Magnetic Reconnection Heating
A Process of Magnetic Energy Conversion into Kinetic Energy of Particles
Magnetic reconnection is a process in which the topology of magnetic
field lines is explosively reconfigured. It ubiquitously takes place in space and laboratory experiments
where there's plasma, responsible for such physical phenomena as solar flares, coronal mass ejections,
and tokamak sawtooth oscillations. Due to the conservation of energy, the energy stored in magnetic
fields is released and converted into the internal energy of plasma during the rearrangement of magnetic
field lines.
Startorus Fusion harnesses multiple poloidal field coils in the spherical tokamak to produce two
plasma rings via induction and promotes their merging into a primary plasma. In this process,
magnetic fields created by the plasma rings undergo reconnection on a massive scale, heating the
plasma to the temperature necessary for fusion reactions rapidly and efficiently.
Compared with mainstream tokamak approaches, this proposal requires nothing more than several sets
of coils to complete the plasma heating. Therefore, it is far less complicated and difficult than
high-power negative ion sources for neutral beam systems and high-power millimeter wave systems,
with strong economic competitiveness and fewer operational difficulties.