Fig. 68: Prominences at the edge of the sun during the totality of a solar eclipse. Note that the diameter of the Sun is about 109 times that of Earth. The prominence at the top is about four times larger than Earth. — William Optics Zenithstar 105 ED Triplet APO f/7, 2x Nikon teleconverter, Nikon F100, Fujichrome Velvia 100F, 1/250s, Side, Turkey, March 29, 2006
