Ульяновский государственный педагогический университет имени И.Н.Ульянова

Ульяновский государственный педагогический университет имени И.Н. Ульянова

Magnetic field reconnection is a key process for particle heating and acceleration during solar flares. Turbulence was not accounted for until numerical simulations allowed the exploration of mutually coupled phenomena spanning a broad range of scales.
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