The Glaciers of the Alps: Being a narrative of excursions and ascents, an account of the origin and phenomena of glaciers and an exposition of the physical principles to which they are relatedTyndall, John
Science
The Glaciers of the Alps: Being a narrative of excursions and ascents, an account of the origin and phenomena of glaciers and an exposition of the physical principles to which they are related
Tyndall, John
Alps -- Description and travel; Glaciers -- Alps
The principle of the method finally applied is all that can here be
referred to; and it, I hope, will be quite intelligible. Two beams of
heat, from two distinct sources, were allowed to fall upon the same
instrument,[A] and to contend there for mastery. When both beams were
perfectly equal, they completely neutralized each other's action; but
when one of them was in any sensible degree stronger than the other, the
predominance of the former was shown by the instrument. It was so
arranged that one of the conflicting beams passed through a tube which
could be exhausted of air, or filled with any gas; thus varying at
pleasure the medium through which it passed. The question then was,
supposing the two beams to be equal when the tube was filled with air,
will the exhausting of the tube disturb the equality? The answer was
affirmative; the instrument at once showed that a greater quantity of
heat passed through the vacuum than through the air.
The experiment was so arranged that the effect thus produced was very
large as measured by the indications of the instrument. But the action
of the simple gases, oxygen, hydrogen, and nitrogen, was incomparably
less than that produced by some of the compound gases, while these
latter again differed widely from each other. Vapours exhibited
differences of equal magnitude. The experiments indeed proved that
gaseous bodies varied among themselves, as to their power of
transmitting radiant heat, just as much as liquids and solids. It was in
the highest degree interesting to observe how a gas or vapour of perfect
transparency, as regards light, acted like an opaque screen upon the
heat. To the eye, the gas within the tube might be as invisible as the
air itself, while to the radiant heat it behaved like a cloud which it
was almost impossible to penetrate.
[Sidenote: SELECTED HEAT.]
Applying the same method, I have found that from the sun, from the
electric light, or from the lime-light, a large amount of heat can be
selected, which is unaffected not only by air, but by the most energetic
gases that experiment has revealed to me; while this same heat, when it
has its _quality_ changed by being rendered obscure, is powerfully
intercepted. Thus the bold and beautiful speculation above referred to
has been made an experimental fact; the radiant heat of the sun does
certainly pass through the atmosphere to the earth with greater
facility than the radiant heat of the earth can escape into space.
[Sidenote: POSSIBLE HEAT OF NEPTUNE.]
Public-domain text, read in full here on John Shaqi.
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