The general diffusion of intelligence, both subjective and objective, as we may say, had of course excited great interest in the eclipse among the people, especially in that part of the country actually within or bordering upon the limits of totality; and though, of course, the nature of the expected event was fully understood by all the educated portion of the community, and by many of the uneducated, still there were some, especially in the rural districts, who vaguely apprehended some great event, to be probably of a disastrous nature, (a hailstorm was the most popular;) and perhaps were as much terrified in anticipation as any entirely ignorant people have ever been at the actual occurrence of this most impressive and sublime spectacle. Of course, excursions were planned by railroad companies and others to points on the line of the shadow, the usual directions for observing were extensively circulated, and the eclipse was made the catch-word for many advertisements whose substance had no connection with it. We are afraid that many persons may have lost the most beautiful features of the scene by a too persistent use of smoked glass, which of course was not necessary during or even near the time of the total obscuration. The weather for some days previous was not very promising--not on account of too much rain, but owing to the absence of it; and every evening the sun set in a bank of haze, which each day seemed to increase, and no storm occurred to clear the air of the burden accumulated by the drought. This was particularly unpromising for the photographers, who needed really clear air for good work; the times of beginning and ending, to which, formerly, great importance was attached, could probably have been observed nearly or quite as well through haze, or even thin cloud. We have just implied that less consequence is now attached to the time observations than was formerly the case; this is due to the great perfection which the lunar and solar theories have now attained, which is such that the prediction of the positions of the sun and moon, and even of the beginning and ending of an eclipse, can be made with greater accuracy, perhaps, than almost any one observer could note them. Still, by combination of all the results, some slight corrections to the tables now used may perhaps be deduced, and on the present occasion this portion of the work was not disregarded, but provided for with all the appliances of modern science.