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The charged particles flow outward from the corona of the sun, follow its magnetic field lines and disperse as far as Saturn. On their way, they collide with gas molecules and cause the molecules to emit light, for example over Earth they form the northern and southern lights.
The charged particles flow outward from the corona of the sun, follow its magnetic field lines and disperse as far as Saturn. On their way, they collide with gas molecules and cause the molecules to emit light, for example over Earth they form the northern and southern lights.