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small observatory at Berlin, whose more immediate object was to institute a series of simultaneous observations at concerted hours at Berlin, Paris, and Freiburg. In 1829 magnetic stations were established throughout Northern Asia, in connection with an expedition to that country which emanated from the Russian government; and in 1832 M. Gauss, the illustrious founder of a general theory of terrestrial magnetism, established a magnetic observatory at Goettingen, which was completed in 1834, and furnished with his ingenious instruments. In 1836 Baron Humboldt addressed a long and highly-interesting letter to the Duke of Sussex, then president of the Royal Society, urging the establishment of regular magnetical stations in the British possessions in North America, Australia, the Cape of Good Hope, and between the tropics, not only for the observation of the momentary perturbations of the needle, but also for that of its periodical and secular movements. This appeal was nobly responded to. The Royal Society, in conjunction with the British Association, called on government to advance the necessary funds to establish magnetical observatories at Greenwich, and in various parts of the British possessions; and in 1839-40 magnetical establishments were in activity at St. Helena, the Cape of Good Hope, Canada, and Van Diemen's Land. The munificence of the directors of the East India Company founded and furnished, at the request of the Royal Society, magnetic observatories at Simla, Madras, Bombay, and Singapore, and the observations will be published in a similar form to those of the British observatories. We will now briefly describe the scheme of observations, and the manner of making them in the different observatories. Each observatory is supplied with three magnetometers, or bars of magnetized steel, delicately suspended by threads of raw silk, which measure the magnetical declination, horizontal intensity, and vertical force--and such astronomical apparatus as is required for ascertaining the time and the true meridian. To these have also been added in each case a most complete and perfect set of meteorological instruments, carefully compared with the standards in possession of the Royal Society, not only for the purpose of affording the necessary corrections of the magnetic observations, but also with a view to obtaining at each station, at very little additional cost and trouble, a complete series of meteorological
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