The last resolvable line in the hydrogen spectrum

Details The last resolvable line in the hydrogen spectrum The last resolvable line in the hydrogen spectrum

Aug 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974sva....18..526k&link_type=abstract

(Astronomicheskii Zhurnal, vol. 51, July-Aug. 1974, p. 892, 893.) Soviet Astronomy, vol. 18, Jan.-Feb. 1975, p. 526, 527. Trans

Astronomy and Astrophysics

Astronomy

3

Electron Density (Concentration), Hydrogen Plasma, Line Spectra, Plasma Diagnostics, Spectral Resolution, Doppler Effect, H Lines, Plasma Density, Spectral Line Width, Stark Effect

Scientific paper

A formula is derived which makes it possible to determine the electron
concentration in a plasma from the number of the extreme resolved line
when there is line broadening from the combined Stark effect and the
Doppler effect. The formula is applied to a series of hydrogen line
shapes, and the conditions for its validity are discussed.

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