Auroræ: Their Characters and SpectraCapron, J. Rand
History
Auroræ: Their Characters and Spectra
Capron, J. Rand
Auroras
+-----+--------+------------------------------------------------+
|W.L. |Probable| Remarks. |
| | error. | |
+-----+--------+------------------------------------------------+
|6297 | 14 |Very bright stripe. } |
| | | } |
|5569 | 2 |Brightest line of the spectrum, } |
| | | became noticeably fainter at } On a faintly |
| | | appearance of the red line. } lighted |
| | | } ground. |
|5390 | .. |Extremely faint line; } |
| | | unreliable observation. } |
| | | } |
|5233 | 4 |Moderately bright. } |
| | | |
|5189 | 9 |This line was very bright when the red line |
| | | appeared at the same time; otherwise equal |
| | | in brilliancy with the preceding one. |
| | | |
|5004 | 3 |Very bright line. |
| | | |
|4694}| |{Broad band of light, somewhat less brilliant |
|4663}| 3 |{ in the middle; very faint in those parts of |
|4629}| |{ the Aurora in which the red line appeared. |
+-----+--------+------------------------------------------------+
A translation of Dr. Vogel’s interesting paper will be found printed _in
extenso_ in Appendix E, and his lithographed drawings of the spectrum in
the green and red portions of the Aurora respectively on Plate VI. figs.
2 and 3. The observations of April 9th by Dr. Vogel are probably, up to
the present time, the most exact of any one Aurora, and I have therefore
in most cases used them for comparison.
[Sidenote: Mr. Backhouse’s catalogue of lines.]
Mr. Backhouse, in a letter to ‘Nature,’ commenting upon my catalogue
of lines, gave the following as the latest determinations from his own
observations:—
No. 1. Wave-length 6060
2. ” 5660
3. ” 5165
4. ” 5015
6. ” 4625
7. ” 4305
(6060 must be a mistake for 6260, and 5660 for 5560.—J. R. C.) Mr.
Backhouse never saw a line at 5320 again. He found the continuous
spectrum to reach from No. 2 to No. 7, being brightest from a little
beyond No. 2 to No. 6. This part of the spectrum did not give him so much
the idea of a true “continuous spectrum” as of a series of bright bands
too close to be distinguished.
[Sidenote: Subsequent full catalogue of Auroral lines.]
Public-domain text, read in full here on John Shaqi.
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