Plasma dynamics in the magnetosheath. I. Behaviour of the main ion components.

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Scientific paper

Some features of solar wind plasma behaviour in the magnetosheath are analysed: a) the shape of the ion distribution function - it is shown that it may be presented as a combination of three populations ("core", "shoulder" and "tail") with different parameters. b) the variability of the distribution functions and hydrodynamic parameters - it is shown that this variability is about an order of magnitude higher than that one in the solar wind. Based on selective measurements a comparison of the characteristics of protons and alpha-particles in the magnetosheath is carried out.

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