The following example input shows the application of heat flux as a function of temperature and X-position as a tabular load: fini /clear /prep7 mp,kxx,1,0.025 mp,c,1,0.28 mp,dens,1,0.054 blc4,0,0,10,2 et,1,plane55 esize,2 amesh,all *dim,MYTABLE,table,3,3,1,X,TEMP sfe,all,,hflux,,%mytable% *set,MYTABLE(0,1,1),10 *set,MYTABLE(0,2,1),100 *set,MYTABLE(0,3,1),1000 *set,MYTABLE(1,0,1),1 *set,MYTABLE(1,1,1),11 *set,MYTABLE(1,2,1),12 *set,MYTABLE(1,3,1),13 *set,MYTABLE(2,0,1),5 *set,MYTABLE(2,1,1),21 *set,MYTABLE(2,2,1),22 *set,MYTABLE(2,3,1),23 *set,MYTABLE(3,0,1),10 *set,MYTABLE(3,1,1),31 *set,MYTABLE(3,2,1),32 *set,MYTABLE(3,3,1),33 /psf,hflu,,2,0,1 /pbc,all,,1 eplo d,node(0,2,0),,10,,,,temp d,node(2,2,0),,50,,,,temp d,node(4,2,0),,100,,,,temp d,node(6,2,0),,200,,,,temp d,node(8,2,0),,500,,,,temp d,node(10,2,0),,1000,,,,temp /solu solve /out,loads,out sfelist /out *uilist,loads.out /eof