Graham's Magazine, Vol. XL, No. 5, May 1852Various
General
Graham's Magazine, Vol. XL, No. 5, May 1852
Various
Literature -- Periodicals; Literature, Modern -- 19th century -- Periodicals
_Paraselenæ._ Mock moons, depending upon the causes which produce the
solar image, or several examples of it, as frequently adorn the arctic
sky. On the 1st of December, 1819, in the evening, while Parry’s
expedition was in Winter Harbor, four paraselenæ were observed, each at
the distance of 21½° from the true moon. One was close to the horizon,
the other perpendicular above it, and the other two in a line parallel
to the horizon. Their shape was like that of a comet, the tail being
from the moon, the side of each toward the real orb being of a light
orange color. During the existence of these paraselenæ, a halo appeared
in a concentric circle round the moon, passing through each image. On
the evening of March 30, 1820, about ten o’clock, the attention of Dr.
Trail, at Liverpool, was directed by a friend to an unusual appearance
in the sky, which proved to be a beautiful display of paraselenæ. The
moon was then 35° above the southern horizon. The atmosphere was nearly
calm, but rather cloudy, and obscured by a slight haze. A wide halo,
faintly exhibiting the prismatic colors, was described round the moon as
a centre, and had a small portion of its circumference cut off by the
horizon. The circular band was intersected by two small segments of a
larger circle, which if completed would have passed through the moon,
and parallel to the horizon. These segments were of a paler color than
the first mentioned circle. At the points of intersection appeared two
pretty well defined luminous discs, equaling the moon in size, but less
brilliant. The western paraselenæ had a tail or coma, which was directed
from the moon, and the eastern also, but less clearly-defined.
_The Rainbow._ The most glorious vision depending upon the
decomposition, refraction, and reflection of light, by the vapor of the
atmosphere reduced to fluid drops, is the well-known arch projected
during a shower of rain upon a cloud opposite to the sun, displaying all
the tints of the solar spectrum. The first marked approximation to the
true theory of the rainbow occurs in a volume entitled _De Radiis Visus
et Lucis_, written by Antonius de Dominis, Archbishop of Spalatro,
published in the year 1611 at Venice. Descartes pursued the subject, and
correctly explained some of the phenomena; but upon Newton’s discovery
of the different degrees of refrangibility in the different colored rays
which compose the sunbeam, a pencil of white or compounded light, the
cause of the colored bands in the rainbow, of the order of their
position, and of the breadth they occupy, was at once apparent. The bow
is common to all countries, and is the sign of the covenant of promise
to all people, that there shall no more be such a wide-spread deluge as
that which the sacred narrative records.
Public-domain text, read in full here on John Shaqi.
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