Computer Science
Scientific paper
Aug 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993kosis..31...87z&link_type=abstract
Kosmicheskie Issledovaniia, Tom 31, Vyp. 4, p. 87 - 100
Computer Science
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.
Avanov Levon A.
Borodkova N. L.
Yukhnevich Yu.
Zastenker Georgy N.
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