GALACTIC COSMIC-RAY FLUX SIMULATION AND PREDICTIONстатья
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Дата последнего поиска статьи во внешних источниках: 29 мая 2015 г.
Аннотация:A dynamic galactic cosmic ray model is proposed to quantitatively describe the z = 1-28 ions and electrons of E = 10-10(5) MeV/nucleon and their particle flux variations around the Earth's orbit and beyond the Earth's magnetosphere due to diverse large-scale variations of solar activity factors. The variations of targe-scale heliospheric magnetic fields and the galactic cosmic ray flux variation time delays relative to solar activity variations are simulated. The lag characteristics and sunspot number predictions having been determined in detail, the model can be used to predict galactic cosmic ray flux levels.