Meteorology: The Science of the AtmosphereTalman, Charles Fitzhugh
Science
Meteorology: The Science of the Atmosphere
Talman, Charles Fitzhugh
Meteorology
Of its occurrence on Ben Nevis, Angus Rankin writes: “The most frequent
manner in which it makes its appearance is as caps of light on the tips
of the lightning rod, but occasionally it appears as jets of flame
projecting from all objects on the top of the tower and from the cowl
of the kitchen chimney, which rises from the roof at some distance
from the tower. These jets are at times from 4 to 6 inches in length,
and make a peculiar hissing sound. During a very brilliant display,
the observer’s hair, hat, pencil, etc., are aglow with the ‘fire,’
but, except for a slight tingling sensation in the head and hands, he
suffers no inconvenience from it. On such occasions, if a stick be
raised above the head, jets of electric light will be seen at its upper
end. The only drawback to observing it with advantage is the unpleasant
character of the weather in which it appears, namely blinding showers
of snow and hail, and squally winds, causing a good deal of snowdrift.”
Rankin records that it was sometimes _heard_ in the daytime, when its
light was invisible. On the Sonnblick a display of St. Elmo’s fire has
been observed to last as long as eight hours.
No luminous electrical phenomenon is more beautiful or, at first sight,
more mysterious than the _aurora_, popularly known, in the northern
hemisphere, as the “northern lights.” This phenomenon is due to the
passage of electrical discharges through the rarefied gases of the
upper atmosphere, and it now appears to be settled beyond controversy
that the discharges are caused by corpuscles or radiations of some kind
emitted from the sun.
Most accounts of the aurora describe the typical appearances that it
assumes as seen from a single place on the surface of the earth, but
say little, if anything, about the form of the phenomenon as a whole
or about its position in space. We shall follow a different plan here,
and ask the reader, first of all, to imagine himself viewing the aurora
from a point some thousands of miles away from our planet.
The solar emission above mentioned, when sufficiently intense, produces
in the upper atmosphere a glow like that seen in a vacuum tube when
an electrical discharge passes through it. From our vantage point in
outer space we shall notice that this glow is not spread over the
whole globe, but forms two rings, which encircle the polar regions of
both hemispheres, though neither the geographic nor the magnetic poles
lie at their centers. The rings do not extend down into the lower
atmosphere, but hang about 60 miles above the earth’s surface.
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