Astronomy in a nutshell : $b The chief facts and principles explained in popular language for the general reader and for schoolsServiss, Garrett Putman
Science
Astronomy in a nutshell : $b The chief facts and principles explained in popular language for the general reader and for schools
Serviss, Garrett Putman
Astronomy -- Juvenile literature
=5. Dip of the Horizon.= Another correction which has to be applied in
many observations depends upon the sphericity of the earth. We have
described the rational horizon, and pointed out how it differs from the
sensible horizon. We have also said that at sea the sensible horizon
nearly accords with the rational horizon (see Part I, Sect. 3). But the
accord is not complete, owing to what is called the dip of the horizon.
In fact, the sea horizon lies below the rational horizon by an amount
varying with the elevation of the eye above the surface. Geometry
enables us to determine just what the dip of the horizon must be for any
given elevation of the eye. A rough and ready rule, which may serve for
many purposes, is that the square root of the elevation of the eye in
feet equals the dip of the horizon in minutes of arc, or of angular
measure. The reader will readily see that the dip of the horizon is a
necessary consequence of the rotundity of the earth. It is because of
this that, as a ship recedes at sea her hull first disappears below the
horizon, and then her lower sails, and finally her top-sails. The use of
a telescope does not help the matter, because a telescope only _sees
straight_, and cannot bend the line of sight over the rim of the
horizon. Atmospheric refraction, however, enables us to see an object
which would be hidden by the horizon if there were no air. In
navigation, which, as a science, is an outgrowth of astronomy, these
things have to be carefully taken into account.
[Illustration:
_Fig. 8. Dip of the Horizon._
It is to be remembered that it is the _sensible_ horizon which dips,
and not the _rational_ horizon. The sensible horizon of the observer
at the elevation A dips below the horizontal plane and he sees round
the curved surface as far as a; in other words his skyline is at a.
The observer at the elevation B has a sensible horizon still more
inclined and he sees as far as b. If the observation were made from
an immense height the observer would see practically half round the
earth
just as we see half round the globe of the moon.
]
[Illustration:
Polar Streamers of the Sun, Eclipse of 1889
]
[Illustration:
The Solar Corona at the Eclipse of 1871 From drawings.
]
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