The Trouvelot astronomical drawings manualTrouvelot, E. L. (Etienne Leopold)
Science
The Trouvelot astronomical drawings manual
Trouvelot, E. L. (Etienne Leopold)
Astronomy -- Pictorial works
It seems to be a well observed fact, that during auroras, a strong
sulphurous odor prevails in high northern latitudes. According to Dr.
Hjaltalin, during these phenomena, "the ozone of the atmosphere
increases considerably, and men and animals exposed out of doors emit a
sulphurous odor when entering a heated room." The Esquimaux and other
inhabitants of the northern regions assert that great auroras are
sometimes accompanied by crepitations and crackling noises of various
sorts. Although these assertions have been denied by several travelers
who have visited the regions of these phenomena, they are confirmed by
many competent observers. Dr. Hjaltalin, who has heard these noises
about six times in a hundred observations, says that they are especially
audible when the weather is clear and calm; but that when the atmosphere
is agitated they are not heard. He compares them to the peculiar sound
produced by a silk cloth when torn asunder, or to the crepitations of
the electric machine when its motion is accelerated. "When the auroral
light is much agitated and the streamers show great movements, it is
then that these noises are heard at different places in the atmosphere."
The spectrum of the auroral light, although it varies with almost every
aurora, always shows a bright green line on a faint continuous spectrum.
In addition to this green line I have frequently observed four broad
diffused bands of greater refrangibility in the spectra of some auroras.
In two cases, when the auroras appeared red towards the west, the
spectrum showed a bright red line, in addition to the green line and the
broad bands described. These facts evidently show that the light of the
aurora is due to the presence of luminous vapors in our atmosphere; and
it may reasonably be supposed that these vapors are rendered luminous by
the passage of electric discharges through them.
THE ZODIACAL LIGHT
PLATE V
In our northern latitudes may be seen, on every clear winter and spring
evening, a column of faint, whitish, nebulous light, rising obliquely
above the western horizon. A similar phenomenon may also be observed in
the east, before day-break, on any clear summer or autumn night. To this
pale, glimmering luminosity the name of "Zodiacal Light" has been given,
from the fact that it lies in the zodiac along the ecliptic.
In common with all the celestial bodies, the zodiacal light participates
in the diurnal motion of the sky, and rises and sets with the
constellations in which it appears. Aside from this apparent motion, it
is endowed with a motion of its own, accomplished from west to east, in
a period of a year. In its motion among the stars, the zodiacal light
always keeps pace with the Sun, and appears as if forming two faint
luminous wings, resting on opposite sides of this body. In reality it
extends on each side of the Sun, its axis lying very nearly in the plane
of the ecliptic.
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