Line shape of the non-thermal 6300 A O/1D/ emission

Details Line shape of the non-thermal 6300 A O/1D/ emission Line shape of the non-thermal 6300 A O/1D/ emission

May 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982p%26ss...30..457s&link_type=abstract

Planetary and Space Science, vol. 30, May 1982, p. 457-461.

Computer Science

Sound

6

Line Shape, Metastable Atoms, Nonthermal Radiation, Oxygen Spectra, Satellite Sounding, Addition Theorem, Altitude Simulation, Distribution Functions, Dynamics Explorer Satellites, Emission Spectra, Fabry-Perot Interferometers, Legendre Functions, Line Of Sight, Oxygen Recombination, Spherical Harmonics, Zenith

Scientific paper

The two-population model of Schmitt, Abreu and Hays (1981) is used to calculate the line shape of the atomic oxygen metastable state, nonthermal O(1D) 6300 A emission, in order to simulate observations made from a space platform at different zenith angles and altitudes. The Addition theorem, for spherical harmonics of a Legendre polynomial expansion of the nonthermal population distribution function, is used to obtain nonthermal line shapes observed at zenith angles other than the local vertical one.

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