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
2006
Aufsatz (Zeitschrift)
Englisch
BKL: | 55.60 Raumfahrttechnik / 39.00 Astronomie: Allgemeines / 50.93 Weltraumforschung | |
Lokalklassifikation TIB: | 770/3520/8000 |
Multipoint observations of sharp boundaries of solar wind density structures
Springer Verlag | 2006
|Sharp boundaries of solar wind plasma structures and their relationship to solar wind turbulence
Online Contents | 2007
|Sharp Boundaries of Solar Wind Plasma Structures and an Analysis of Their Pressure Balance
Springer Verlag | 2005
|Sharp Boundaries of Solar Wind Plasma Structures and an Analysis of Their Pressure Balance
Online Contents | 2005
|