Line shape of the non-thermal 6300 Å O(1D) emission |
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| Authors: | G.A. Schmitt V.J. Abreu P.B. Hays |
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| Affiliation: | Space Physics Research Laboratory, The University of Michigan, Ann Arbor, MI 48109, U.S.A. |
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| Abstract: | The line shape of the non-thermal O(1D) 6300 Å emission is calculated using the two population model of Schmitt, Abreu and Hays (Planet. Space Sci.29, 1095, 1981). The calculated line shapes simulate observations made from a space platform at different zenith angles and altitudes. The non-thermal line shapes observed at zenith angles other than the local vertical have been obtained by using the Addition theorem for spherical harmonics of a Legendre polynomial expansion of the non-thermal population distribution function. |
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