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Cross sections for excitation by proton impact are necessary for quantitative interpretation of auroral spectra. These have been measured for excitation resulting when protons of a few kev energy shoot into low-pressure nitrogen. Interference filters select various spectral features and a photomultiplier detects the light emitted. The light-detection apparatus is calibrated against a standard tungsten filament lamp. The measured cross sections are not for the excitation of a given molecular level, but for a process resulting in the emission of one photon in a given transition. Cross sections measured include: the 0,0 first negative band of N₂⁺, λ3912; the 2,0 Meinel band of N₂⁺, λ7850; a group of N i lines around λ8216; the Balmer line H_β; and the (4,2) and (3,1) first positive bands of N₂, excited by impact of fast atoms. Results are presented graphically, covering the range 1.5 to 4.5 kev. Also included are measurements of the total charge-exchange cross section for protons in nitrogen and an estimate of the ionization cross section.
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Carleton et al. (1958) studied this question.
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