Auroræ: Their Characters and SpectraCapron, J. Rand
History
Auroræ: Their Characters and Spectra
Capron, J. Rand
Auroras
Dr. Richardson (‘Sir John Franklin’s Narrative’), so long ago as the
years 1819-1822, made many recorded observations on the connexion of
clouds with the Aurora Borealis in the Polar regions. Some of these are
alluded to in Chapter V., section “Height of the Aurora,” for the purpose
of showing the moderate distance he found it to be above the earth; and
his inference is there mentioned, “that the Aurora Borealis is constantly
accompanied by or immediately precedes the formation of one or other
of the various kinds of cirro-stratus.” On the 13th November and 18th
December, 1820, the connexion of an Aurora with a cloud intermediate
between cirrus and cirro-stratus is mentioned. It is, however, also
mentioned that the most vivid coruscations of the Aurora were observed
when there were only a few attenuated shoots of cirro-stratus floating in
the air, or when that cloud was so rare that its existence was only known
by the production of a halo round the moon. (An instance of attenuated
streaks of cirro-stratus in connexion with an auroral arc will be found
in the Aurora seen at Guildown on the 4th February 1874, a sketch of
which is reproduced on Plate VI. fig. 1.)
[Sidenote: Polarity discerned in cirro-stratus clouds.]
Dr. Richardson goes on to express his opinion that he, on some occasions,
discerned a polarity in the masses of clouds belonging to a certain kind
of cirro-stratus (approaching cirrus), by which their long diameters,
having all the same direction, were made to cross the magnetic meridian
nearly at right angles.
[Sidenote: Apparent polarity of Aurora might perhaps be ascribed to the
clouds themselves.]
Dr. Richardson further suggests that if it should be thereafter proved
that the Aurora depends upon the existence of certain clouds, its
apparent polarity might perhaps be ascribed to the clouds themselves
which emit the light; or, in other words, the clouds might assume their
peculiar arrangement through the operation of one cause (magnetism, for
instance), while the emission of light might be produced by another—a
change in their internal constitution perhaps connected with a motion of
the electric fluid.
Dr. Richardson further remarks that, generally speaking, the Aurora
appeared in small detached masses for some time before it assumed that
convergency towards the opposite parts of the horizon which produced the
arched form.
[Sidenote: Sir John Franklin’s observations.]
Sir John Franklin says in his Polar expeditions he often perceived the
clouds in the daytime disposed in streams and arches such as the Aurora
assumes.
[Sidenote: Dr. Low’s.]
Dr. Low (‘Nature,’ iv. p. 121) considers he witnessed a complete display
of auroral motions in cirrus cloud, and considers all clouds subject
to magnetic or diamagnetic polarization; he states that when the lines
converge towards the magnetic pole fine weather follows, and when at
right angles to it wet and stormy.
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