The experiment will use two optical telescopes: one, of 250/1200 mm, placed on the ground at high altitude (in mountains, at more that 1,500 m) and another one, of 125mm, airborne on a turbo jet flying along the umbra path on the Romanian territory. Both the telescopes will be equipped with fast reading (SCASI) 786 x 512 pixels CCD. As a byproduct, the digital images of the solar corona will be obtained during the totality; their processing could give valuable information about the coronal structure and dynamics as well as on solar prominences, coronal streamers and coronal mass ejections.