Physics
Scientific paper
Mar 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985rpspr....q..17s&link_type=abstract
In its USSR Rept.: Space (JPRS-USP-85-003) p 17 (SEE N85-25284 15-12) Transl. into ENGLISH from Geomagnetizm i Aeronomiya (US
Physics
Cosmic Rays, Electromagnetic Pulses, Relativistic Particles, Solar Flares, Atmospheric Effects, Flux Quantization, Ground Stations, Time Response
Scientific paper
A previous work showed that 24 hours before an increase in the flux of relativistic particles from solar flares, pulsations are observed in cosmic rays with periods of 30 to 40, 60 to 90 and less frequently 120 to 160 minutes. Cosmic ray data several hours before the increase in flux of relativistic particles on the Earth generated during solar flares was investigated. Five minute data from stations of the world network were analyzed for several vents. The results show that pulsations before solar flares cannot be caused by the influence of the atmosphere or magnetosphere on the intensity of cosmic rays. This indicates that the pulsations in cosmic rays before solar flares are of interplanetary or solar origin.
Filippov Alexandre T.
Starodubtsev S. A.
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