[en] The first two harmonics of sidereal wave in the intensity variations of the Budapest underground telescopes are studied on a year-to-year basis. By comparing the sidereal daily vectors obtained in sectors of opposite IMF directions at a pair of similar telescopes located at conjugate latitudes, one is able to disentangle the solar effects from a galactic anisotropy. Applying this procedure for the Budapest and Hobart measurements, the vector ascribable to galactic anisotropy has an amplitude of approximately 0.02% and phase approximately 5 hr. An attempt is made to draw some conclusion on the undistorted galactic anisotropy by taking into account the heliomagnetospheric deflection. (author)