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  2. History of nuclear fusion - Wikipedia

    en.wikipedia.org/wiki/History_of_nuclear_fusion

    The first successful man-made fusion device was the boosted fission weapon tested in 1951 in the Greenhouse Item test. The first true fusion weapon was 1952's Ivy Mike, and the first practical example was 1954's Castle Bravo. In these devices, the energy released by a fission explosion compresses and heats the fuel, starting a fusion reaction.

  3. Artificial hair integrations - Wikipedia

    en.wikipedia.org/wiki/Artificial_hair_integrations

    These bond attachments generally last 4–6 weeks before a maintenance appointment is necessary. Fusion method involves a machine similar to a hot glue gun used to attach human hair extensions to individual strands of one's natural hair of about 1/8 to 1/4 inch squared sections for a truly authentic look. Another option for fusion attachments ...

  4. Fusion 360 - Wikipedia

    en.wikipedia.org/wiki/Fusion_360

    In 2009, the tech demo Inventor Fusion was released. In the summer of 2013, Fusion 360 was publicly announced as a cloud-enabled version of the original. [9] In January 2024, Fusion was rebranded, dropping the '360' from the previous product name 'Fusion 360'. [10] After release, other Autodesk products were integrated into Autodesk Fusion:

  5. Nuclear fusion enters ‘new era’ after major breakthrough for ...

    www.aol.com/news/nuclear-fusion-enters-era-major...

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  6. List of fusion experiments - Wikipedia

    en.wikipedia.org/wiki/List_of_fusion_experiments

    10-beam NIR and frequency-tripled 351 nm UV laser; fusion yield of 10 13 neutrons; attempted ignition, but failed due to fluid instability of targets; led to construction of NIF: 1.3 PW: 120 kJ: 30 J: Livermore: LLNL: ISKRA-5: Operational-1989: 12-beam iodine gas laser, fusion yield 10 10 to 10 11 neutrons [93] 100 TW: 30 kJ: 0.3 J: Sarov: RFNC ...

  7. Nuclear fusion - Wikipedia

    en.wikipedia.org/wiki/Nuclear_fusion

    This difference in mass arises as a result of the difference in nuclear binding energy between the atomic nuclei before and after the fusion reaction. Nuclear fusion is the process that powers active or main-sequence stars and other high-magnitude stars, where large amounts of energy are released.

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