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The ribbon of energetic neutral atoms discovered by the Interstellar Boundary Explorer is the brightest feature in the sky at kiloelectronvolt energies, yet its total power is a tiny fraction of the solar wind power that ultimately sustains it. Integrating representative published ribbon fluxes over the ribbon solid angle gives a ribbon power near 8.92e+13 watts against a solar wind kinetic power near 7.53e+19 watts, a fraction of about 1.2e-06. The smallness of the fraction is itself the informative result: the ribbon can be sustained by the secondary charge-exchange process proposed for it without straining the heliosheath energy budget, and even order-of-magnitude errors in the flux integration cannot change that conclusion. The integration is computed from stated published fluxes with the deposited script, not measured here.
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William Alexander Aldred (2026) studied this question.
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