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The vast power radiated by our sun is generated by the fusion process wherein light atoms combine with an accompanying release of energy. In nature, proper conditions for fusion occur only in the interior of stars. Researchers are attempting to produce the conditions that will permit fusion to take place on earth. | |||||||||||||||||||
The United Nations projects an increasing population and increasing energy demands. In order to meet future needs, long-term sustainable energy sources are required. Ideally future energy sources will comprise a mix of energy technologies - solar, renewables, advanced nuclear fission and fusion. | |||||||||||||||||||
Fusion requires energetic collisions of very light elements, usually hydrogen isotopes, resulting in a nuclear reaction that leads to more stable helium nuclei and other byproducts. A net loss of mass results, yielding free energy as given by Einstein's famous equation. | |||||||||||||||||||
![]() There are three basic confinement mechanisms required for fusion reactions: gravitational, inertial, and magnetic. The Tokamak Fusion Test Reactor (TFTR) at Princeton(below left) uses magnetic confinement. | |||||||||||||||||||
![]() Plasma radiation within the Princeton Tokamak during operation. | |||||||||||||||||||
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