10 5 30 Scarcely visible; bank in north faint.

This aurora was due to the _inner vortex ascending_, whose period was at

this time 28 days.

There are several circumstances to be observed in this case. The bow

brightened and faded simultaneously with the aurora, and respected the

vertex of the auroral bank, being apparently concentric with it. The

bow, therefore, depends on the same cause, but differs from the aurora

in being limited to the _surface_ of the atmosphere in which the vortex

has produced a wave to the southward of its central path, as may be

understood by inspecting Fig. 2, Sec. 1,--the figure representing the

polar current of the central vortex. On the 29th of May, 1840,[32] the

author saw a similar phenomenon, at the same time of night, and passing

over the same stars southward until it reached within 5d of Jupiter and

Saturn, to which it was parallel. This atmospheric wave offers a greater

resistance to the passage of the ether: hence the light. On this account

it is, also, that when the passage of a vortex is attended by an auroral

display there will be no thunder-storm. There may be an increase of

wind; but the atmosphere at such times is too dry to make a violent

storm, and there is a silent restoration of the equilibrium, by the

ether passing through the dry atmosphere, without meeting any

condensable vapor, and becoming luminous on account of the greater

resistance of the air when unmixed with vapor. We thus see also the

connection between the aurora and the linear cirri, and we have a

triumphant explanation of the fact, that when the observer is north of

the northern limit of the vortices, he sees the aurora to the south and

not to the north; for, to see it to the northward, he would have to see

it in the same latitude as it appears in the south, and, consequently,

have to see across twice the complement of the latitude. We thus see,

also, why the temperature falls after an aurora; for, the passage of

electricity in any shape, must have this effect on account of the great

specific caloric of this fluid. We see, also, why the aurora should be

more frequent where the magnetic intensity is greatest and be

consequently invisible at the equator, and why the magnetic needle is so

sensibly affected at the time of its occurrence. We may, perhaps, here

be allowed to allude to another phenomenon connected with terrestrial

magnetism and electricity.

Outlines of a mechanical theory of storms · 第 92 / 118 题