RU Camelopardalis is a W Virginis variable which has light curve with
irregularly variable amplitude, mean value and phase. The Fourier-spec
trum of the light variation shows a complex structure with the charact
eristic period of 22 days. The visual observations before 1960 also sh
ow this complex variation, but a dominant regular component was found
in these data, too. There are some possible mechanisms underlying the
erratic variations of stars: deterministic chaos, stochastic excitatio
n and multiperiodicity with unresolved frequencies. In order to choose
from these mechanisms we applied different kinds of analyses and nume
rical tests. The time-frequency analysis of the light curve indicates
that the variation cannot be modelled by a multiperiodic variation. Ph
ase-space reconstruction of the data was made in order to prove the ex
istence of low dimensional chaos, but the phase portraits do not show
any regular structure, i.e. the data cannot be modelled with a low dim
ensional (approximately 2 - 3) chaotic system.