Abstract
Voyager 1 explored the satellite Titan at a solar zenith angle of 73°. Photoelectron fluxes in the atmosphere of Titan for this same angle (73°) have been calculated for an atmospheric model with molecular nitrogen. The Photoelectron impact excitation rates of a′πg and b′πu states of N2 are also calculated.
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More From: Journal of Geophysical Research: Space Physics
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