Auroræ: Their Characters and SpectraCapron, J. Rand
History
Auroræ: Their Characters and Spectra
Capron, J. Rand
Auroras
B. The question of the violet-pole spectrum. Here I make the remark that
in comparing other spectra with that of the Aurora, it is, I think, too
much the practice to trust to the coincidence (more or less perfect) of
one or perhaps two lines out of many; whereas we know by experience that
most spectra have so well-marked a general as well as special character
that, when once seen, they are recognized afterwards with the greatest
ease and without measurements. An experience and proof of this is found
in a set of “Photographed Spectra” which the Autotype Company have
reproduced for me.
[Sidenote: Coincidence of one or two lines not sufficient to establish
identity.]
Of course no two given spectra can be considered identical unless their
principal lines coincide; but, on the other hand, the coincidence
of one or two lines out of many, without other features, cannot be
satisfactorily or conclusively held to establish identity.
[Sidenote: Ångström’s compared spectra.]
In Professor Herschel’s letter (Phil. Mag. ser. 4, vol. xlix. p. 71),
Professor Ångström’s representation of the “spectrum of the glow
discharge round the negative pole of air-vacuum tubes” is given, in
comparison with the Aurora-lines and those of olefiant gas. This
illustration is here introduced.
Ångström’s representation of the Spectrum of the glow discharge round the
negative pole of Air-vacuum tubes, and its comparison with the Spectrum
of the Aurora.
[Illustration: Wave-lengths, in hundred-thousandths of a millimetre.]
It is unfortunate that in this illustration and in Professor Herschel’s
paper the wave-lengths of the Aurora-lines are not given in figures, but
must be roughly calculated from the scale. Professor Herschel speaks of
Ångström’s drawing as representing a _normal_ spectrum, and as derived
from authentic sources, such as Vogel, Barker, and others; but beyond
this we are not certain as to its origin.
In illustration of the difficulty of constructing any thing like a
general typical Aurora-spectrum I append a Table of eight Auroral spectra
taken at hazard:—
[Sidenote: Table of compared Aurora.]
Auroral lines and bands.
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