Changes in cosmic ray intensity observed on CORONAS-I satellite during magnetic storms in April 1994

Details Changes in cosmic ray intensity observed on CORONAS-I satellite during magnetic storms in April 1994 Changes in cosmic ray intensity observed on CORONAS-I satellite during magnetic storms in April 1994

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....9.3520b&link_type=abstract

Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int

Physics

Scientific paper

The energetic charged particles (Ep > 70 MeV and Ee> 55 MeV) were measured by SONG instrument on board low altitude polar-orbiting CORONAS-I satellite. The interplanetary shock arrivals on 3-4 April 1994 (Dst=111 nT) and 17 April 1994 (Dst=-201 nT) caused significant variations of fluxes of the energetic charged particles detectable on altitude of CORONAS-I satellite. The latitudinal dependence of these effects has been investigated separately for south and north of the minimum L equator on 500 km. The comparison with changes in the cutoff rigidities calculated by Smart et al. (1999a) is done.

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