In a subsequent communication, Herr
Magnus treats of the reflection of heat radiated at the surfaces of fluor-spar and other
bodies.
Having succeeded in obtaining the heat
from different substances at 150° C free from the rays of flames and other thermogenic
bodies, and afforded proof that there are some substances which emit waves of one or but
few lengths, while others present them in more frequent variety, it next appeared
interesting to solve the problem how bodies behave with reference to reflective power;
whether, in bodies which act -similarly upon light, differences parallel to those which
are observed in respect of the absorption and transmission of heat do not also occur in
its reflection.
Differences in reflective power are
unmistakably apparent only when rays are reflected which have a uniform, or but slightly
varying, length. Such rays have already been derived either from a section of the spectrum
furnished by a rock-salt prism, or by transmitting the rays from a source of heat of many
wave-lengths through substances which absorb a number of them. There are, however, but
very few bodies that transmit rays of only one or few wave-lengths; moreover, such rays,
obtained by either method, have a very low intensity.
In spite of this difficulty, MM. de la
Provostaye and Desains showed, as early as 1849, that different quantities of the heat
from a Locatelli's lamp were reflected from speculum metal, silver and platinum, according
as it had been conducted through glass or rocksalt; and, for reflecting surfaces of all
kinds, less in the case of glass than in that of rock-salt.
Soon afterwards, by an extended series
of experiments, and employing the prismatically dispersed heat of a lamp, it was proved
by the same physicists that heat from the different portions of the spectrum is
differently reflected. But, doubtless in consequence of the low intensity of the incident
heat, their researches had reference solely to reflection by means of metallic surfaces.
Now, if in rock-salt we possess a substance that emits waves of only one or but few
lengths, and are acquainted with other bodies which, at 150° C, also radiate but a few
kinds, researches can be instituted on reflection at non-metallic surfaces. It has thus
appeared that the different kinds of heat or wave-lengths are reflected from such surfaces
in very different proportions. One of the most striking examples may here be adduced: it
refers to the reflective power of fluor-spar.
Of the heat radiated by a great variety
of substances, unequal (though but slightly differing) amounts were reflected at an angle
of 45°; being in the case of
Silver between 83 and 90 per cent.
Glass between 6 and 14 per cent.
Rock-salt between 5 and 12 per cent.
Fluor-spar between 6 and 10 per cent.
But of the heat from rock-salt,
fluor-spar reflected 28 to 30 per cent., whereas silver, glass, and rock-salt returned no
more of this heat than in the preceding cases.
Here, too, it was evident, as in the
experiments on thermic transmission, that sylvine emits, besides a large quantity of the
rock-salt kind, species of heat of another nature. Fluor-spar reflects 15 to 17 per cent.
of the heat from sylvine; less, consequently, than that from rock-salt, and more than that
from the other radiating bodies.
Granted an eye that could distinguish
different wave-lengths of heat in the same manner as wave-lengths of light, and when the
waves from rock-salt are incident upon different bodies, fluor-spar will appear to it
brighter than any. If the rays are derived from sylvine, fluor-spar would seem still
brighter than all the above bodies, but not so bright as when submitted to the rock-salt
rays.
Melloni has shown that different
substances transmit heat in very unequal proportions, and that the source of heat has a
marked influence on the facility of transmission. Still, the sources of heat were only
distinguished by degree; it was merely recognised that an increased temperature
corresponds to increased variability of wave length. It now appears that at one and the
same temperature, and that-viz, 150 ° C -- far below incandescence, different substances emit
very different kinds of heat, and that, within such a range, an extraordinarily large
number of different heat-rays or wave-lengths continually intermingle. This manifold
intermixture is particularly furthered by the selective reflection taking place at the
different surfaces.
It follows from what has been said that
an eye capable of discerning the different wave-lengths of heat, as it can now
discriminate the colours of light, would perceive, with very little warmth to itself,
every possible variety of tint in surrounding objects.