  The paper presents results of laboratory experiment modeling the interaction
between Lunar magnetic anomalies and Solar wind. To model the LMA we use
quadrupole magnetic field. The main dimentionless parameter of the problem, the
ion inertia length relative to the mini-magnetosphere size, well corresponds
between experiment and LMA conditions. The main result is measurement of the
magnetically reflected proton fluxes, which show qualitative agreement to
available satellite data.
