Physics
Scientific paper
Jul 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983rpsba..17...22f&link_type=abstract
In its USSR Rept.: Space Biol. and Aerospace Med., Vol. 17, No. 3, May - Jun. 1983 (JPRS-83828) p 22-29 (SEE N83-35606 23-51)
Physics
Interplanetary Space, Proton Flux Density, Radiation Hazards, Solar Cosmic Rays, Solar Flares, Energy Spectra, Solar Cycles, Space, Spectrum Analysis, Time Functions
Scientific paper
The principal characteristics of solar cosmic radiation events in the 20th and 21st cycles of solar activity are discussed. A uniform row of data concerning solar cosmic radiation has been obtained. An analysis of large-scale variations of the proton intensity time profile has demonstrated that the variations are associated with the structure of the interplanetary magnetic field which depends on interplanetary shock waves. The relative proton geoeffectiveness of the Empirical distributions of standard characteristics of the solar cosmic (SCR) radiation proton intensity profile and regression relations are derived. They are used to predict radiation parameters of SCR events.
No associations
LandOfFree
Evaluation of statistical characteristics of solar cosmic radiation flares in twentieth and twenty-first cycles of solar activity does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Evaluation of statistical characteristics of solar cosmic radiation flares in twentieth and twenty-first cycles of solar activity, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Evaluation of statistical characteristics of solar cosmic radiation flares in twentieth and twenty-first cycles of solar activity will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1628821