The problem of thermal stabilization of telescope optics is familiar to many amateur astronomers. The mirror of a reflector telescope, just taken for observation from a warm room or car interior, takes a long time to cool down to the ambient air temperature. A boundary layer of warm air appears above the reflecting surface, and upward currents rise along the tube. All this spoils the picture, especially at high magnification. At a temperature difference of 10-15° the main mirror of a large telescope can cool down for several hours, making it impossible to make quality observations.