AbstractFlux and dose rate dynamics of solar cosmic rays were measured by the Lyulin dosimeter during the events 19 October 1989 and 23 March 1991. The maximum dose rate registered was 0.4, 0.12 and 0.01 cGy/hour, respectively. Based on the latitude distribution of particle flux a power law form for the energy spectra of solar protons in the anisotropic phase of the events on 19 October 1989 and 23 March 1991 was determined. It was obtained that after the development of geomagnetic storm protons with energies more than 1 GeV were registered.


    Zugriff

    Zugriff prüfen

    Verfügbarkeit in meiner Bibliothek prüfen

    Bestellung bei Subito €


    Exportieren, teilen und zitieren



    Titel :

    Peculiarities of the solar proton events of 19 October 1989 and 23 March 1991 according to the measurements onboard the Mir space station


    Beteiligte:
    Petrov, V.M. (Autor:in) / Mahkmtov, V.S. (Autor:in) / Panova, N.A. (Autor:in) / Shurshakov, V.A. (Autor:in) / Dachev, Ts.P. (Autor:in) / Semkova, J.V. (Autor:in) / Matvijchuk, Yu.P. (Autor:in)

    Erschienen in:

    Advances in Space Research ; 14 , 10 ; 645-650


    Erscheinungsdatum :

    01.01.1994


    Format / Umfang :

    6 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch