Abstract
Abstract We investigate switching of the accretion column between the stellar hemispheres in the magnetosphere of a star with the dipole magnetic field aligned with the stellar rotation axis. We show that such switching can produce “hiccups” in the observed lightcurves. The intensity of emitted radiation from the stellar surface as seen by distant observers is computed from our two dimensional axisymmetric viscous and resistive magnetohydrodynamic numerical simulations. This result is used to construct a three-dimensional model of a star with the ring-shaped hot spots from the accretion columns at the stellar surface. We compute the intensity from such hot spots. To obtain a non-axisymmetric model with arc-shaped hot spots, we remove a ring section in the azimuthal direction from the hot-spots and compute the intensity of the radiated emission. Such models can be used to relate physical parameters in the simulations to the observations. We show an example with the intensity computed from our model compared to observational light curve.
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