Meteorology: The Science of the AtmosphereTalman, Charles Fitzhugh
Science
Meteorology: The Science of the Atmosphere
Talman, Charles Fitzhugh
Meteorology
| | (chimney pots and slates |
| | removed) | 50
10 | Whole gale | Seldom experienced inland; |
| | trees uprooted; considerable |
| | structural damage occurs | 59
11 | Storm | Very rarely experienced; |
| | accompanied by widespread |
| | damage | 68
12 | Hurricane | | Above 75
--------+---------------+---------------------------------+-----------
The clouds receive more attention at some weather stations than at
others. A routine observation consists of noting the kinds of clouds
visible, the direction or directions from which they are moving,
and the degree of cloudiness--i. e., the extent to which the sky is
clouded, stated in tenths, from O = cloudless, to 10 = completely
overcast. At many of the more important stations the movements of
clouds are observed with a _nephoscope_. The reflecting nephoscope,
used in this country, consists of a black mirror in which the image of
the moving cloud is watched, the direction of its motion being read off
from the graduated circular frame of the mirror. There is also a device
for measuring the apparent speed of the cloud. From this the actual
speed can be calculated if the height of the cloud is known. There are
other nephoscopes, such as Besson’s in which the cloud’s movements are
watched directly, and not by reflection.
[Illustration: BESSON’S COMB NEPHOSCOPE]
The importance of sunshine among the elements of weather and climate
is evidenced by the fact that at least two States of the Union,
South Dakota and California, contend for the title of “the Sunshine
State”--which does not properly belong to either of them. Arizona is
the sunniest State of all, and the whole Southwest is sunnier than
South Dakota.
Devices for registering the duration of sunshine are called _sunshine
recorders_. One type (the Campbell-Stokes) works on the burning-glass
principle; in others the sun’s rays trace a record on photographic
paper. The instrument used by the Weather Bureau consists of an air
thermometer having a bulb at each end, one bulb being coated with
lampblack. There is a small column of mercury between the two inclosed
masses of air. The thermometer is inclosed in a sheath of glass, from
which the air is exhausted. When the sun shines on this instrument,
the air in the black bulb warms and expands, and the mercury is
forced toward the other bulb until it comes in contact with a pair of
electrodes, thus closing an electrical circuit. While the circuit is
closed, the registering apparatus connected with the instrument makes
a step-shaped mark once every minute. When the sun stops shining, the
mercury drops back, the circuit is broken, and the recording pen merely
traces a straight line.
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