The whole magnetic system is perpetually undergoing secular and
periodical changes, which are so irregular and complicated that half a
century is sufficient to alter the form and position of all the lines
that have been mentioned. The foci of magnetic intensity, and the whole
system represented by the magnetic lines, are moving along the two
hemispheres in opposite directions; those in the northern hemisphere are
going from west to east, and those in the southern from east to west;
and as the foci of maximum intensity move with different velocities, the
forms, as well as the places, of the curves are slowly, yet continually,
changing. The weaker magnetic focus in the northern hemisphere moved
through 50 degrees of longitude in 250 years.
The declination is subject to periodic variations depending upon the
position of the moon, and to annual variations arising from the motion
of the sun in the ecliptic, as well as to horary variations
corresponding to changes of temperature from the diurnal rotation of the
earth.
Throughout the middle latitudes of the northern hemisphere the north end
of the magnet has a mean motion from east to west from eight in the
morning till half-past one, it then moves to the east till evening,
after which it makes another excursion to the west, and returns again to
its original position at eight in the morning. The extent of its
variation is greater in the day than in the night, in summer than in
winter. It decreases from the middle latitudes in Europe, where it is 13
or 14 minutes, to the equator, where it is only 3 or 4; but at the
equator the variations are performed with extreme regularity. The horary
motions of the south end of the magnet in the southern hemisphere are
accomplished in an exactly opposite direction. Between these two
magnetic hemispheres there is a line passing through an infinity of
places, and very nearly coinciding with the line of minimum magnetic
intensity, where the horary phenomena of both hemispheres are combined,
each predominating alternately at opposite seasons. At St. Helena, which
is one of the places in question, and nearly on the line of minimum
intensity, the horary motion of the north end of the magnet corresponds
in direction during one half of the year with the movement in the
northern hemisphere, and in the other half of the year the direction at
the same hours corresponds with that in the southern hemisphere, the
passage from the one to the other being at the equinoxes, when the
diurnal variations at the usual hours partake more or less of the
characteristics of both on different days.[152]
Public-domain text, read in full here on John Shaqi.
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