The first telescopic view of the sun is apt, it must be confessed,
to be a disappointment. The moon is certainly a much more attractive
subject for a casual glance. Its craters and mountain ranges catch
the eye at once, while the solar disc presents an appearance of almost
unbroken uniformity. Soon, however, it will become evident that the
uniformity is only apparent. Generally speaking, the surface will
quickly be seen to be broken up by one or more dark spots (Plate V.),
which present an apparently black centre and a sort of grey shading
round about this centre. The margin of the disc will be seen to be
notably less bright than its central portions; and near the margin,
and oftenest, though not invariably, in connection with one of the
dark spots, there will be markings of a brilliant white, and often of
a fantastically branched shape, which seem elevated above the general
surface; while as the eye becomes more used to its work it will be
found that even a small telescope brings out a kind of mottled or
curdled appearance over the whole disc. This last feature may often
be more readily seen by moving the telescope so as to cause the solar
image to sweep across the field of view, or by gently tapping the
tube so as to cause a slight vibration. Specks of dirt which may have
gathered upon the field lens of the eye-piece will also be seen; but
these may be distinguished from the spots by moving the telescope
a little, when they will shift their place relatively to the other
features; and their exhibition may serve to suggest the propriety of
keeping eye-pieces as clean as possible.
[Illustration: PLATE VI.
Photograph of Bridged Sunspot (Janssen). _Knowledge_, February, 1890.]
Public-domain text, read in full here on John Shaqi.
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