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.


    Access

    Check access

    Check availability in my library

    Order at Subito €


    Export, share and cite



    Title :

    Multipoint observations of sharp boundaries of solar wind density structures


    Contributors:

    Published in:

    Cosmic Research ; 44 , 6 ; 493-499


    Publication date :

    2006-12-01


    Size :

    7 pages




    Type of media :

    Article (Journal)


    Type of material :

    Electronic Resource


    Language :

    English




    Multipoint observations of sharp boundaries of solar wind density structures

    Zastenker, G. N. / Riazantseva, M. O. / Eiges, P. E. | Online Contents | 2006



    Sharp boundaries of solar wind plasma structures and their relationship to solar wind turbulence

    Riazantseva, M.O. / Khabarova, O.V. / Zastenker, G.N. et al. | Elsevier | 2007


    Sharp Boundaries of Solar Wind Plasma Structures and an Analysis of Their Pressure Balance

    Riazantseva, M. O. / Khabarova, O. V. / Zastenker, G. N. et al. | Springer Verlag | 2005


    Sharp Boundaries of Solar Wind Plasma Structures and an Analysis of Their Pressure Balance

    Riazantseva, M. O. / Khabarova, O. V. / Zastenker, G. N. et al. | Online Contents | 2005