Lord Kelvin: An account of his scientific life and workGray, Andrew
Science
Lord Kelvin: An account of his scientific life and work
Gray, Andrew
Kelvin, William Thomson, Baron, 1824-1907
Sir William Thomson's electrical and other inventions are too numerous
to specify here, and they are in constant use wherever precision of
measurement is aimed at or required. Long ago he invented electrometers
for absolute measurements of electrical potential ("electric pressure");
more recently his current-balances have given the same precision to
electrodynamic measurement of currents. All his early instruments were
made by Mr. James White, Glasgow. The business founded by Mr. White,
and latterly carried on at Cambridge Street, has developed immensely,
and is now owned by a limited liability company--Messrs. Kelvin and
James White (Limited).
For many years Sir William Thomson was a keen yachtsman, and his
schooner yacht, the _Lalla Rookh_, was well known on the Clyde and in
the Solent. An expert navigator, he delighted to take deep-sea voyages
in his yacht, and went more than once as far as Madeira. Many
navigational and hydrodynamical problems were worked out on these
expeditions. For a good many years, however, he had given up sea-faring
during his times of relaxation, and lived in Glasgow and London and in
Largs, Ayrshire, where he built, in 1875, a large and comfortable house,
looking out towards the Firth and the Argyleshire lochs he knew and
loved so well.
In the course of his deep-sea expeditions in his yacht he became
impressed with the utility of Sumner's method of determining the
position of a ship. Let us suppose that at a given instant the altitude
of the sun is determined from the ship. The Greenwich meantime, and
therefore the longitude at which the sun is vertical, is known by
chronometer, and the declination of the sun is known from the Nautical
Almanac. The point on the earth vertically under the sun can be marked
on the chart, and a circle (or rather, what would be a circle on a
terrestrial globe) drawn round it from every point of which the sun
would have the observed altitude. The ship is at a point on this circle.
Some time after the altitude of the sun is observed again, and a new
"circle" is drawn. If the first "circle" be bodily shifted on the chart
along the distance run in the interval, it will intersect the second in
two points, one of which will be the position of the ship, and it is
generally possible to tell which, without danger of mistake.
Public-domain text, read in full here on John Shaqi.
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