Absorption line

Definition and stakes

Portrait of Cecilia Payne-Gaposchkin Cecilia Payne-Gaposchkin,  Stellar atmospheres (1925)

“ Production of the maximum of an absorption line. Ordinates are logarithms of computed fractional concentrations; abscissae are temperatures in thousands of degrees. The curves reproduced are those for the Mg + line at 4481. The upper broken curve represents the fraction of magnesium atoms that is singly ionized at the corresponding temperature; the lower broken curve represents the fraction of the Mg + atoms present that is in a suitable state for the absorption of 4481. ”
Source: Gutenberg

Portrait of Cecilia Payne-Gaposchkin Cecilia Payne-Gaposchkin,  Stellar atmospheres (1925)

“ The suggestions that were put forward in the chapter just quoted indicate that different lines, at their maxima, arise from different “effective levels,” the more abundant atoms appearing, other things being equal, at higher levels.
As an absorption line is traced through the classes adjacent to the one at which it attains maximum, it begins to diminish in intensity, owing to the decrease in the number of suitable atoms. If the line is very intense, the first effect of the fall in the number of suitable atoms is a reduction in the width and wings.
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Source: Gutenberg

Portrait of Arthur Schuster Arthur Schuster,  1911 Encyclopædia Britannica, Volume 25… (1911)

“ A. Kundt, [62] who initiated this line of investigation, came to the conclusion that the absorption spectra of certain organic substances like cyanin and fuchsin were displaced towards the red by the solvent, and that the displacement was the greater the greater the dispersive power of the solvent. This law cannot be maintained in its generality, but nevertheless highly dispersive substances like carbon bisulphide are always found to produce a greater shift than liquids of smaller dispersion like water and alcohol. ”
Source: Wikisource

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