A Popular History of Astronomy During the Nineteenth Century: Fourth EditionClerke, Agnes M. (Agnes Mary)
History
A Popular History of Astronomy During the Nineteenth Century: Fourth Edition
Clerke, Agnes M. (Agnes Mary)
Astronomy -- History -- 19th century
The opinion of the Kew observers as to the nature of such disturbances
was strongly swayed by another curious result of the "statistical
method" of inquiry. They found that of 1,137 instances of spots
accompanied by faculæ, 584 had those faculæ chiefly or entirely on the
left, 508 showed a nearly equal distribution, while 45 only had faculous
appendages mainly on the right side.[455] Now the rotation of the sun,
as we see it, is performed from left to right; so that the marked
tendency of the faculæ was a lagging one. This was easily accounted for
by supposing the matter composing them to have been flung upwards from a
considerable depth, whence it would reach the surface with the lesser
_absolute_ velocity belonging to a smaller circle of revolution, and
would consequently fall behind the cavities or "spots" formed by its
abstraction. An attempt, it is true, made by M. Wilsing at Potsdam in
1888[456] to determine the solar rotation from photographs of faculæ had
an outcome inconsistent with this view of their origin. They
unexpectedly gave a uniform period. No trace of the retardation poleward
from the equator, shown by the spots, could be detected in their
movements. But the experiment was obviously inconclusive;[457] and M.
Stratonoff's[458] repetition of it with ampler materials gave a full
assurance that faculæ rotate like spots in periods lengthening as
latitude augments.
The ideas of M. Faye were, on two fundamental points, contradicated by
the Kew investigators. He held spots to be regions of _uprush_ and of
heightened temperature; they believed their obscurity to be due to a
_downrush_ of comparatively cool vapours. Now M. Chacornac, observing,
at Ville-Urbanne, March 6, 1865, saw floods of photospheric matter
visibly precipitating themselves into the abyss opened by a great spot,
and carrying with them small neighbouring maculæ.[459] Similar instances
were repeatedly noted by Father Secchi, who considered the existence of
a kind of _suction_ in spots to be quite beyond question.[460] The
tendency in their vicinity, to put it otherwise, is _centripetal_, not
_centrifugal_; and this alone seems to negative the supposition of a
central uprush.
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