RADIAL DEPENDENCE OF RESIDUAL, 11-YEAR, AND 22-YEAR VARIATIONS IN INTENSITY OF GALACTIC COSMIC RAYS

摘要

Using the data on the intensity of galactic cosmic rays, obtained during the last two solar activity cycles by similar detectors of the network of spacecraft near the Earth and in the distant heliosphere, we reproduce the radial profile of the intensity corresponding to the periods of minimum of the 22nd and 23rd cycles and the maximum of the 22nd cycle. The profile for the 23rd cycle is also determined. An attempt is made to redefine the residual and 11-year variations so that their characteristics would become independent of the 22nd wave of intensity. The radial dependence of all three basic long-term variations in the intensity of galactic cosmic rays is estimated and briefly discussed.