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- W1763801356 abstract "Numerous investigators who have studied the structure of the mercury green line λ 5460.97 A. have found that it consists of a wide central unresolved band, flanked on either side by three or more clearly resolved components that are usually designated as satellites. Janicki has shown, however, and so has Nagaoka, that the central portion of the line can be resolved into well defined components when a Lummer plate of high resolving power is used by itself, or is crossed with another of the same kind, or with a high grade échelon spectrograph. From such investigations it would appear to be definitely settled that the line is produced by twelve separable and distinct wave-lengths. These components, as measured by Nagaoka, are shown in their relative positions, and with approximately their relative intensities, in fig. 1. The values of their relative wave-lengths, as measured by Janicki and Nagaoka, are given in Table I. In their investigations on the structure of the line λ 5460.97 A., Janicki, Prince Galitzin and Wilip, Stansfield and one of the writers found that, when an Heraeus quartz mercury arc lamp was used as the source of light (and also when other forms of lamps were used as well), the structure of the line underwent a profound modification when the radiation was produced by the passage of very heavy electric currents in place of weak ones. Janicki observed, in place of the original line and its satellites, a peculiar system of five equidistant bands, the original components of the line being apparently lost in a continuous spectrum." @default.
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- W1763801356 date "1922-10-02" @default.
- W1763801356 modified "2023-10-16" @default.
- W1763801356 title "On the absorption of λ 5460.97 A. by luminous mercury vapour" @default.
- W1763801356 doi "https://doi.org/10.1098/rspa.1922.0070" @default.
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