Proton aurora on the dayside.

Physics

Scientific paper

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Scientific paper

A simple procedure to evaluate the Balmer excitation rates of Hα and Hβ to produce the corresponding volume emission rates vs. height, using semi-empirical range relations of protons in air is used. The calculations are carried out with identified ion-energy particle spectra of the dayside aurora obtained by low altitude satellites. It is found that the calculated emission intensities of Hα are observable by ground-based optical devices.

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