Thermonuclear fusion is a process that takes place all over the universe in the cores of stars. The light nuclei of atoms fuse together, releasing large amounts of energy. To fuse, the atoms need to overcome the repulsive electrostatic forces that act between their positively charged nuclei. This can be achieved, for example, by high temperatures or by external forces pushing them together.
Lecture Inertial Confinement Fusion: [ Ссылка ]
Other Fusion Energy Courses: [ Ссылка ]
0:00 Inertial Confinement Fusion
0:06 Thermonuclear Fusion
0:37 Magnetic Confinement
0:46 Inertial Confinement
1:26 Target
3:14 Driver
4:59 National Ignition Facility
8:50 Direct and Indirect Drive
10:23 Fast Ignition
11:20 Inertial Fusion Power Plant Concepts
12:33 HYLIFE II
12:53 Magneto-Inertial Fusion
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