Laboratory absorption strengths for HD 4-0 and 5-0 lines of astronomical interest

Details Laboratory absorption strengths for HD 4-0 and 5-0 lines of astronomical interest Laboratory absorption strengths for HD 4-0 and 5-0 lines of astronomical interest

Jan 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980icar...41..142m&link_type=abstract

Icarus, vol. 41, Jan. 1980, p. 142-146.

Physics

1

Absorption Spectra, Deuterium, Gas Giant Planets, Planetary Atmospheres, Absorption Spectroscopy, Abundance, Line Spectra, Planets, Jovian Planets, Absorption, Density, Temperatures, Atmosphere, Wavelengths, Intensity, Experiments, Analysis, Data, Spectrum, Deuterium, Abundance, Solar System, Isotopes, Parameters, Equipment, Procedure

Scientific paper

Selected lines in the 4-0 and 5-0 bands of HD have been studied with
absorption paths up to 80 m and densities up to 0.76 amagat at
laboratory temperature. The strengths of these lines are of particular
interest in the study of the atmospheres of the outer planets.

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