Abstract
The flow patterns in the mock-up model of the cross-flow type mercury target were measured using the PIV technique under water flow conditions at room temperature. The experimental results were compared with the analytical results conducted with the thermal hydraulic analysis code, STAR-CD. As a result, it was confirmed experimentally that the cross-flow could be realized in most of the proton beam path area, where the removal of the high density heat is important, with the proper flow rate distribution along the proton beam path. The analytical result showed the good correspondence to the experimental result. Then the mercury flow field and the temperature distribution were analyzed taking the volumetric heat generation by the spallation reaction into consideration. The volumetric heat generation calculated for the proton beam energy and power of 1.5GeV and 5MW were assumed in the analysis.The mercury flow analysis showed that the maximum mercury temperature less than the design criteria of 300 deg C can be attained with the inlet mercury velocity of more than 1.1m/s and that the recirculation flow seen in the rear of the proton beam path is considered to cause no excessive temperature rise.
