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The Sun

The energy of the sun comes from fusion of hydrogen nuclei 4H + 2e  He + 5 + 2 (+ 26 MeV). H. Bindingsenergi per nukleon. nukleoner. He. The Sun. E = mc 2 m He &lt; 4m H + 2m e. Every second 4 million tons of mass is converted to energy. Fusion is a universal source of energy.

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In IEA/ITPA CC meeting (November 29-30 at JET, Bruce attended from us),

In IEA/ITPA CC meeting (November 29-30 at JET, Bruce attended from us), 2007 Reports and 2008 Proposals of ITPA/IEA joint multi-machine experiments were circulated and discussed. We would like to appreciate spokes-person's effort to lead the collaboration work.

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