ИСТИНА

We present the five-year observations of deeply eclipsing polar FL Ceti (SDSS J015543.40+002807.2). During these years polar was at all three stages of brightness - a ``low'', an ``intermediate'' and a ``high''. The profile of the light curves depends on the level of brightness, i.e. on the amount of transferred matter. In a ``high'' state there is no any faint phase of brightness and some humps are observed. In a ``low'' state a faint phase lasted about of 1/3 of the orbital period is present.