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Jon Christian reports that nuclear fusion, the reaction that powers stars like our Sun, could be a source of nearly unlimited electricity. But before that can happen, scientists need to find a way to stabilize super-heated plasma in fusion reactions. Now, researchers (physicists) from Princeton University and the Department of Energy (DOE) think they’ve figured it out — and the technique could prove useful for an experimental European reactor scheduled to go online in 2025.

Magnetic Islands
The work, described in a new paper published in the journal Physical Review Letters, deals with a type of structure in plasma that researchers call a “magnetic island.” Magnetic islands can cause complex plasma disruptions capable of shutting down fusion experiments and even damaging reactors. The researchers found that by bombarding plasma with radio-frequency waves while creating small fluctuations in its temperature, they could stabilize the material and prevent the dangerous magnetic islands from forming.

ITER Saw
The Princeton and DOE researchers believe the new work could be useful at the International Thermonuclear Experimental Reactor (ITER), a huge international project that fusion researchers hope will pave the way for practical fusion power when it goes online in about five years. “There is worry about islands getting large and causing disruptions in ITER,” Allan Reiman, a Princeton researcher who worked on the new stabilization project, said in a statement. “Taken together, these new effects should make it easier to stabilize ITER plasmas.”

For more, see (here).

Remember, the fusion process needs fuel (Helium-3) for example, and that's one of the reasons China is now on the Moon, i.e., to see if the backside of the Moon has similar Helium-3 in the regolith as does the front facing Earth that is known to contain Helium-3. This may help them decide where to build a base on the front or the back, which is safer because the Moon would block radiation coming from our Sun.

For more on Helium-3 on the Moon, see: (here).

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