Astronomical DiscoveryTurner, H. H. (Herbert Hall)
History
Astronomical Discovery
Turner, H. H. (Herbert Hall)
Astronomy -- History
And here I must admit that this is about as far as
we have got at present in the investigation of this relationship. _Why_
the needle behaves in this way we have as yet only the very vaguest ideas;
suggestions of different kinds have certainly been put forward, but none
of them as yet can be said to have much evidence in favour of its being
the true one. For our present purpose, however, it is sufficient to note
that there is this very real connection, and that consequently Schwabe's
sun-spot period may have a very real importance with regard to changes in
our earth itself.
[Illustration:
GREENWICH MAGNETIC CURVES
1859-60
PLATE XIII.
GREENWICH MAGNETIC CURVES FOR APRIL 1841-1860]
[Sidenote: Illustration of spurious connection.]
But I may perhaps repeat the word of caution already uttered against
extending without sufficient evidence this notion of the influence of
sun-spots to other phenomena, such as weather. A simple illustration will
perhaps serve better than a long argument to show both the way in which
mistakes have been made and the way in which they can be seen to be
mistakes. There is at the Royal Observatory at Greenwich an instrument for
noting the direction of the wind, the essential part being an ordinary
wind-vane, the movements of which are automatically recorded on a sheet of
paper. As the wind shifts from north to east the pencil moves in one
direction, and when it shifts back again towards the north the pencil
moves in the reverse way. But sometimes the wind shifts continuously from
north to east, south, west, and back to north again, the vane making a
complete revolution; and this causes the pencil to move continuously in
one direction, until when the vane has come to north again, the pencil is
far away from the convenient place of record; on such occasions it is
often necessary to replace it by hand. Then again, the vane may turn in
the opposite direction, sending the pencil inconveniently to the other
side of the record. During the year it is easy to count the number of
complete changes of wind in either direction, and subtracting one number
from the other, we get the excess of complete revolutions of the vane in
one direction over that in the other. Now if these rather arbitrary
numbers are set down year by year, or plotted in the shape of a diagram,
we get a curve which may be compared with the sun-spot curve, and during a
period of no less than sixteen years--from 1858 to 1874--there was a
remarkable similarity between the two diagrams. From this evidence _alone_
it might fairly be inferred that the sun-spots had some curious effect
upon the weather at Greenwich, traceable in this extraordinary way in the
changes of the wind. But the particular way in which these changes are
recorded is so arbitrary that we should naturally feel surprise if there
was a real connection between the two phenomena; and fortunately there
were other records preceding these years and following them which enabled
Public-domain text, read in full here on John Shaqi.
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