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I use two-dimensional axisymmetric numerical simulations of star-diskmagnetospheric interaction to construct a three-dimensional model of hot spotson the star created by infalling accretion columns. The intensity of emittedradiation is computed with minimal assumptions, as seen by observers atinfinity from the different angles. In the illustrative examples, shown is achange in the intensity curve with changes in the geometry of the model, andalso a change in results with modification in the physical parameters in thesimulation.

Light curve variation caused by accretion column switching stellar hemispheres