Auroræ: Their Characters and SpectraCapron, J. Rand
History
Auroræ: Their Characters and Spectra
Capron, J. Rand
Auroras
There is, however, one point to which I desire to draw attention, which
is this, that common to both the Doctor’s and my own Geissler spectrum I
found the before-mentioned rather bright line between γ and α. This line
I found no equivalent for in either of the carbon-tubes. For spectra of
coal-gas and oxygen-tubes, see Plate XIV. spectra 2, 3, & 4.
[Sidenote: Tube- and flame-spectra of carbon do not correspond.]
In comparing the spectra, it should be remembered that the tube- and
flame-spectra of carbon do not correspond. Compare, for instance, the
spectrum of coal-gas or CO₂ in tube, and the well-known lines or bands
in the blue base of a candle-flame. The sharper edge of the yellow
line or band of the carbon-tubes will be found about midway between
the two bright yellow candle-lines or bands. The first of the very
beautiful group of lines or bands in the green in the candle-flame
falls considerably behind the sharper edge of the green line or band
in the tube, while the third bright band in the tube, alone of the
three, corresponds with a very faint band in the candle-flame. A line
or band in the violet in the tube-spectrum finds no equivalent in the
candle-spectrum. For comparison of the carbon-tube and flame spectra (the
principal lines of the tube being alone shown), see Plate XVI. spectra 6
& 7.
[Sidenote: Prof. Piazzi Smyth’s measurements of the components of the
citron-band in a coal-gas flame.]
_Note._—Prof. Piazzi Smyth has been good enough, at my instance, to
measure the components of the citron band of the carbo-hydrogen spectrum
(near Ångström’s Aurora-line), as seen in a coal-gas blowpipe-flame urged
with common air.
The spectroscope used had prisms giving 22° of dispersion between A and
H, and the observing telescope magnified 10 times. The following is a
table of the results communicated to me by the Professor:—
Reading of
Intensity. Micrometer.
Reference line, lithium β 4 16·55
” sodium, α1 10 18·45
” ” α2 10 18·51
Citron band. Carbo-hydrogen.
Line 1, exquisitely clear 6 21·28
2, ” 5 21·88
3, ” 3 22·44
4, faint but clear 2 22·95
5, faint 1 23·38
6, faint and hazy 1 23·70
7, doubtful ? 23·92
Reference line, thallium α 10 25·08
[Sidenote: Comparison of Dr. Vogel’s O lines and Dr. Watts’s
carbon-lines.]
From Dr. Watts’s ‘Index of Spectra’ I have extracted the three principal
carbon-tube bands or lines; and they compare with Dr. Vogel’s oxygen-tube
as under:—
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