A rocket measurement of O(1S) and N2(+) emissions in a pulsating aurora

Computer Science – Sound

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Auroral Spectroscopy, Emission Spectra, Nitrogen, Optical Emission Spectroscopy, Oxygen Spectra, Atmospheric Chemistry, Energy Transfer, Molecular Excitation, Reaction Kinetics, Rocket Sounding

Scientific paper

Rocket measurements of the O(1S-1D) 557.7-nm and N2(+)(B2Sigma u - X2 Sigma g +) (0-0) 391.4-nm emission profiles for the steady component of an international brightness coefficient 1+ aurora, which exhibited irregular pulsations, are presented. The N2(+) volume emission profile is found to be in good agreement with theoretical profiles calculated from the primary-electron energy spectra recorded near apogee on the same flight. The O(1S) emission is found to increase with altitude relative to the N2(+) emission between 100 and 130 km, and possible mechanisms for the excitation of O(1S) are examined. It is found that either energy transfer from N2(A3Sigma u +) or the reaction of N(+) with O2 can explain most of the observed O(1S) emission, but the possibility of a different excitation mechanism cannot be ruled out.

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