The automatic VESSEL-coupling technique was tested with two coolant mixing cases. One is performed in a generic four-loop PWR and the other in the AP1000 reactor.
4.1. The Coolant Mixing in a Four-Loop PWR
The TRACE model consists of an RPV represented by a CY-V, a core represented by a CA-V, hot-legs, and cold-legs. The overall RPV height and radius are 12.245 and 1.7002 m. It is discretized into 16 axial nodes, 4 azimuthal nodes, and 2 radial nodes. The reactor has four hot-legs and four cold-legs symmetrically connected to the RPV. In this model, the circuits are not considered. The Cartesian Vessel is subdivided into nine square fuel assemblies arranged in a 3 × 3 matrix.
Figure 10 shows the TRACE models for the RPV and the core.
Four FILL and BREAK components are connected to a portion of the cold and hot legs to define the boundary conditions of the problem, e.g., loops mass flow rate, coolant temperature, and pressure. The coolant enters the cold legs, then flows into the downcomer of the RPV and from there to the lower plenum where the flow changes direction and flows upwards entering into the core bottom. The coolant flows through the core and enters the upper plenum. Finally, it exits the RPV and flows into the BREAKs through the hot legs. The core is modeled by the Cartesian VESSEL, which is connected to the RPV-axial face Nr. 2 (core inlet) and the axial face Nr. 11 (core outlet). Hence, the core region in the CY-V is blocked, i.e., no coolant flows through it. Please take
Figure 9 as a reference. Once the code is launched, the steps listed under
Section 3.2.1 are performed sequentially. According to the VESSEL components configuration, 32 additional PIPEs (as Junctions connecting the two VESSEL components) are constructed and inserted into the TRACE data structure automatically. In total, 16 of them are at the core inlet plane and 16 are at the core outlet plane.
Figure 11 illustrates the quantitative distribution of the additional PIPEs from the point of the CA-V (1 × 4 + 2 × 4 + 4 × 1 = 16).
TRACE first runs a Steady-State (SS) simulation. During the SS, the inlet velocity at loop1 is 15 m/s. Inlet velocities of the other three loops are identical to 10 m/s. The inlet coolant temperature is 400 K. The outlet pressure is 15.55 MPa. After the SS, a TRACE transient (TS) simulation is carried out. The total problem time is 50.0 s. The boundary conditions for the transient are given in
Table 1.
The cold coolant and hot coolant first mix a little bit in the CY-V downcomer. Then, the main mixing effect happens in the CY-V lower plenum. The coolant then flows from the CY-V lower plenum to the CA-V core and there in the core some mixing would happen. Next, the coolant flows out of the CA-V core and to the CY-V upper plenum. There the final mixing takes place. Particularly for this testing case, what we are concerned about is whether the coolant can flow between the two VESSELs properly and whether the coolant mixing effect behaves rationally in/between the two VESSELs.
Figure 12 exhibits the qualitative distribution of the coolant temperature in the RPV and the core at the end of the transient. It can be observed that the coolant temperature of the cylindrical sectors of the CY-V corresponding to the loop-1 and of the Cartesian cells linked to it are hotter than the one of the other sectors/cells.
The coolant temperature distribution at the core inlet demonstrates that the coolant flows from the CY-V to the CA-V correctly. Similarly, the coolant temperature distribution at the core outlet shows that the coolant flow from the CA-V to the CY-V is passed from one VESSEL to the other properly. The roughly same temperature distribution at the CA-V inlet and outlet planes indicates weak coolant mixing in the core. However, we can see an obvious difference between the CY-V inlet and outlet planes. There at the CY-V outlet, the hot part is cooler and the cold part is hotter than that at the CY-V inlet. This indicates a considerable mixing in the core, which is not consistent with the conclusion from the CA-V analysis. This phenomenon is due to a “mixing” when the coolant flows from the coarse CY-V mesh to the fine CA-V mesh (from the lower plenum to the core) and then back to the CY-V mesh (from core to upper plenum). The intersections between fields in the different meshes introduce a sort of “averaging effect” into the system and thus cause a stronger mixing effect in the CY-V than that in the CA-V. This effect is now under study at KIT.
Another phenomenon we can observe from the figure is that the colors of the outer ring in the CY-V mesh intrude into the inner ring. These sorts of distortions are due to MED meshing limitations. The appearance has no concern with the physical aspects.
Figure 13 and
Figure 14 exhibit the coolant temperature evolutions at the core inlet planes of the two VESSELs. Each curve represents an individual sector/cell on the planes. The former is for the CY-V (4 sectors) and the latter is for the CA-V (9 cells). The increase in the coolant temperature at the core inlet of sectors 2 and 4 is due to the coolant mixing taking place in the downcomer since these sectors are the neighbor sectors of sector 1 (hotter coolant).
Keeping in mind the cell indexing of the Cartesian VESSEL in
Figure 10, it can be seen in
Figure 14 that cell 9 is the hottest, cells 6 and 8 the second hottest, and cell 5 the third hottest. The coolant temperature of cell 9 is similar to the CY-V sector 1 while the coolant temperature of cells 6 and 8 are similar to sectors 2 and 4, see
Figure 13 and
Figure 14. The reason for it is the spatial correspondence of these cells and sectors which are automatically mapped with the MEDcoupling library. The transfer of physical fields between the two VESSELs is straightforward. On the contrary, cells 2/4/5/6/8 in the CA-V get the coolant from multiple cells of the CY-V. Thus, some kind of “averaging” effect would happen in those cells. Particularly, cells 6 and 8 of the CA-V mix the coolant from the hottest cell 1 and cell 2/4 of the CY-V. Therefore, their temperature curves in
Figure 14 are in the middle of cell 1 and cell 3/7. Similarly, cells 2 and 4 of the CA-V mix the coolant from the coldest cell 3 and cell 4/2 of the CY-V. Therefore, their temperature curves in
Figure 14 are in the middle of cell 3 and cell 3/7. Cell 5 is special because its coolant is from all of the 4 cells of CY-V.
Figure 15 and
Figure 16 show the coolant temperature evolutions at the core outlet planes of the two VESSELs. Each curve represents an individual cell/sector on the planes. The former is for the CA-V (9 cells) and the latter is for the CY-V (4 sectors). The minor difference between
Figure 14 and
Figure 16 indicates a weak coolant mixing effect in the core (by CA-V). However, a similar “averaging” effect happens when the coolant flows from the nine cells of CA-V to the four sectors of CY-V. The reason is that each of the four sectors in the CY-V gets the coolant from multiple cells of the CA-V. Particularly, sector 1 mixes the coolant from cell 5/6/8/9. Sector 2 mixes the coolant from the cell 4/5/7/8. Sector 3 mixes the coolant from the cell 1/2/4/5. Sector 4 mixes the coolant from the cell 2/3/5/6. Due to the two “averaging” effects happening on the core inlet/outlet as well as the coolant mixing in the core region, the temperature of the core flow-out coolant is more homogeneous than the core flow-in coolant in the CY-V.
In general, it can be stated that the coolant mixing in the downcomer is significant while the one inside the core is moderate.
4.2. The Coolant Mixing in the AP1000 Reactor
The configuration of the reactor and nodalization of the model were previously illustrated in
Section 2.2 and
Section 3. The RPV is represented by a CY-V and the core by a CA-V. The CY-V is nodalized to 8 azimuthal sectors and 2 radial rings while the CA-V is nodalized to 15 × 15 = 165 cells (each cell represents 1 fuel assembly), among which, 68 are dummy cells and 157 are real cells.
Figure 17 only presents the real cells. Consequently, 456 additional PIPEs (as Junctions connecting the two VESSEL components) are constructed and inserted into the TRACE data structure automatically by the approach presented here. In total, 228 (1 × 96 + 2 × 56 + 3 × 4 + 8 × 1 = 228,
Figure 17) of them are at the core inlet plane and 228 are at the core outlet plane.
Figure 17 illustrates the quantitative distribution of the additional PIPEs from the point of the CA-V (for example, the yellow 8 means this cell connects to 8 CY-V sectors via 8 additional PIPEs as Junctions).
Figure 17 gives the CY-V mesh as well. There, the sector indexes, the location of the loops, and the hot/cold legs are shown: the cold-legs (vessel inlet) of loop1 correspond to sectors 4 and 6 while the cold-legs of loop2 correspond to sectors 2 and 8. The hot-legs of loop1 and loop2 correspond to sectors 5 and 1.
First of all, a steady-state (SS) TRACE simulation is performed for an inlet mass flow rate of 3567 kg/s and coolant temperature of 553.7 K per loop (fixed as boundary conditions at the four FILL components). The outlet pressure is 15.45 MPa and is defined in the BREAK components. Afterward, a transient (TS) simulation is completed with the boundary conditions given in
Table 2. The transient lasts for 50 s.
The transient is defined by decreasing the coolant temperature of the loop-1 from 553.7 to 543.7 K at the transient beginning. As a consequence, a coolant mixing will take place in the CY-V downcomer, in the CY-V lower plenum and the mixing pattern will be propagated to the CA-V core. After the final mixing in the CY-V upper plenum, the coolant will flow out of the RPV. The main question is to check if the automatic VESSEL-coupling is working properly for a coolant mixing problem.
Figure 18 exhibits the coolant temperature distributions in both the CY-V (top) and the CA-V (bottom) as shown by the new post-processing capability implemented in TRACE. It can be observed that the coolant temperature field of the loop-1 corresponding part in the CY-V and CA-V meshes is cooler than other parts. Particularly, the coolant temperature distribution at the core inlets implies that the coolant temperature was correctly transferred from the CY-V to the CA-V by the automatic VESSEL-coupling approach. The same conclusion can be drawn for the coolant temperature distribution at the core outlets.
The coolant temperature evolution at the core inlet and outlet of the CY-V are plotted in
Figure 19 and
Figure 20, see
Figure 17 for sector indexes. The coolant mixing in the downcomer and lower plenum can be observed if we examine the coolant temperature evolutions of sectors 3 and 7 which are the results of the coolant mixing between the coolant of the sectors 2 and 4 and the sectors 8 and 6.
This mixing pattern propagates from the CY-V lower plenum to the CA-V core at the core inlet and from the CA-V core to the CY-V upper plenum at the core outlet, where the mixing continues to happen in a moderate manner leading to a small reduction in the coolant temperature of the sectors 1, 2, and 8 at the core outlet compared to the ones at the core inlet. Contrary to it, the coolant temperature of sectors 4, 5, and 6 increases slightly at the core outlet compared to the core values at the core inlet.
In
Figure 21, 16 representative cells of the CA-V are selected for the discussion of results from the CA-V side. To compare with the CY-V, 8 cells do not intersect with the CY-V sectors and their coolant comes from individual sectors. Eight cells intersect with the CY-V sectors and their coolant comes from two sectors. There, the correspondence of the CA-V cells with the CY-V sectors (and with the two loops) can be observed. The 16 representative cells are divided into two groups: the hot-part (loop2) and the cold-part (loop1).
Figure 22 and
Figure 23 show the coolant temperature evolutions of the hot-part and cold-part cells at the CA-V core inlet plane. Cells 1, 3, 5, 7, 9, 11, 13, and 15 have approximately identical trends as the corresponding sectors in the CY-V (1–8). Whereas some small differences can be observed due to the slight coolant mixing in the first level of the CA-V. Cells 2, 4, 6, 8, 10, 12, 14, and 16 are the CA-V cells that intersect with two CY-V sectors. The coolants from the two CY-V sectors mix when they flow into those CA-V cells. The mixing effect is inferred from
Figure 22 and
Figure 23, where the curves of the intersected CA-V cells located between their corresponding CY-V cells are exhibited.
Figure 24 and
Figure 25 give the coolant temperature evolution of the representative CA-V cells (
Figure 21) at the core outlet. Most of the curves are approximately identical to that of the same cells at the core inlet except for cells 15, 4, 6, and 7. Thus, we can tell that the coolant mixing in the CA-V is relatively weak. At the core outlet plane, the coolant flows from CA-V to CY-V. There, each CY-V cell connects to a set of multiple CA-V cells. Compared with
Figure 20, we can see a good agreement between the two distributions at the core outlets of the two VESSELs. If you look at sector 1 in the CY-V and cells 16, 1, and 2 in the CA-V, for example, the coolant temperature of sector 1 is slightly lower than the hottest cell 1 because colder coolant from boundary cells 2 and 16 contributes to sector 1 as well.
According to the analysis of the coolant mixing on the previous academic reactor, it can be inferred that the physical mixing and the “averaging effect” should both play a role in the AP1000 reactor when the coolant flows via the path of “CY-V to CA-V to CY-V”, because the meshes of the two VESSELs differ in spatial resolution and cell arrangement.
Figure 26 plots the coolant temperature profile at the core inlet and outlet of the AP1000 CY-V and CA-V. There, the data points, as well as the theta coordinates are the ones of the CY-V sectors and the indexed CA-V cells that were given in
Figure 21. The left subplot gives the field from CY-V, while the right gives the field from CA-V. For both subplots, the orange curve and block represent the field at the core inlet, while dark green represents the field at the core outlet.
We can see an obvious shrinkage of the hot part (between the lines 1–2 and 8–1) and an expansion of the cold part (between the lines 3–4 and 6–7) when comparing the temperature profile at the CY-V core outlet to that at the CY-V core inlet. The more eccentric the block is on this radar map, the more inhomogeneously the temperature field distributes at the core inlet or outlet planes.
Globally, the temperature band at the outlet moves closer to the center, which indicates a flatter coolant temperature distribution at the core outlet. However, this sort of shrinkage, expansion, and movement is not that noticeable in
Figure 26 (right). This leads to the conclusion that the coolant mixing in the CA-V is weak (consistent with the analysis in
Figure 22,
Figure 23,
Figure 24 and
Figure 25). Thus, we can conclude that the “averaging effect” contributes to the temperature flatting that is observed in
Figure 26 (left). This effect is still under study at present. Nevertheless, the result from the AP1000 reactor demonstrates the adequacy and efficiency of the automatic VESSEL-coupling approach presented and discussed here.