Abstract We investigate the large scale flow pattern of 36–1600 keV protons observed in association with several large interplanetary shocks on ISEE-3 between August 1978 and April 1980. The distribution function in the solar wind frame and its temperal evolution indicates that these particles can behave as a coherent population in the solar wind. This population propagates along the magnetic field in the same direction as the solar wind flow, ahead of the shock, and in the opposite direction after the passage of the perturbed region associated with the shock.


    Zugriff

    Zugriff prüfen

    Verfügbarkeit in meiner Bibliothek prüfen

    Bestellung bei Subito €


    Exportieren, teilen und zitieren



    Titel :

    Low-energy protons associated with interplanetary shocks as an independent population in the solar wind


    Beteiligte:
    Sanahuja, B. (Autor:in) / Domingo, V. (Autor:in)

    Erschienen in:

    Advances in Space Research ; 4 , 2-3 ; 319-322


    Erscheinungsdatum :

    1984-01-01


    Format / Umfang :

    4 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch





    The influence of interplanetary shocks on solar protons measured in the stratosphere

    Bazilevskaya, G.A. / Stozhkov, Yu.I. / Struminsky, A.B. | Elsevier | 1994



    Acceleration of Solar Wind Ions by Oblique Interplanetary Shocks

    Baring, M. G. / Ogilvie, K. W. / Ellison, D. C. et al. | British Library Conference Proceedings | 1995