COSMOS, VOL. II - World eBook Library
COSMOS, VOL. II - World eBook Library COSMOS, VOL. II - World eBook Library
11 Yl uninvestigated. DISCOVERIES IN THE CELESTIAL SPACES. 719 Observations of inclination were only carried on in a few of tlie capital cities of Western and Southern Europe; Graham, it is true, attempted in London in 1723, to measure by the oscillations of a magnetic needle, the intensity of the magnetic terrestrial force, which varies both with space and time, but since Borda's fruitless attempt on his last voyage to the Canaries, in 1776, Lemanon was the first who succeeded in La Perouses's expedition, in 1785, in comparing the intensity in different regions of the earth. In the year 1683, Edmund Halley sketched his theory of four magnetic poles or points of convergence, and of the periodical movement of the magnetic line without declination, basing his theory on a large number of existing observations of declination of very unequal value, by Baffin, Hudson, James Hall, and Schouten. In order to test this theory, and render it more perfect by the aid of new and more exact observations, the English Government permitted him to make three voyages (1698-1702) in the Atlantic Ocean, in a vessel under his own command. In one of these he reached 52 S. lat. This expedition constituted an epoch in the history of telluric magnetism. Its result was the construction of a general variation chart, on which the points at which navigators had found an equal amount of variation were connected together by curved lines. Never before, I believe, had any government fitted out a naval such ad- expedition for an object whose attainment promised vantages to practical navigation, while at the same time it deserved to be regarded as peculiarly scientific and physicomathematical. As no phenomenon can be thoroughly investigated by a careful observer, without being considered in its relation to other phenomena, Halley, on his return from his voyage hazarded the conjecture that the northern light was of a magnetic origin. I have remarked, in the general picture of nature, that Faraday's brilliant discovery (the evolution of light by magnetic force) has raised this hypothesis, enounced as early as in the year 1714, to empirical certainty. But if the laws of terrestrial magnetism are to be thoroughly investigated that is to say, if they are to be sought in the great cycle of the periodic movement in space of the three varieties of magnetic curves, it is by no means sufficient that the diurnal regular or disturbed course of the needle should be
720 COSMOS. observed at the magnetic stations which, since 1828, have begun to cover a considerable portion of the earth's surface, both in northern and southern latitudes;* but four times in every century an expedition of three ships should be sent out, to examine as nearly as possible at the same time the state of the magnetism of the earth, so far as it can be investigated in those parts which are covered by the ocean. The magnetic equator, or the curve at which the inclination is null, must not merely be inferred from the geographical position of its nodes (the intersections with the geographical equator) ; but the course of the ship should be made continually to vary' according to the observations of inclination, so as' never to leave the tract of the magnetic equator for the time being. Land expeditions should be combined with these voyages, in order, where masses of land cannot be entirely traversed, to determine at what points of the coast-line the magnetic curves (especially those having no variation) enter. Special attention might also perhaps be deservedly directed to the movement and gradual changes in the oval configuration, and almost concentric curves of variation of the two isolated closed systems in Eastern Asia, and in the South Pacific in the meridian of the Marquesas Group.f Since the memo- rable Antarctic expedition of Sir James Clarke Ross, (1839 1843,) fitted out with admirable instruments, has thrown so much light over the polar regions of the southern hemisphere, and has determined empirically the position of the magnetic south pole ; and since my honoured friend, the great mathematician, Frederick Gauss, has succeeded in establishing the first general theory of terrestrial magnetism, we need not renounce the hope that the many requirements of science and navigation will lead to the realisation of the plan I have already proposed. May the year 1850 be marked as the first normal epoch in -which the materials for a magnetic chart and may permanent scientific institutions shall be collected ; (Academies) impose upon themselves the practice of reminding every twenty-five or thirty years governments, favourable to the advance of navigation, of the importance of an under- taking whose great cosmical importance depends on its long continued repetition. * Cosmos, pp. 184 186. t Op. at., p. 175.
- Page 323 and 324: 668 COSMOS. plied, and as Christian
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- Page 331 and 332: 676 COSMOS. closely bears upon the
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- Page 335 and 336: 680 COSMOS. feelings of those natio
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- Page 339 and 340: 684 COSMOS. Waisselrode of Allen, b
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- Page 349 and 350: 694 COSMOS. fixed in a central poin
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- Page 355 and 356: 700 COSMOS. Laprey in the important
- Page 357 and 358: 702 COSMOS. he first directed towar
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- Page 361 and 362: 706 COSMOS. 1610, Galileo informed
- Page 363 and 364: 708 COSMOS. descent lime-ball appea
- Page 365 and 366: 710 COSMOS. cised a happy influence
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- Page 383 and 384: 728 COSMOS. perature, the alternati
- Page 385 and 386: 730 COSMOS. Men had now discovered
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720 <strong>COSMOS</strong>.<br />
observed at the magnetic stations which, since 1828, have begun<br />
to cover a considerable portion of the earth's surface, both in<br />
northern and southern latitudes;* but four times in every century<br />
an expedition of three ships should be sent out, to examine<br />
as nearly as possible at the same time the state of the magnetism<br />
of the earth, so far as it can be investigated in those<br />
parts which are covered by the ocean. The magnetic<br />
equator, or the curve at which the inclination is null, must<br />
not merely be inferred from the geographical position of its<br />
nodes (the intersections with the geographical equator) ; but<br />
the course of the ship should be made continually to vary'<br />
according to the observations of inclination, so as' never to<br />
leave the tract of the magnetic equator for the time being.<br />
Land expeditions should be combined with these voyages, in<br />
order, where masses of land cannot be entirely traversed, to<br />
determine at what points of the coast-line the magnetic<br />
curves (especially those having no variation) enter. Special<br />
attention might also perhaps be deservedly directed to the<br />
movement and gradual changes in the oval configuration, and<br />
almost concentric curves of variation of the two isolated<br />
closed systems in Eastern Asia, and in the South Pacific in<br />
the meridian of the Marquesas Group.f Since the memo-<br />
rable Antarctic expedition of Sir James Clarke Ross, (1839<br />
1843,) fitted out with admirable instruments, has thrown so<br />
much light over the polar regions of the southern hemisphere,<br />
and has determined empirically the position of the magnetic<br />
south pole ; and since my honoured friend, the great mathematician,<br />
Frederick Gauss, has succeeded in establishing the<br />
first general theory of terrestrial magnetism, we need not<br />
renounce the hope that the many requirements of science and<br />
navigation will lead to the realisation of the plan I have<br />
already proposed. May the year 1850 be marked as the first<br />
normal epoch in -which the materials for a magnetic chart<br />
and may permanent scientific institutions<br />
shall be collected ;<br />
(Academies) impose upon themselves the practice of reminding<br />
every twenty-five or thirty years governments, favourable to<br />
the advance of navigation, of the importance of an under-<br />
taking whose great cosmical importance depends on its long<br />
continued repetition.<br />
* Cosmos, pp. 184 186.<br />
t Op. at., p. 175.