Assuming that the solar wind can be modeled with the equations as in slide 1.3-a (page 17 of the pdf) of CM6 (assuming negligible collisions), then we can state that:

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The magnetic field generated by the sun is transported with the plasma

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Using these equations we can estimate the distribution function of solar wind particles in phase space

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The density of the solar wind can be neglected in the calculation of the solar wind dynamics because Maxwell equations are sufficient

Crowdly

Assuming that the solar wind can be modeled with the equations as in slide 1.3-a...

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