Auroræ: Their Characters and SpectraCapron, J. Rand
History
Auroræ: Their Characters and Spectra
Capron, J. Rand
Auroras
+-----+---------+--------+-------+-------------------+--------+
|Line.| Reading | Wave- |Assumed| Comments. |Probable|
| |on scale.|lengths.| line. | | error. |
|-----+---------+--------+-------+-------------------+--------|
| 1. | 61 | 5690 | 5570 |Common Aurora-line.| -20 |
| 2. | 68 | 5320 | 5316 | Corona line. | + 1 |
| 3. | 80 | 4850 | 4860 | F, hydrogen. | - 3 |
| 4. | 98 | 4350 | 4340 | G, hydrogen. | + 6 |
+-----+---------+--------+-------+-------------------+--------+
[61 is evidently wrong, and was probably a mistake for 63.]
[Sidenote: G. F. Barker’s observations.]
George F. Barker, observing at New Haven (U.S.A.), saw, on November 9th,
a crimson and white Aurora, which he examined with a single glass-prism
spectroscope, by Duboscq, of Paris. The line positions were obtained by
an illuminated millimetre scale. In the white Aurora were four lines (the
red one being absent); in the red Aurora five. The wave-lengths of the
Aurora-lines were run out as follows:—
(1.) Between C and D, 6230 (Zöllner’s 6270).
(2.) ” D and E, 5620 (Ångström’s 5570).
(3.) ” E and _b_, 5170 (Winlock’s 5200).
(4.) ” _b_ and F, 5020.
(5.) ” F and G, 4820 (Alvan Clarke’s, jun., 4850).
[Sidenote: Spectrum of Aurora of Feb. 4, 1872. Prof. Piazzi Smyth’s
observations.]
Mr. Procter’s Aurora-lines will be found noticed in connexion with the
spectrum of oxygen; and Lord Lindsay’s lines, with a comparison scale
drawing, are separately described further on in this Chapter. The Aurora
of February 4th, 1872, had many observers; some of whom communicated
at the time spectroscopic notes. Professor Piazzi Smyth minutely
describes the display as seen in Edinburgh, and saw “Ångström’s green
Aurora-line perpetually over citron acetylene[13] at W.L. 5579, and the
red Aurora-line between lithium _a_ and sodium _a_, but nearer to the
latter, say at W.L. 6370.” Extremely faint greenish and bluish lines also
appeared at W.L. 5300, 5100, and 4900 nearly.
[Sidenote: Rev. T. W. Webb’s observations.]
The Rev. T. W. Webb, with a very fine slit, saw the green Auroral line
even in the light reflected from white paper. With a wider slit he saw a
crimson band in the brighter patches of that hue, and beyond an extent of
greenish or bluish light, which he suspected to be composed of contiguous
bands.
[Sidenote: R. J. Friswell’s observations.]
R. J. Friswell, coming up the Channel at 9.40, with a Hoffman’s
direct-vision spectroscope (the observing telescope removed), saw the
green line, a crimson line near C, and faint traces of structure in the
blue and violet.
[Sidenote: The Rev. S. J. Perry’s observations.]
Public-domain text, read in full here on John Shaqi.
Reviews
Reviews
No reviews yet
Be the first to share your thoughts on this work.
Elsewhere in the archive
Join the Discussion
Join the discussion
Sign in to leave a comment or review.
Sign InorCreate an account