磁暴主相的形成同微粒流的速度关系密切，但同微粒流密度的关系不大。
The formation of the storm's main phase is closely related to the velocity of the corpuscular stream, while the relation with the density of stream, is poor.
据初步估计，我们的计算与帕克尔等的理论结果相符，并可以解释磁暴主相。
With a suitable choice of the parameter of the solar wind and the capture probability, our result may explain fairly well the theoretical investigation of Parker and others.
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