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
That portion of the carbon which was not taken up by alkaline earths, but
remained mixed with the atmosphere, as carbonic acid, was gradually consumed
by the vegetation of the earlier stages of processes of vegetable life, only
retained the small quantity which it now possesses, and which is not
injurious to the sulphurous vapor have occasioned the destruction of the
species of mollusca and fish which inhabited the inland waters of the
earlier world, and have given rise to the formation of the contorted beds of
gypsum, which have doubtless been frequently affected by shocks of
earthquakes.
Gaseous and liquid fluids, mud, and molten earths, ejected from the craters
of volcanoes, which are themselves only a kind of "intermittent springs,"
rise from the earth under precisely analogous physical relations.*
[footnote] *Humboldt, 'Asie Centrale', t. i., p. 43.
All these substances owe their temperature and their chemical character to
the place of their origin. The 'mean' temperature of aqueous springs is
less than that of the air at the point whence they emerge, if the water flow
from a height; but their heat increases with the depth of the strata with
which they are in contact at their origin. We have already spoken of the
numerical law regulating this increase. The blending of waters that have
come from the height of a mountain with those that have sprung from the
depths of the earth, render it difficult to determine the position of the
'isogeothermal lines'* (lines of equal internal
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terrestrial temperature, when this determination is to be made from the
temperature of flowing springs.
[footnote] *On the theory of isogeothermal (chthonisothermal) lines,
consult the ingenious labors of Kupffer, in Pogg, 'Annalen', bd xv., s. 184,
and bd xxxii., s. 270, in the 'Voyage dans l'Oural', p. 382-298, and in the
'Edinburgh Journal of Science', New Series, vol. iv., p. 355. See, also,
Kamtz, 'Lehrb. der Meteor.', bd. ii., s. 217; and, on the ascent of the
chthonisothermal lines in mountainous districts, Bischof, s. 174-198.
Such at any rate, is the result I have arrived at from my own observations
and those of my fellow-travelers in Northern Asia. The temperature of
springs, which has become the subject of such continuous physical
investigation during the last half century, depends, like the elevation of
the line of perpetual snow, on very many simultaneous and deeply-involved
causes. It is a function of the temperature of the stratum in which they
take their rise, of the specific heat of the soil, and of the quantity and
temperature of the meteoric water,* which is itself different from the
temperature of the lower strata of the atmosphere, according to the
different modes of its origin in rain, snow, or hail.**
[footnote] *Leop. v. Buch, in Pogg., 'Annalen', bd. xii., s. 405.
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