Abstract The results of comparison of the characteristics of sharp boundaries of small-scale and medium-scale solar wind structures in the case of their simultaneous observation on widely spaced spacecraft are described. It is shown that even very sharp boundaries, with duration of several seconds or fractions of a second, retain their amplitude and remain very sharp during solar wind propagation to distances of up to a million kilometers.
Multipoint observations of sharp boundaries of solar wind density structures
Cosmic Research ; 44 , 6 ; 493-499
2006-12-01
7 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
Multipoint observations of sharp boundaries of solar wind density structures
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