Blackwood's Edinburgh Magazine, Vol. 70, No. 431, September 1851Various
History
Blackwood's Edinburgh Magazine, Vol. 70, No. 431, September 1851
Various
England -- Periodicals; Scotland -- Periodicals
"But it is not the outline only which is thus systematically
false. The drawing of the solid form is worse still; for it
is to be remembered that, although clouds of course arrange
themselves more or less into broad masses, with a light side
and a dark side, both their light and shade are invariably
composed of a series of divided masses, each of which has in
its outline as much variety and character as the great outline
of the cloud; presenting, therefore, a thousand times repeated,
all that I have described as the general form. Nor are these
multitudinous divisions a truth of slight importance in the
character of sky, for they are dependent on, and illustrative
of, a quality which is usually in a great degree overlooked--the
enormous retiring spaces of solid clouds. Between the illumined
edge of a heaped cloud and that part of its body which turns
into shadow, there will generally be a clear distance of several
miles--more or less, of course, according to the general size
of the cloud; but in such large masses as Poussin and others of
the old masters, which occupy the fourth or fifth of the visible
sky, the clear illumined breadth of vapour, from the edge to
the shadow, involves at least a distance of five or six miles.
We are little apt, in watching the changes of a mountainous
range of cloud, to reflect that the masses of vapour which
compose it are linger and higher than any mountain-range of the
earth; and the distances between mass and mass are not yards of
air, traversed in an instant by the flying form, but valleys
of changing atmosphere leagues over; that the slow motion of
ascending curves, which we can scarcely trace, is a boiling
energy of exulting vapour rushing into the heaven a thousand
feet in a minute; and that the topling angle, whose sharp edge
almost escapes notice in the multitudinous forms around it, is
a nodding precipice of storms, three thousand feet from base to
summit. It is not until we have actually compared the forms of
the sky with the hill-ranges of the earth, and seen the soaring
alp overtopped and buried in one surge of the sky, that we begin
to conceive or appreciate the colossal scale of the phenomena of
the latter. But of this there can be no doubt in the mind of any
one accustomed to trace the forms of cloud among hill-ranges--as
it is there a demonstrable and evident fact--that the space of
vapour visibly extended over an ordinarily clouded sky is not
less, from the point nearest to the observer to the horizon,
than twenty leagues; that the size of every mass of separate
form, if it be at all largely divided, is to be expressed in
terms of _miles_; and that every boiling heap of illuminated
mist in the nearer sky is an enormous mountain, fifteen or
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