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shorter distance of the Admiralty and Chelsea. Dead flats are found to be universally unfavourable; and generally stations are useless nearly in the proportion of the miles of dead flat looked over. On the contrary, stations between hill and hill, looking across a valley, or series of valleys, are mostly clear; and water surfaces are found to produce fewer obscure days than land in any situation. The period least favourable of the same day is an hour or two before and after the sun's passage of the meridian, particularly on dead levels, where the play of the sun's rays on the rising exhalations renders distant vision exceedingly obscure. The tranquillity of the morning and evening are ascertained to be the most favourable hours for observation. A message from London to Portsmouth is usually transmitted in about fifteen minutes; but, by an experiment tried for the purpose, a single signal has been transmitted to Plymouth and back again in three minutes, which by the Telegraph route is at at least five hundred miles. In this instance, however, notice had been given to make ready, and every captain was at his post to receive and return the signals. The progress was at the rate of one hundred and seventy miles in a minute, or three miles per second, or three seconds at each station; a rapidity truly wonderful! The number of signals produced by the English telegraph is sixty-three--by which they represent the ten digits, the letters of the alphabet, many generic words, and all the numbers which can be expressed by sixty-three variations of the digits. The signals are sufficiently various to express any three or four words in twice as many changes of the shutters. The observers at these telegraphs are not expected to keep their eye constantly at the glass, but look only every five minutes for the signal to make ready. The telescopes are Dolland's Achromatics, at which one would wonder, if every thing done for governments were not converted into a job. The intention should have been to enable the observer to see the greatest number of hours; consequently the light should be intercepted by the smallest quantity of glass. Dollond's achromatics contain, however, six lenses, and possess no recommendation but their enlarged field, and their freedom from prismatic colours in that field; points of no consequence in looking through a fixed glass at a fixed and circumscribed object. The field of the Galilean telescope is quite larg
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