High N emission and absorption lines of the sun. II

Details High N emission and absorption lines of the sun. II High N emission and absorption lines of the sun. II

Feb 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975soph...40..329g&link_type=abstract

Solar Physics, vol. 40, Feb. 1975, p. 329-331.

Physics

2

Absorption Spectra, Emission Spectra, Pressure Broadening, Solar Spectra, Spectral Line Width, Line Spectra, Optical Transition, Recombination Reactions, Solar Magnetic Field, Spectroheliographs, Zeeman Effect

Scientific paper

Considering the electronic pressure broadening of high n solar
recombination lines, an upper wavelength limit of the observable region
of possible lines is derived. The reason that no lines have been
observed is discussed.

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