Blurring of lines at the limit of the hydrogen series

Details Blurring of lines at the limit of the hydrogen series Blurring of lines at the limit of the hydrogen series

Jan 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979afz....15..155k&link_type=abstract

(Astrofizika, vol. 15, Jan.-Mar. 1979, p. 155-163.) Astrophysics, vol. 15, no. 1, July 1979, p. 93-98. Translation.

Astronomy and Astrophysics

Astrophysics

1

Astrophysics, H Lines, Hydrogen Plasma, Line Spectra, Spectral Line Width, Background Radiation, Balmer Series, Blurring, Doppler Effect, Electron Density (Concentration), Light Scattering, Stark Effect

Scientific paper

An expression is obtained for determining the electron density in a hydrogen plasma on the basis of the last observable line in the Balmer series. The expression is derived for the case of line broadening by the Stark effect (ions + electrons) and the Doppler effect when the observations are made in the presence of background radiation that reduces the line contrast.

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