Heinrich Kayser

Kayser was born at Bingen am Rhein. Kayser's early work was concerned with the characteristics of acoustic waves.^[3] He discovered the occurrence of helium in the Earth's atmosphere in 1868 during a solar eclipse when he detected a new spectral line in the solar spectrum. In 1881, Kayser coined the word "adsorption". Together with Carl Runge, he examined the spectra of chemical elements.^[4][5][6] This included the determination of the wavelengths, brightness and sharpness of 4500 lines from the spectrum of iron, an element chosen to act as the standard, as well as 2000 lines for carbon, since iron was vaporised in a carbon arc. The work was later extended to other elements and they developed empirical formulas for the inverse of the wavelength of the type: ${\displaystyle \lambda ^{-1}=A+Bm^{-2}+Cm^{-4}}$, where ${\displaystyle A,B,C}$ are constants and ${\displaystyle m}$ is any positive integer. However, these formulas were superseded by the one by Rydberg. After the conclusion of his collaboration with Runge, he seems to have mostly diverted his research from spectroscopy.^[7] In 1905, he wrote a paper on electron theory.^[8]

The kayser unit, associated with wavenumber, of the CGS system was named after him, with his early recognition of the importance of the inverse wavelength measurements in vacuum rather than in air cited as a reason.^[9] He died at Bonn in 1940.

• Lehrbuch der Physik für Studierende . Enke, Stuttgart 3rd ed. 1900 Digital edition by the University and State Library Düsseldorf