Meteorology: The Science of the AtmosphereTalman, Charles Fitzhugh
Science
Meteorology: The Science of the Atmosphere
Talman, Charles Fitzhugh
Meteorology
is, on the whole, well justified for the following reasons: We see the
rainbow where rain is falling, while the sun is shining in the opposite
part of the sky. Our rainstorms usually come from the west and pass
away to the east. A morning rainbow can only be seen in the west, and
indicates that rain is approaching us. An evening rainbow (ignoring
lunar bows) is seen only in the east, and shows that the rain area is
receding from us, giving place to clear skies.
[Illustration: THE CIRCUMZENITHAL ARC
(_From a drawing by L. Besson in La Nature._)
Parts of the halos of 22° and 46°, upper tangent arc of the 22° halo,
and two parhelia are also shown. The circumzenithal arc is always
brightly colored.]
Ice crystals in the atmosphere, such as those composing the higher
clouds, produce a great variety of optical phenomena, known as _halos_.
Some phenomena of this class are common, others exceedingly rare.
Moreover, there are several theoretically possible forms of halo
of which observations have never yet been reported, so that halo
observing can be recommended to the amateur meteorologist as offering
opportunities for making interesting discoveries.
Halos take the form of narrow rings of definite angular size around
the sun or moon (not to be confused with the coronas, of variable
dimensions, described below), rings passing through the luminary, arcs
in various other positions, and roundish spots of colored or white
light. They may be seen separately or in combination. In rare cases,
a dozen or more different forms of halo are visible at the same time,
producing a most spectacular display. One of the most remarkable
displays of this kind in the history of science was seen, in different
degrees of development, over the eastern United States on November 1
and 2, 1913; an event which greatly stimulated interest in the study
of halos in this country. Complex halos are quite common in the polar
regions; where they are seen not only in the sky, but also in the air,
charged with ice particles, close to the earth.
Whenever a thin veil of cirrus or cirro-stratus clouds overspreads the
sky there is a likelihood that halos will be visible. Those formed
near the sun, however, frequently pass unnoticed, on account of the
dazzling brightness of that luminary. Smoked or tinted glasses greatly
facilitate their observation.
[Illustration: DIAGRAMS OF THE PRINCIPAL FORMS OF HALO
(_After Besson, Monthly Weather Review, July, 1914._)
Public-domain text, read in full here on John Shaqi.
Reviews
Reviews
No reviews yet
Be the first to share your thoughts on this work.
Elsewhere in the archive
Join the Discussion
Join the discussion
Sign in to leave a comment or review.
Sign InorCreate an account