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Fusion energy: Progress, partnerships, and the path to deployment
Over the past decade, fusion energy has moved decisively from scientific aspiration toward a credible pathway to a new energy technology. Thanks to long-term federal support, we have significantly advanced our fundamental understanding of plasma physics—the behavior of the superheated gases at the heart of fusion devices. This knowledge will enable the creation and control of fusion fuel under conditions required for future power plants. Our progress is exemplified by breakthroughs at the National Ignition Facility and the Joint European Torus.
L. J. Wittenberg, J. F. Santarius, G. L. Kulcinski
Fusion Science and Technology | Volume 10 | Number 2 | September 1986 | Pages 167-178
Technical Paper | Fusion Fuel Cycles | doi.org/10.13182/FST86-A24972
Articles are hosted by Taylor and Francis Online.
An analysis of astrophysical information indicates that the solar wind has deposited an abundant, easily extractable source of 3He onto the surface of the moon. Apollo lunar samples indicate that the moon's surface soil contains ∼109 kg of 3He. If this amount of 3He were to be used in a 50% efficient D-3He fusion reactor, it would provide 107 GW(electric)-yr of electrical power. The energy required to extract 3He from the lunar regolith and transport it to earth is calculated to be ∼2400 GJ/kg. Since the D-3He reaction produces 6 × 105 GJ of energy per kilogram of 3He, the energy payback ratio is ∼250. Implications for the commercialization of D-3He fusion reactors and for the development of fusion power are discussed.