Maps of molecular emission in the extended atmosphere of Mira. The emission was integrated in the spectral range corresponding to the main emission component between about 35 and 55 km s^-1 (optimized for each transition). The emission is shown in gray in units of Jy km s^-1 and with cyan contours at 10, 50, and 90% of the maximum flux. Additionally, a black contour at the 3σ noise level is shown. The location of continuum center of Mira A is indicated with a plus symbol whose size corresponds to the physical size of the stellar disk. The red contour shows the continuum emission at 50% of the peak value and represents the continuum extent smeared by the synthesized beam. The FWHMs of the beams are shown with hatched ellipses.