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

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

Oct 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994adspr..14..645p&link_type=abstract

Advances in Space Research, vol. 14, no. 10, p. 645-650

Mathematics

2

Magnetic Storms, Mir Space Station, Solar Cosmic Rays, Solar Protons, Angular Distribution, Dosimeters, Geomagnetic Pulsations, Mathematical Models, Radiometers

Scientific paper

Flux 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 antisotropic phase of the events on 19 October 1989 and 23 March 1991 was determined. It was determined that after the development of geomagnetic storms, protons with energies more than 1 GeV were registered.

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