure (average of first two nodes) |
| Tabs = T + TOFFST = absolute temperature |
| T = temperature (average of first two nodes) |
| TOFFST = offset temperature (input on TOFFST command) |
| Cp = specific heat (input as C on MP command) |
| A = flow cross-sectional area (input as A on R command) |
| Lo = length of member (distance between nodes I and J) |
| Rgas = gas constant (input as Rgas on R command) |
Thermal Conductivity Matrix
The thermal conductivity matrix is given by:
(13–152) |
where:
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| Ks = thermal conductivity (input as KXX on MP command) |
| B2 = h AI |
| h = film coefficient (defined below) |
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| B3 = h AJ |
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| D = hydraulic diameter (input as D on R command) |
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| w = mass fluid flow rate in the element |
w may be determined by the program or may be input by the user:
(13–153) |
The above definitions of B4 and B5, as used by Equation 13–152, cause the energy change due to mass transport to be lumped at the outlet node.
The film coefficient h is defined as:
(13–154) |
Nu, the Nusselt number, is defined for KEYOPT(4) = 1 as:
(13–155) |
where:
A common usage of Equation 13–155 is the Dittus-Boelter correlation for fully developed turbulent flow in smooth tubes (Holman([56])):
(13–156) |
where:
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Heat Generation Load Vector
The internal heat generation load vector is due to both average heating effects and viscous damping:
(13–157) |
where:
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| VDF = viscous damping multiplier (input on RMORE command) |
| Cver = units conversion factor (input on RMORE command) |
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| v = average velocity |
The expression for the viscous damping part of Qn is based on fully developed laminar flow.
Bernoulli's equation is:
(13–158) |
where:
| Z = coordinate in the negative acceleration direction |
| P = pressure |
| γ = ρg |
| g = acceleration of gravity |
| v = velocity |
| PPMP = pump pressure (input as Pp on R command) |
| CL = loss coefficient |
The loss coefficient is defined as:
(13–159) |
where:
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| k = loss coefficient for typical fittings (input as K on R command) |
| f = Moody friction factor, defined below: |
For the first iteration of the first load step,
(13–160) |
where:
| fm = input as MU on MP command |
For all subsequent iterations
(13–161) |
The smooth pipe empirical correlation is:
(13–162) |
Bernoulli's Equation 13–158 may be simplified for this element, since the cross-sectional area of the pipe does not change. Therefore, continuity requires all velocities not to vary along the length. Hence v1 = v2 = va, so that Bernoulli's Equation 13–158 reduces to:
(13–163) |
Writing Equation 13–163 in terms of mass flow rate (w = ρAv), and rearranging terms to match the second half of Equation 13–150,
(13–164) |
Since the pressure drop (PI - PJ) is not linearly related to the flow (w), a nonlinear solution will be required. As the w term may not be squared in the solution, the square root of all terms is taken in a heuristic way:
(13–165) |
Defining:
(13–166) |
and
(13–167) |
Equation 13–165 reduces to:
(13–168) |
Hence, the pressure conductivity matrix is based on the term
and the pressure (gravity and pumping) load vector
is based on the term Bc PL.
Two further points:
(-ZI + ZJ)g is generalized as:
(13–170)
where:
{Δx} = vector from node I to node J {at} = translational acceleration vector which includes effects of angular velocities (see Acceleration Effect)