Personal Narrative Of Travels To The Equinoctial Regions Of America During The Years 1799-1804 - Volume 1 - By Alexander Von Humboldt And Aime Bonpland.
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The Quantity Of Light Received On
That Part Of The Sea Where The Visual Ray Terminates; And The
Extinction Of The Reflected Light During Its Passage Through The
Intermediate Strata Of Air.
It may happen, notwithstanding the
serenity of the sky and the transparency of the atmosphere, that
the ocean is
Feebly illuminated at thirty or forty leagues'
distance; or that the strata of air nearest the earth may
extinguish a great deal of the light, by absorbing the rays that
traverse them.
The rounded peak, or western dome of the Silla, concealed from us
the view of the town of Caracas; but we distinguished the nearest
houses, the villages of Chacao and Petare, the coffee plantations,
and the course of the Rio Guayra, a slender streak of water
reflecting a silvery light. The narrow band of cultivated ground
was pleasingly contrasted with the wild and gloomy aspect of the
neighbouring mountains. Whilst contemplating these grand scenes, we
feel little regret that the solitudes of the New World are not
embellished with the monuments of antiquity.
But we could not long avail ourselves of the advantage arising from
the position of the Silla, in commanding all the neighbouring
summits. While we were examining with our glasses that part of the
sea, the horizon of which was clearly defined, and the chain of the
mountains of Ocumare, behind which begins the unknown world of the
Orinoco and the Amazon, a thick fog from the plains rose to the
elevated regions, first filling the bottom of the valley of
Caracas. The vapours, illumined from above, presented a uniform
tint of a milky white. The valley seemed overspread with water, and
looked like an arm of the sea, of which the adjacent mountains
formed the steep shore. In vain we waited for the slave who carried
Ramsden's great sextant. Eager to avail myself of the favourable
state of the sky, I resolved to take a few solar altitudes with a
sextant by Troughton of two inches radius. The disk of the sun was
half-concealed by the mist. The difference of longitude between the
quarter of the Trinidad and the eastern peak of the Silla appears
scarcely to exceed 0 degrees 3 minutes 22 seconds.* (* The difference
of longitude between the Silla and La Guayra, according to Fidalgo,
is 0 degrees 6 minutes 40 seconds.)
Whilst, seated on the rock, I was determining the dip of the
needle, I found my hands covered with a species of hairy bee, a
little smaller than the honey-bee of the north of Europe. These
insects make their nests in the ground. They seldom fly; and, from
the slowness of their movements, I should have supposed they were
benumbed by the cold of the mountains. The people, in these
regions, call them angelitos (little angels), because they very
seldom sting. They are no doubt of the genus Apis, of the division
melipones. It has been erroneously affirmed that these bees, which
are peculiar to the New World, are destitute of all offensive
weapons. Their sting is indeed comparatively feeble, and they use
it seldom; but a person, not fully convinced of the harmlessness of
these angelitos, can scarcely divest himself of a sensation of
fear. I must confess, that, whilst engaged in my astronomical
observations, I was often on the point of letting my instruments
fall, when I felt my hands and face covered with these hairy bees.
Our guides assured us that they attempt to defend themselves only
when irritated by being seized by their legs. I was not tempted to
try the experiment on myself.
The dip of the needle at the Silla was one centesimal degree less
than in the town of Caracas. In collecting the observations which I
made during calm weather and in very favourable circumstances, on
the mountains as well as along the coast, it would at first seem,
that we discover, in that part of the globe, a certain influence of
the heights on the dip of the needle, and the intensity of the
magnetical forces; but we must remark, that the dip at Caracas is
much greater than could be supposed, from the situation of the
town, and that the magnetical phenomena are modified by the
proximity of certain rocks, which constitute so many particular
centres or little systems of attraction.* (* I have seen fragments
of quartz traversed by parallel bands of magnetic iron, carried
into the valley of Caracas by the waters descending from the
Galipano and the Cerro de Avila. This banded magnetic iron-ore is
found also in the Sierra Nevada of Merida. Between the two peaks of
the Silla, angular fragments of cellular quartz are found, covered
with red oxide of iron. They do not act on the needle. This oxide
is of a cinnabar-red colour.)
The temperature of the atmosphere varied on the summit of the Silla
from eleven to fourteen degrees, according as the weather was calm
or windy. Every one knows how difficult it is to verify, on the
summit of a mountain, the temperature, which is to serve for the
barometric calculation. The wind was east, which would seem to
prove that the trade-winds extend in this latitude much higher than
fifteen hundred toises. Von Buch had observed that, at the peak of
Teneriffe, near the northern limit of the trade-winds, there exists
generally at the elevation of one thousand nine hundred toises, a
contrary current from the west. The Academy of Sciences recommended
the men of science who accompanied the unfortunate La Perouse, to
employ small air-balloons for the purpose of ascertaining at sea
the extent of the trade-winds within the tropics. Such experiments
are very difficult. Small balloons do not in general reach the
height of the Silla; and the light clouds which are sometimes
perceived at an elevation of three or four thousand toises, for
instance, the fleecy clouds, called by the French moutons, remain
almost fixed, or have such a slow motion, that it is impossible to
judge of the direction of the wind.
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