Solar wind is a continuous flow of particles (mainly helium-hydrogen plasma) rushing into surrounding space out of the corona of the Sun with speeds from 300 to 1200 km/s. The solar wind is not the visible sunlight. The main reason for it occurrence is high temperature of the corona (millions of degrees). However the way it happens is a very complex problem.
The Van-Allen radiation belts are formed by these particles caught and collected in magnetosphere of planets if these particles do not have enough kinetic energy to pass through the magnetosphere.
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