Auroræ: Their Characters and SpectraCapron, J. Rand
History
Auroræ: Their Characters and Spectra
Capron, J. Rand
Auroras
| N. | VN. | VN. | | |
-------------+--------+------+------+------+------+------+--------+------
* No results in the examined spectra; but see Plate XIII. fig. 2.
** Too uncertain in position for comparison (see Plate XIII. fig. 1).
Tested by coincidence, or close proximity of lines to those of the
Aurora, we arrange the spectra in the following order:—(1) iron, (2)
air-spark, (3) hydrogen, (4) air-tube, (5) phosphoretted hydrogen, (6)
carbon and oxygen.
The air-tube spectrum might perhaps stand higher in the scale but for its
broad bands, which make comparison doubtful. Lines of oxygen possibly
escape detection in the Aurora from the faint character of its spectrum.
The phosphorus and iron spectra are especially interesting in connexion
with Professor Nordenskiöld’s “metallic and magnetic cosmic dust in the
Polar regions” (see Phil. Mag. ser. 4, vol. xlviii. p. 546).
[Sidenote: Additional Table of compared spectra.]
As an addendum to the foregoing, on Plate IX. fig. 1 will be found a
Table I have prepared, in which a type Aurora and also Vogel’s and
Barker’s Auroræ are compared with eight other spectra, viz.:—
S. Solar spectrum.
N. Nitrogen (air): Watts.
O. Oxygen (air): Watts.
C.H. Carburetted-hydrogen vacuum-tube: Watts.
C.I. Carburetted-hydrogen flame: Watts.
C.C. Blue base of candle-flame: Capron.
O.P. Oxygen vacuum-tube: Procter.
I. Iron: Watts.
The divisions and vertical lines will guide the eye in making comparison
of the spectra.
CHAPTER XII.
SOME NOTES ON PROFESSOR ÅNGSTRÖM’S THEORY OF THE AURORA-SPECTRUM.
[The substance of these appeared in the ‘Philosophical
Magazine’ for April 1875, in conjunction with the “Comparison
of the Tube and other Spectra” (Chapter XI.), but they are now,
for the sake of convenience, made a separate article.]
[Sidenote: Professor Ångström’s propositions.]
In a contribution by the late Professor Ångström to a solution of the
problem of the Aurora-spectrum (an abstract of which appeared in ‘Nature’
of July 16, 1874), the Professor is stated, amongst other things, to have
laid down certain propositions in substance as follows:—
[Sidenote: That the Aurora has two spectra.]
1st. That the Aurora has two different spectra—the one comprising the one
bright line in the yellow-green only, and the other the remaining fainter
lines.
[Sidenote: That bright line does not coincide with HC₂.]
2ndly. That the bright line falls within a group of hydrocarbon lines,
but does not actually coincide with any prominent line of such group, and
that Dr. Vogel’s finding this line to coincide with a not well-marked
band in the air-spectrum must be regarded as a case of accidental
coincidence.
[Sidenote: That moisture is _nil_ in Aurora region.]
3rdly. That moisture in the region of the Aurora must be regarded as
_nil_, and that oxygen and hydrogen must alone there act as conductors of
electricity.
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