MAGNETIC VARIATIONS.

Let us now see whether we cannot assign an adequate cause for the

secular and periodic variations in the inclination and declination of

the needle. These have been generally referred to changes of

temperature, as in fact, also, the magnetism of the earth is sometimes

ascribed to galvanic or electric currents, called forth by a daily

change of temperature. Our theory gives a totally different explanation

of these variations.

In the northern hemisphere, the north point of the needle moves from

east to west in the morning from about 8 1/2 A.M. to 1 1/2 P.M., and

returns to its mean position about 10 P.M. It then passes over to the

east, and again returns to its mean position about 8 or 9 A.M. The

analogy of this motion, with the horary changes in the barometer,

indicate a common origin. Humboldt, in the instructions he drew up for

the Antarctic Expedition under Sir James Ross, says: "The phenomena

of periodical variations depend manifestly on the action of _solar

heat_, operating probably through the medium of thermo electric currents

induced on the earth's surface. Beyond this rude guess, however,

_nothing is yet known of their physical cause_. It is even still a

matter of speculation whether the solar influence be a principal or only

a subordinate cause." That the sun may exert a modifying influence on

the phenomenon is not unlikely, but that he cannot be the principal

cause, is evident from the following considerations. These horary

variations of the magnetic needle are as great at the bottom of deep

mines far removed from solar influence, as on the surface. They are as

great, _ceteris paribus_ on a small island in the midst of the ocean, as

in the interior of continents, where the heating power of the surface is

vastly greater. They are extremely regular, so that between the tropics,

according to the sagacious Humboldt, "the time of the day may be known

by the direction of the needle, as well as by the height of the

barometer."

But what is the cause of these variations? This question is the most

difficult of all physical problems, and we shall only aim at indicating

the causes which are yet perhaps too intricately involved to afford a

positive numerical determination. Admitting the existence of two

principal solid masses whose general direction is from south to north,

and that these masses are more susceptible of permeation by the ethereal

fluid than the waters in which they are suspended, we have a general

solution of the position of the magnetic poles, and of the isogonic,

isoclinic, and isodynamic lines. Considering, too, that the southern

poles of these masses are the points of ingress, and the northern poles

the points of egress, it is easily understood that the ethereal medium

having the temperature of space, will cause the southern hemisphere to

be colder than the northern, and also that the magnetic poles will be

the poles of maximum cold, and the centres respected by the isothermal

and isogeothermal lines.

The general direction of the magnetism of the earth may be considered as

the controlling influence, therefore, in determining the position of the

magnetic needle; but there are other causes which, to some extent, will

modify the result. That half of the globe turned away from the sun will

partake of the density of the ether at that distance, which is greater

than on the side next the sun; the magnetic intensity ought, therefore,

to be greater in the night than in the day. The poles of the great

terrestrial magnets, or even the position of a magnetic needle on the

surface, are continually placed by the earth's rotation in a different

relation to the axes of the terral vortex, and the tangential current,

which is continually circulating around the globe, has its inclination

to a given meridian in a perpetual state of change. If we conceive that

there is a tendency to force the needle at right angles to this current,

we shall have an influence which varies during the day, during the year,

and during the time occupied by a complete revolution of the node. The

principal effect, however, of the horary variation of the needle is due

to the radial stream of the sun, which not only penetrates the

atmosphere, but also the solid crust of the earth. Its principal

influence is, however, an indirect influence, as we shall endeavor to

explain.

No fact in the science of electro-magnetism is, perhaps, better

established than the disposition of an ethereal current to place itself

at right angles to the magnetic meridian, and conversely, when the

current is not free to move, to place the needle at right angles to the

current. Now, the terrestrial magnet or magnets, may be considered to be

surrounded by a body of ether in rotation, which, in the earth, on its

surface, and for some distance from the surface, is made to conform to

the general rule, that is, to circulate at right angles to the magnetic

meridian. Outside this again, the ether more and more conforms to the

position of the axis of the vortex, and this position varying, it must

exert _some_ influence on the surface currents, and, therefore, change

in some degree the position of the magnetic meridian. The radial stream

comes from the sun in parallel lines, and strikes the globe and its

superficial ethereal envelope just as we have shown its action on the

atmosphere; but in this last case the magnetic equator is not a great

circle, neither can we suppose its effects to be an accumulation of a

fluid which is imponderable at points 90d from the plane passing through

the centre of the earth and sun, and coincident with the plane of the

central meridian, and a depressing effect on that meridian. Its precise

influence must be, from the nature of the cause, to deflect the circular

current towards the poles, in places less than 90d from the meridian,

and a contrary effect must be produced in places greater than 90d from

the meridian. Let us assume, for argument's sake, that the magnetic

poles of the earth correspond to the poles of rotation, the parallels of

latitude will, therefore, represent the ethereal currents circulating

around the globe. Now, at sunrise, the radial stream of the solar vortex

is tangential to the surface, and, therefore, can produce no change in

these currents. As the sun ascends say about 8 or 9 A.M., the radial

stream striking only the surface of the earth perpendicularly in that

place where the sun is vertical (which we will suppose at the equator),

streams off on every side, as the meridians do from the pole, and the

circles of latitude (that is the ethereal currents) being parallel to

the equator, they are met by the radial stream obliquely, and deflected

towards either pole. By this deflection they are no longer at right

angles to the meridians. But, from the principle of reaction above

noticed, the magnetic meridians will place themselves at right angles to

the current, or, in other words, the magnetic pole will change its

position on the surface of the earth with respect to that particular

place. But, in other parts of the world, the meridians are in opposite

phases at the same instant of absolute time; therefore, the magnetic

poles are not points, but wide areas enclosing the magnetic poles of all

the countries under the sun. As this conforms to observation, it is

worthy our especial attention, and may be understood by the subjoined

figure, in which the oblique curves represent the course of the

tangential current in the different positions of the sun, the parallel

lines representing the solar radial stream.

[Illustration: Fig. 24]

As the sun gains altitude the action of the radial stream is at a

greater and greater angle to the circular currents, and attains its

maximum at noon, still acting, however, after noon; but seeing that the

circular current possesses a force of re-action, that is, that the

magnetism of the earth is ever striving to bring these currents to their

natural direction, an hour or two after noon, the currents tend again to

the equator, and the maximum deflection is passed, and finally ceases a

few hours after sunset. Now let us attend to what is going on on the

opposite side of the world. The radial stream passing over the polar

regions, now produces a contrary effect; the ethereal atmosphere of the

great magnet is accumulated on the farthest side from the sun, by the

action of the radial stream passing over the polar region, the parallel

currents are now bent towards the equator, being at a maximum in places

where it is an hour or two past midnight. Before they were concave to

the equator, and now they are convex; the magnetic meridian is therefore

deflected the contrary way to what it was in the day time, by the same

principle of reaction. After the maximum, say at 4 A.M., the deflection

gradually ceases, and the magnetic meridian returns to its mean position

at 8 or 9 A.M. These times, however, of maximum and minimum, must vary

with the time of the year, or with the declination of the sun, with the

position of the moon in her orbit, with the perigee of the orbit, and

with the place of the ascending node; there are also minor influences

which have an effect, which present instrumental means cannot render

appreciable.

What says observation? The needle declines from its mean position in the

whole northern hemisphere to the westward, from about 8.30 A.M., until

1.30 P.M.; it then gradually returns to its mean position by 10 A.M.

After 10 P.M., it passes over to the eastward, and attains its maximum

deflection about three or four hours after midnight, and is found again

at its mean position about 9 A.M. Now, this is precisely the direction

of the deviation of the magnetic meridian, the needle therefore only

follows the meridian, or still continues to point to the temporary

magnetic pole. And although we have assumed, for the sake of simplicity,

that the mean magnetic pole corresponds to the pole of rotation; in

truth there are two magnetic poles, neither of which correspond; yet

still the general effect will be the same, although the numerical

verification will be rendered more difficult.

In the southern hemisphere the effect is the reverse, (this southern

hemisphere, however, must be considered separated from the northern by

the magnetic equator, and not by the geographical one,) the needle

declines to the eastward in the morning, and goes through the same

changes, substituting east for west, and west for east. Does observation

decide this to be to be a fact also? Most decidedly it does; and this

alone may be considered a positive demonstration, that the theory which

explains it is true. The contrary deflection of the needle in the

northern and southern hemisphere may be formally proclaimed as utterly

beyond the reach of the common theory of magnetism to explain. This

difficulty arises from considering the needle as the disturbed body

instead of the earth; and also from the fact that the effect of solar

heat must be common to needles in both hemispheres, and act upon similar

poles, and consequently the deflection must be in the same direction.

But a still more capital feature is presented by the discovery of

Colonel Sabine, that the deflection is in contrary directions at the

Cape of Good Hope, at the epoch of the two equinoxes. This arises from

the great angle made by the magnetic meridian at this place, with the

terrestrial meridian--the variation being by Barlow's tables, 30d to the

westward. The sun varies in declination 47d throughout the year. At the

southern solstice, therefore the radial stream strikes the circular

current on the southern side, and deflects it towards the equator,

rendering the declination to the westward in the morning; but at the

northern solstice the radial stream strikes the current on its northern

side, and the deflection is eastward in the morning. And the vicinity of

the Cape of Good Hope is, perhaps, the only part of the world where this

anomaly will obtain; as it is necessary not only that the declination

shall be considerable, but also that the latitude shall not be very

great.

Observation also determines that the amount of the horary variation

increases with the latitude. Near the equator, according to Humboldt, it

scarcely amounts to three or four minutes, whilst it is from thirteen to

fourteen minutes in the middle of Europe. The theory explains this also;

for as the circles recede from the equator, the angles made by their

planes with the direction of the radial stream increases, and hence the

force of deflection is greater, and the effect is proportioned to the

cause. We have also a satisfactory explanation of the fact that there

has not yet been discovered a line of _no variation of horary

declination_ as we might reasonably anticipate from the fact that the

declinations are in _contrary directions_ in the northern and southern

hemisphere. This is owing to the ever-varying declination of the sun.

There would be such a line, no doubt, if the axis of the earth were

perpendicular to the plane of the orbit, and the magnetic pole coincided

with the pole of rotation: for then the equator would be such a line.

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