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Three ways to improve the theory and therefore the understanding of the physical processes in the interplanetary medium (during both quiet and disturbed periods of solar activity) are suggested. They are: (1) the development and consequently the use ofhigher order moments (fluid) equationsas well as of more realisticclosure conditionsandtransport coefficientsfor the macroscopic description of the solar wind ; (2) the undertaking ofcomputer simulation experimentson the nonlinear collectivedoi:10.1017/s0074180900067978 fatcat:75uk4lp3mjdfdkhpfaaqdkzvfm