Frolov S G
Kosm Biol Aviakosm Med. 1983 May-Jun;17(3):18-23.
This paper presents the principal characteristics of solar cosmic radiation events in the 20th and 21st cycles of solar activity. 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 Sun southern hemisphere is significantly lower than of the northern hemisphere in both the 20th and the 21st cycles. Empirical distributions of standard characteristics of the SCR proton intensity profile and regression relations have been derived. They can be used to predict radiation parameters of SCR events.
本文介绍了太阳活动第20和21周期中太阳宇宙辐射事件的主要特征。已获得了关于太阳宇宙辐射的一组统一数据。对质子强度时间剖面的大规模变化分析表明，这些变化与取决于行星际激波的行星际磁场结构有关。在第20和21周期中，太阳南半球的相对“质子”地球有效性显著低于北半球。已得出太阳宇宙辐射质子强度剖面标准特征的经验分布和回归关系。它们可用于预测太阳宇宙辐射事件的辐射参数。
