On probing the outer planets with the Raman effect

Details On probing the outer planets with the Raman effect On probing the outer planets with the Raman effect

May 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977rvgsp..15..227p&link_type=abstract

Reviews of Geophysics and Space Physics, vol. 15, May 1977, p. 227-234.

Physics

Optics

4

Molecular Spectra, Planetary Atmospheres, Raman Spectra, Aerosols, Atmospheric Models, Atmospheric Optics, Hydrogen, Jupiter Atmosphere, Molecular Rotation, Neptune (Planet), Rotational Spectra, Uranus (Planet)

Scientific paper

The paper examines the feasibility of using the H2 rotational Raman spectrum to study the physical structure of the atmospheres of the outer planets. Computations of the strengths of the S(0) and S(1) lines are made for a wide range of physical conditions on the basis of a semi-infinite homogeneous pure H2 atmospheric model. Initial applications of the Raman probe technique to Jupiter and Uranus are reported.

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