Preliminary determination of the wave-lengths of the hydrogen lines, derived from photographs taken at ovar at the eclipse of the Sun, 1900, May 28
The spectrum of the “flash” obtained in observations of solar eclipses furnishes a method of determining the wave-lengths of the hydrogen series with great accuracy, as these lines are strongly shown and sharply defined. As the determination of these wave-lengths is somewhat removed from the general...
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| Veröffentlicht in: | Proceedings of the Royal Society of London 1901-09, Vol.68 (442), p.33-35 |
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| Format: | Artikel |
| Sprache: | eng |
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| Online-Zugang: | Volltext |
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| Zusammenfassung: | The spectrum of the “flash” obtained in observations of solar eclipses furnishes a method of determining the wave-lengths of the hydrogen series with great accuracy, as these lines are strongly shown and sharply defined. As the determination of these wave-lengths is somewhat removed from the general subject of eclipse spectroscopy, it seemed suitable for a separate paper. |
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| ISSN: | 0370-1662 2053-9126 |
| DOI: | 10.1098/rspl.1901.0009 |