Cosmos: A Sketch of the Physical Description of the Universe, Vol. 1Humboldt, Alexander von
History
Cosmos: A Sketch of the Physical Description of the Universe, Vol. 1
Humboldt, Alexander von
Astronomy; Cosmography; Physical geography; Science -- History
[footnote] ** On the temperature of the drops, of rain in Cumana, which
fell to 72 degrees, when the temperature of the air shortly before had been
86 degrees and 88 degrees, and during the rain sank to 74 degrees, see my
'Relat. Hist.', t. ii., p. 22. The rain-drops, while falling, change the
normal temperature they originally possessed, which depends on the height of
the clouds from which they fell, and their heating on their upper surface by
the solar rays. The rain-drops, on their first production, have a higher
temperature than the surrounding medium in the superior strata of our
atmosphere, in consequence of the liberation of their latent heat; and they
continue to rise in temperature, since, in falling through lower and warmer
strata, vapor is precipitated on them, and they thus increase in size
(Bischof, 'Warmelehre des inneren Erdkorpers' s. 73); but this additional
heating is compensated for by evaporation. The cooling of the air by rain
(putting out of the question what probably belongs to the electric process
in storms) is effected by the drops, which are themselves of lower
temperature, in consequence of the cold situation in which they were formed,
and bring down with them a portion of the higher colder air, and which
finally, by moistening the ground, give rise to evaporation. The cooling of
the air by rain (putting out of the question what probably belongs to the
electric process in storms) is effected by the drops, which are themselves
of lower temperature, in consequence of the cold situation in which they
were formed, and bringi down with them a portion of the higher colder air,
and which finally, by moistening the ground, give rise to evaporation.
These are the ordinary relations of the phenomenon. When, as occasionally
happens, the rain-drops are warmer than the lower strata of the atmosphere
(Humboldt, 'Rel. Hist.', t. iii., p. 513), the cause must probably be sought
in higher warmer currents, or in a higher temperature of widely-extended and
not very thick clouds, from the action of the sun's rays. How, moreover,
the phenomenon of supplementary rainbows, which are explained by the
interference of light, is connected with the original and increasing size of
the falling drops, and how an optical phenomenon, if we know how to observe
it accurately, may enlighten us regarding a meteorological process,
according to diversity of zone, has been shown, with much talent and
ingenuity, by Arago, in the 'Annuaire' for 1836, p. 300.
Public-domain text, read in full here on John Shaqi.
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