At about half-past four the edge of the sun was visibly indented; some persons maintained that they could see the moon some time previous to the contact; but this must probably be ascribed to a lively imagination. Smoked glass now came into demand, and all eyes were anxiously watching the rapidly decreasing orb. I had secured, through the kindness of an influential friend, an excellent position on the court-house, itself a high building and situated on the highest point in the town, commanding a fine view in all directions, particularly toward the north-west, from which quarter the shadow was sweeping toward us at the rate of more than a mile every second. Some five or six gentlemen had followed me to the roof of the building, after which the ladder leading to the cupola was drawn up, to prevent a general ascent by the crowd below. At a quarter or twenty minutes past five, the wind began to abate, and the darkness was quite noticeable, and of course from that time continually increased, the general effect being like that of moonlight some time before the totality. The darkness was much more striking than at any time during the annular eclipse of 1854; this was probably owing to the total absence of any cloud, which would have reflected and multiplied the light of the unobscured portion of the sun, as on that occasion. A minute or so before the totality, the complete circle of the moon was easily visible, with faint brushes of light streaming from it in all directions, which were soon to assume much larger dimensions, and, apparently, though not really, a greater brilliancy. I cast now my eyes to the north-western horizon, and saw a brick-red tinge on the sky evidently caused by the rapidly approaching umbra. The long-expected moment had come; the last direct beam from the sun vanished, and a magnificent corona of rays, faint, of course, compared with the solar light, but bright in the prevailing gloom, shot out round the disc of the moon. These rays were prolonged in four directions at right angles to each other much more than elsewhere; having in these directions a length about equal to the sun's diameter, making the corona or aureola obviously cruciform in its shape.