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

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

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