Total Solar Eclipse 2006, corona
Fig. 31: The corona of the sun. On can see the lines of the sun's magnetic field with the pols on the lower left and upper right side. The brightness range of the corona from the inner edge to the most distant outer parts is so huge that it can't be captured wit one single shot on one slide. — William Optics Zenithstar 105 ED Triplet APO f/6, 2x Nikon Teleconverter, Nikon F100, Fujichrome Velvia 100F, 1/2s, Side, Turkey, 29 March 2006