Radiative association in planetary atmospheres

Details Radiative association in planetary atmospheres Radiative association in planetary atmospheres

Mar 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992p%26ss...40..243d&link_type=abstract

Planetary and Space Science (ISSN 0032-0633), vol. 40, Feb.-Mar. 1992, p. 243-246.

Physics

11

Airglow, Atmospheric Chemistry, Atmospheric Radiation, Emission Spectra, Planetary Atmospheres, Helium, Nitric Oxide, Oxygen Ions, Positive Ions

Scientific paper

A summary account is presented of radiative association processes that may be significant in producing continuum emission in the atmospheres of the planets. The importance of the radiative association of N and O and of NO + O has been established by the presence in the airglow of the emission spectra. The possible contributions of O + O, O + O2 and O(+) + O are discussed. The radiative association of He(+) and H may be an important source of HeH(+) in the Jovian ionospheres.

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