Laboratory absorption strengths for the H2 /4,0/ and /3,0/ S/1/ lines

Details Laboratory absorption strengths for the H2 /4,0/ and /3,0/ S/1/ lines Laboratory absorption strengths for the H2 /4,0/ and /3,0/ S/1/ lines

Nov 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978apj...225l.157t&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 225, Nov. 1, 1978, p. L157-L160. Research supported by the Research

Astronomy and Astrophysics

Astrophysics

3

Absorption Spectra, Gas Giant Planets, Hydrogen, Line Spectra, Molecular Absorption, Planetary Atmospheres, Space Environment Simulation, Space Laboratories

Scientific paper

Long-path absorption measurements of the (3,0) and (4,0) S(1) quadrupole lines of molecular hydrogen have been made, yielding an accurate experimental line strength for the (4,0) line and confirming previous estimates for the (3,0) line. The H2 (4,0) S(1) line is significantly weaker than theoretical predictions, a result of importance to our understanding of the atmospheres of the outer planets.

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