Hydrodynamics and heat transfer for downward liquid metal flow in a rectangular channel in the presence of a coplanar magnetic field

2016 ◽  
Vol 52 (1) ◽  
pp. 155-162
Author(s):  
N. Yu. Pyatnitskaya ◽  
◽  
E. V. Sviridov ◽  
N. G. Razuvanov ◽  
◽  
...  
Keyword(s):  
Magnetic Field ◽  
Heat Transfer ◽  
Liquid Metal ◽  
Rectangular Channel ◽  
Metal Flow ◽  
Liquid Metal Flow

scholarly journals Magneto-Convective Analyses of the PbLi Flow for the EU-WCLL Fusion Breeding Blanket

Energies ◽  
2021 ◽  
Vol 14 (19) ◽  
pp. 6192
Author(s):  
Fernando R. Urgorri ◽  
Ivan Fernández-Berceruelo ◽  
David Rapisarda
Keyword(s):  
Magnetic Field ◽  
Heat Transfer ◽  
Liquid Metal ◽  
Heat Source ◽  
Metal Flow ◽  
Intense Magnetic Field ◽  
Liquid Metal Flow ◽  
Computational Analyses ◽  
Fusion Breeding ◽  
Convective Phenomenon

The Water Cooled Lithium Lead (WCLL) breeding blanket is one of the driver blanket concepts under development for the European Demonstration Reactor (DEMO). The majority of the blanket volume is occupied by flowing PbLi at eutectic composition. This liquid metal flow is subdued to high fluxes of particles coming from the plasma which are translated into a high non-homogeneous heat volumetric source inside the fluid. The heat is removed from the PbLi thanks to several water tubes immersed in the metal. The dynamics of the PbLi is heavily affected by the heat source and by the position of the tubes. Moreover, the conducting fluid is electrically coupled with the intense magnetic field used for the plasma confinement. As a result, the PbLi flow is strongly affected by the Magnetohydrodynamics (MHD) forces. In the WCLL, the MHD and convective interactions are expected to be comparable. Therefore, the PbLi dynamics and consequently the heat transfer between the liquid metal and the water coolant will be ruled by the magneto-convective phenomenon. This work presents 3D computational analyses of the PbLi flow in the frontal region of the WCLL design. The simulations include the combined effect of MHD forces caused by the magnetic field and the buoyancy interaction created by the temperature distribution. The latter is determined by the PbLi dynamics, the volumetric heat source and the position of the water tubes. Simulations have allowed computing the heat transfer between the PbLi and the water tubes. Nusselt and Grashof numbers have been obtained in the different regions of the system.

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