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 idea that solar maculation depends in some way upon the position of
the planets occurred to Galileo in 1612.[493] It has been industriously
sifted by a whole bevy of modern solar physicists. Wolf in 1859[494]
found reason to believe that the eleven-year curve is determined by the
action of Jupiter, modified by that of Saturn, and diversified by
influences proceeding from the earth and Venus. Its tempting approach to
agreement with Jupiter's period of revolution round the sun, indeed,
irresistibly suggested a causal connection; yet it does not seem that
the most skilful "coaxing" of figures can bring about a fundamental
harmony. Carrington pointed out in 1863, that while, during _eight
successive periods_, from 1770 downwards, there were approximate
coincidences between Jupiter's aphelion passages and sun-spot maxima,
the relation had been almost exactly reversed in the two periods
preceding that date;[495] and Wolf himself finally concluded that the
Jovian origin must be abandoned.[496] M. Duponchel's[497] prediction,
nevertheless, of an abnormal retardation of the maximum due in 1881
through certain peculiarities in the positions of Uranus and Neptune
about the time it fell due, was partially verified by the event, since,
after an abortive phase of agitation in April, 1882, the final outburst
was postponed to January, 1894. The interval was thus 13.5 instead of
11.1 years; and it is noticeable that the delay affected chiefly the
southern hemisphere. Alternations of activity in the solar hemispheres
were indeed a marked feature of the maximum of 1884, which, in M. Faye's
view,[498] derived thence its indecisive character, while sharp, strong
crises arise with the simultaneous advance of agitation north and south
of the solar equator. The curve of magnetic disturbance followed with
its usual strict fidelity the anomalous fluctuations of the sun-spot
curve. The ensuing minimum occurred early in 1889, and was succeeded in
1894 by a maximum slightly less feeble than its predecessor.[499]
It cannot be said that much progress has been made towards the
disclosure of the cause, or causes, of the sun-spot cycle. No external
influence adequate to the effect has, at any rate, yet been pointed out.
Most thinkers on this difficult subject provide a quasi-explanation of
the periodicity in question through certain assumed vicissitudes
affecting internal processes;[500] Sir Norman Lockyer and E. von
Oppolzer reach the same end by establishing self-compensatory
fluctuations in the solar atmospheric circulation; Dr. Schuster resorts
to changes in the electrical conductivity of space near the sun.[501] In
all these theories, however, the course of transition is arbitrarily
arranged to suit a period, which imposes itself as a fact peremptorily
claiming admittance, while obstinately defying explanation.
Public-domain text, read in full here on John Shaqi.
Reviews
Reviews
No reviews yet
Be the first to share your thoughts on this work.
Elsewhere in the archive
Join the Discussion
Join the discussion
Sign in to leave a comment or review.
Sign InorCreate an account