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Calculating the point of void departure, zd,
iteratively
It is shown in this section that it is important to calculate the point of void
departure accurately in order to predict the subcooled void fraction accurately.
When we use a very fine computational grid it is sufficient to predict
to within
one steplength. However, for a coarse grid which is
constructed by the guidelines described in section 8.5
the first steplengths are in general very coarse due to a low linear heat
generation rate q'. The result is that
is calculated using values
of q' and the physical properties for a z-level which is off by as much as
30 cm when compared to the true zd.
Since q' is increasing rapidly in this area
will be seriously
affected by this calculation procedure.
The error on
will canalize itself to the subcooled void fraction
where
especially in the region totally dominated by subcooled boiling
may be off by more than 20 % as compared to a fine grid solution. In Figure
8.2 we have compared plots of the coarse grid void fraction
calculation with a fine grid solution in which the
is calculated
very accurately (the accurate method of calculating
is described
later in this section). As we can see the error is largest in the area with a
high degree of subcooling and the error decreases with decreasing subcooling
according to the Levy profile fit (see (6.97)). In Figure
8.3 we can see the influence of the erroneous
on the
flow quality distribution. The error on
is as we can see also serious--in
fact the relative errors on
and
are of the same order of
magnitude. The error on the void fraction is most
inconvenient since the void fraction is feed back to the neutronics calculation
with an error on the power distribution as the result.
It is important to note that this 20 % error on
arises from an error
on
of only 1 %, ie
is a sensitive quantity in
regard to the calculation of
.
The remedy for the above mentioned problem is to calculate
(and
zd for that matter) accurately without considering the underlying grid.
In Figure 8.4 we see a close-up of the computational grid around
the point of void departure. Our problem is to find the point of void departure
which lies somewhere between the grid points illustrated.
In our implementation we have used the properties at the previous z-level to
evaluate the void departure criterion at the current z-point (see
(6.93)), ie for
which is appropriate for our
purpose we calculate the enthalpy at the point of void departure at grid point
i by the expression
 |
(8.12) |
where hf is evaluated at point i-1. The reason for this calculational
procedure is that we ignore the property variation which has a limited impact on
in order to save some property calculations.
With reference to Figure 8.4 the problem is to find the void
departure point, zd. We should be aware that a situation can occur in which
the void departure point is situated a bit to the left of the point zi. This
is a result of using the old properties to calculate
8.4.
In any case we can state that our task is to solve the equation
![\begin{displaymath}
\mbox{$<\!{h}\!>$}- h_{\ell,d}(z) = 0 \qquad\mbox{where}\quad z \in [z_j;z_{i+1}]
\end{displaymath}](img1451.gif) |
(8.13) |
where
is the mixture enthalpy (see (6.103) p.
) in [J/kg] and j is either i or i-1 as discussed
previously. The solution to (8.13) is the point of void departure,
zd.
Since we have to solve a non-linear equation (8.13) numerically in a
limited range of z-values the best choice is to use a numerical method in the
group of enclosure methods which, as stated previously, work on a range of
the independent variable.
We have chosen the Pegasus method described in section
7.3 in order to solve (8.13) since it is one of
the fastest and more robust enclosure methods.
For comparison we have included Figures 8.5 and
8.6 which compare coarse and fine grid solutions when we employ
an accurate grid independent calculation of .
As we can see the
coarse grid solution lies close to the fine grid solution!
Since we know that
is one of the critical quantities it is
interesting to investigate the accuracy of the Saha-Zuber correlation. As noted
in section 6.7.2.4 it is the expression for
which
is of interest in BWR design. The Saha-Zuber correlation for this case may be
written
 |
(8.14) |
where we have
 |
(8.15) |
When Saha and Zuber [34, p. 6-57] compared this expression to
experimental data they derived up to 25 % from the correlation, ie the Stanton
number varied from 0.0049 to 0.0081.
The impact on the value of
for a typical BWR operating state in
shown in Table 8.1.
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Up: Core flow implementation
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